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description Publicationkeyboard_double_arrow_right Article , Other literature type , Preprint 2018 Sweden, Italy, Italy, Italy, Switzerland, United KingdomPublisher:American Astronomical Society Funded by:EC | GAIA-ESO-MWEC| GAIA-ESO-MWMariagrazia Franchini; Carlo Morossi; Paolo Di Marcantonio; Miguel Chavez; Gerry Gilmore; Sofia Randich; Ettore Flaccomio; Sergey E. Koposov; Andreas J. Korn; Amelia Bayo; Giovanni Carraro; Andrew R. Casey; E. Franciosini; A. Hourihane; Paula Jofre; Carmela Lardo; James R. Lewis; Laura Magrini; L. Morbidelli; G. G. Sacco; Clare Worley; Tomaz Zwitter;We present a high resolution synthetic spectral library, INTRIGOSS, designed for studying FGK stars. The library is based on atmosphere models computed with specified individual element abundances via ATLAS12 code. Normalized SPectra (NSP) and surface Flux SPectra (FSP), in the 4830-5400 A, wavelength range, were computed with the SPECTRUM code. INTRIGOSS uses the solar composition by Grevesse et al. 2007 and four [alpha/Fe] abundance ratios and consists of 15,232 spectra. The synthetic spectra are computed with astrophysical gf-values derived by comparing synthetic predictions with a very high SNR solar spectrum and the UVES-U580 spectra of five cool giants. The validity of the NSPs is assessed by using the UVES-U580 spectra of 2212 stars observed in the framework of the Gaia-ESO Survey and characterized by homogeneous and accurate atmospheric parameter values and by detailed chemical compositions. The greater accuracy of NSPs with respect to spectra from the AMBRE, GES_Grid, PHOENIX, C14, and B17 synthetic spectral libraries is demonstrated by evaluating the consistency of the predictions of the different libraries for the UVES-U580 sample stars. The validity of the FSPs is checked by comparing their prediction with both observed spectral energy distribution and spectral indices. The comparison of FSPs with SEDs derived from ELODIE, INDO--U.S., and MILES libraries indicates that the former reproduce the observed flux distributions within a few percent and without any systematic trend. The good agreement between observational and synthetic Lick/SDSS indices shows that the predicted blanketing of FSPs well reproduces the observed one, thus confirming the reliability of INTRIGOSS FSPs. Comment: 32 pages, 12 figures
Edinburgh Research E... arrow_drop_down OA@INAF - Istituto Nazionale di AstrofisicaArticle . 2018Data sources: OA@INAF - Istituto Nazionale di AstrofisicaPublikationer från Uppsala UniversitetArticle . 2018 . Peer-reviewedData sources: Publikationer från Uppsala UniversitetInfoscience - EPFL scientific publicationsOther literature typeData sources: Infoscience - EPFL scientific publicationshttps://doi.org/10.48550/arxiv...Article . 2018License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.euAccess RoutesGreen hybrid 9 citations 9 popularity Top 10% influence Average impulse Top 10% Powered by BIP!visibility 8visibility views 8 download downloads 6 Powered bymore_vert Edinburgh Research E... arrow_drop_down OA@INAF - Istituto Nazionale di AstrofisicaArticle . 2018Data sources: OA@INAF - Istituto Nazionale di AstrofisicaPublikationer från Uppsala UniversitetArticle . 2018 . Peer-reviewedData sources: Publikationer från Uppsala UniversitetInfoscience - EPFL scientific publicationsOther literature typeData sources: Infoscience - EPFL scientific publicationshttps://doi.org/10.48550/arxiv...Article . 2018License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.3847/1538-4357/aaca3c&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint 2018Publisher:MDPI AG Authors: Soebur Razzaque; Lili Yang;Soebur Razzaque; Lili Yang;The origin of sub-TeV gamma rays detected by Fermi-LAT from the Fermi bubbles at the Galactic center is still unknown. In a hadronic model, acceleration of protons and/or nuclei and their subsequent interactions with gas in the bubble volume can produce observed gamma rays. Such interactions naturally produce high-energy neutrinos, and detection of those can discriminate between a hadronic and a leptonic origin of gamma rays. Additional constraints on the Fermi bubbles gamma-ray flux in the TeV range from recent HAWC observations restrict hadronic model parameters, which in turn disfavor Fermi bubbles as the origin of a large fraction of neutrino events detected by IceCube along the bubble directions. We revisit our hadronic model and discuss future constraints on parameters from observations in very high-energy gamma rays and neutrinos. Comment: 9 pages, 4 figures. Invited article submitted to MDPI journal Galaxies for its special issue, Searching for Connections among the Fermi Bubbles, the Galactic Center GeV Excess, and Loop I, edited by D. Malyshev
Galaxies arrow_drop_down GalaxiesOther literature type . Article . 2018 . Peer-reviewedLicense: CC BYFull-Text: http://www.mdpi.com/2075-4434/6/2/47/pdfhttps://doi.org/10.48550/arxiv...Article . 2018License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.3390/galaxies6020047&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen gold 9 citations 9 popularity Top 10% influence Average impulse Average Powered by BIP!more_vert Galaxies arrow_drop_down GalaxiesOther literature type . Article . 2018 . Peer-reviewedLicense: CC BYFull-Text: http://www.mdpi.com/2075-4434/6/2/47/pdfhttps://doi.org/10.48550/arxiv...Article . 2018License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.3390/galaxies6020047&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Preprint , Article 2020 Czech Republic, France, ItalyPublisher:EDP Sciences Ester Antonucci; Marco Romoli; Vincenzo Andretta; Silvano Fineschi; Petr Heinzel; J. Daniel Moses; Giampiero Naletto; Gianalfredo Nicolini; D. Spadaro; Luca Teriaca; A. Berlicki; Gerardo Capobianco; Giuseppe Crescenzio; Vania Da Deppo; Mauro Focardi; Fabio Frassetto; K. Heerlein; Federico Landini; Enrico Magli; A. M. Malvezzi; Giuseppe Massone; Radek Melich; Piergiorgio Nicolosi; Giancarlo Noci; Maurizio Pancrazzi; Maria G. Pelizzo; Luca Poletto; Clementina Sasso; Udo Schühle; Sami K. Solanki; Leonard Strachan; Roberto Susino; Giuseppe Tondello; Michela Uslenghi; Joachim Woch; Lucia Abbo; Alessandro Bemporad; Marta Casti; S. Dolei; Catia Grimani; Mauro Messerotti; Marco Ricci; Thomas Straus; Daniele Telloni; Paola Zuppella; Frédéric Auchère; Roberto Bruno; Angela Ciaravella; Alain Jody Corso; Miguel Alvarez Copano; Regina Aznar Cuadrado; Raffaella D'Amicis; R. Enge; Alessio Gravina; Sonja Jejčič; Philippe Lamy; A. C. Lanzafame; Thimo Meierdierks; Ioanna Papagiannaki; Hardi Peter; German Fernandez Rico; M.G. Sertsu; Jan Staub; Kanaris Tsinganos; Marco Velli; Rita Ventura; Enrico Verroi; Jean-Claude Vial; Sébastien Vivès; Antonio Volpicelli; Stephan Werner; Andreas Zerr; Barbara Negri; Marco Castronuovo; Alessandro Gabrielli; R. Bertacin; Rita Carpentiero; Silvia Natalucci; F. Marliani; Marco Cesa; Philippe Laget; Danilo Morea; Stefano Pieraccini; Paolo Radaelli; Paolo Sandri; Paolo Sarra; Stefano Cesare; Felice Del Forno; Ernesto Massa; Mauro Montabone; Sergio Mottini; Daniele Quattropani; Tiziano Schillaci; Roberto Boccardo; Rosario Brando; Arianna Pandi; Cristian Baietto; Riccardo Bertone; Alberto Álvarez-Herrero; Pilar García Parejo; María Cebollero; Mauro Amoruso; Vito Centonze;handle: 2318/1834172 , 11576/2669637 , 20.500.11769/491734 , 11583/2847550 , 2158/1217265 , 11577/3352909 , 11104/0313131
Aims. Metis is the first solar coronagraph designed for a space mission and is capable of performing simultaneous imaging of the off-limb solar corona in both visible and UV light. The observations obtained with Metis aboard the Solar Orbiter ESA-NASA observatory will enable us to diagnose, with unprecedented temporal coverage and spatial resolution, the structures and dynamics of the full corona in a square field of view (FoV) of ±2.9° in width, with an inner circular FoV at 1.6°, thus spanning the solar atmosphere from 1.7R⊙to about 9R⊙, owing to the eccentricity of the spacecraft orbit. Due to the uniqueness of the Solar Orbiter mission profile, Metis will be able to observe the solar corona from a close (0.28 AU, at the closest perihelion) vantage point, achieving increasing out-of-ecliptic views with the increase of the orbit inclination over time. Moreover, observations near perihelion, during the phase of lower rotational velocity of the solar surface relative to the spacecraft, allow longer-term studies of the off-limb coronal features, thus finally disentangling their intrinsic evolution from effects due to solar rotation.Methods. Thanks to a novel occultation design and a combination of a UV interference coating of the mirrors and a spectral bandpass filter, Metis images the solar corona simultaneously in the visible light band, between 580 and 640 nm, and in the UV H ILyman-αline at 121.6 nm. The visible light channel also includes a broadband polarimeter able to observe the linearly polarised component of the K corona. The coronal images in both the UV H ILyman-αand polarised visible light are obtained at high spatial resolution with a spatial scale down to about 2000 km and 15 000 km at perihelion, in the cases of the visible and UV light, respectively. A temporal resolution down to 1 s can be achieved when observing coronal fluctuations in visible light.Results. The Metis measurements, obtained from different latitudes, will allow for complete characterisation of the main physical parameters and dynamics of the electron and neutral hydrogen/proton plasma components of the corona in the region where the solar wind undergoes the acceleration process and where the onset and initial propagation of coronal mass ejections (CMEs) take place. The near-Sun multi-wavelength coronal imaging performed with Metis, combined with the unique opportunities offered by the Solar Orbiter mission, can effectively address crucial issues of solar physics such as: the origin and heating/acceleration of the fast and slow solar wind streams; the origin, acceleration, and transport of the solar energetic particles; and the transient ejection of coronal mass and its evolution in the inner heliosphere, thus significantly improving our understanding of the region connecting the Sun to the heliosphere and of the processes generating and driving the solar wind and coronal mass ejections.Conclusions. This paper presents the scientific objectives and requirements, the overall optical design of the Metis instrument, the thermo-mechanical design, and the processing and power unit; reports on the results of the campaigns dedicated to integration, alignment, and tests, and to the characterisation of the instrument performance; describes the operation concept, data handling, and software tools; and, finally, the diagnostic techniques to be applied to the data, as well as a brief description of the expected scientific products. The performance of the instrument measured during calibrations ensures that the scientific objectives of Metis can be pursued with success.
Archivio Istituziona... arrow_drop_down Archivio Istituzionale (AperTO); Archivio istituzionale della ricerca - Università di Padova; IRIS - Università degli Studi di Catania; Astronomy and Astrophysics; Publications Open Repository TOrino; Archivio istituzionale della ricerca - Università di UrbinoArticle . 2020 . 2019 . Peer-reviewedLicense: EDP Sciences Copyright and Publication Licensing PolicyRepository of the Czech Academy of SciencesArticle . 2020Data sources: Repository of the Czech Academy of SciencesRepository of the Czech Academy of SciencesArticle . 2020Data sources: Repository of the Czech Academy of SciencesIRIS - Università degli Studi di CataniaArticle . 2020Data sources: IRIS - Università degli Studi di CataniaMémoires en Sciences de l'Information et de la CommunicationArticle . 2020Flore (Florence Research Repository)Article . 2020Data sources: Flore (Florence Research Repository)https://doi.org/10.48550/arxiv...Article . 2019License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.euAccess RoutesGreen bronze 114 citations 114 popularity Top 1% influence Top 10% impulse Top 1% Powered by BIP!more_vert Archivio Istituziona... arrow_drop_down Archivio Istituzionale (AperTO); Archivio istituzionale della ricerca - Università di Padova; IRIS - Università degli Studi di Catania; Astronomy and Astrophysics; Publications Open Repository TOrino; Archivio istituzionale della ricerca - Università di UrbinoArticle . 2020 . 2019 . Peer-reviewedLicense: EDP Sciences Copyright and Publication Licensing PolicyRepository of the Czech Academy of SciencesArticle . 2020Data sources: Repository of the Czech Academy of SciencesRepository of the Czech Academy of SciencesArticle . 2020Data sources: Repository of the Czech Academy of SciencesIRIS - Università degli Studi di CataniaArticle . 2020Data sources: IRIS - Università degli Studi di CataniaMémoires en Sciences de l'Information et de la CommunicationArticle . 2020Flore (Florence Research Repository)Article . 2020Data sources: Flore (Florence Research Repository)https://doi.org/10.48550/arxiv...Article . 2019License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1051/0004-6361/201935338&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint 2019Publisher:Oxford University Press (OUP) U. Munari; Joshi; Debabrata Banerjee; Klemen Čotar; Sergei Yu. Shugarov; Rajka Jurdana-Šepić; R. Belligoli; A Bergamini; M. Graziani; G. L. Righetti; A. Vagnozzi; P. Valisa;We have been monitoring, at high cadence, the photometric and spectroscopic evolution of VES 263 following the discovery in 2018 of a brightening labeled as event Gaia-18azl. VES 263 is so far a neglected emission-line object discovered in the 1960s on objective prism plates, tentatively classified as a semi-regular AGB cool giant by automated analysis of ASASSN lightcurves. We have discovered that VES 263 is a bonafide massive pre-Main Sequence object (~12 Msun), of the Herbig AeBe type. It is located at 1.68+/-0.07 kpc distance, within the Cyg OB2 star-forming region, and it is highly reddened (E(B-V)=1.80+/-0.05) by interstellar extinction. In quiescence, the spectral energy distribution is dominated by the 20,000 K photospheric emission from the central B1II star, and at wavelenghts >=6 micron by emission from circumstellar warm dust (Tdust up to 400 K). The 2018-19 eruption was caused by a marked brightening of the accretion disk around the B1II star as traced by the evolution with time of the integrated flux and the double-peaked profile of emission lines. At the peak of the eruption, the disk has a bulk temperature of ~7500 K and a luminosity L>=860 Lsun, corresponding to a mass accretion rate >=1.1x10(-5) Msun/yr. Spectroscopic signature of possible bipolar jets (at -700 and +700 km/s) of variable intensity are found. We have reconstructed from Harvard, Moscow and Sonneberg photographic plates the photometric history of VES 263 from 1896 to 1995, showing through 1953-1969 a state much brighter than current eruption. To appear in MNRAS
Monthly Notices of t... arrow_drop_down Monthly Notices of the Royal Astronomical SocietyArticle . 2019 . Peer-reviewedLicense: OUP Standard Publication ReuseData sources: Crossrefhttps://doi.org/10.48550/arxiv...Article . 2019License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1093/mnras/stz2078&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen hybrid 5 citations 5 popularity Top 10% influence Average impulse Average Powered by BIP!more_vert Monthly Notices of t... arrow_drop_down Monthly Notices of the Royal Astronomical SocietyArticle . 2019 . Peer-reviewedLicense: OUP Standard Publication ReuseData sources: Crossrefhttps://doi.org/10.48550/arxiv...Article . 2019License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1093/mnras/stz2078&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint , Conference object 2019Embargo end date: 01 Jan 2019 Spain, FrancePublisher:arXiv Ballester, Otger; Blanch, Oscar; Boix, Joan; Bregeon, Johan; Brun, Patrick; Çolak, §ıdıka Merve; Doro, Michele; Da Deppo, Vania; Font, Lluís; Gabella, Omar; García-Tenorio García-Balmaseda, Rafael; Gaug, Markus; Maggio, Camilla; Martínez, Manel Cruz; Martínez, Óscar; Adrover, Pere Munar; Ramos, Raúl; Rivoire, Stephane; Staniˇc, Samo; Villar, David; Vasileiadis, George; Wang, Longlong; Zavrtanik, Marko;International audience; The Cherenkov Telescope Array (CTA) is the next generation ground based observatory for gamma ray astronomy at very high energies. Employing more than 100 Imaging Atmospheric Cherenkov Telescopes in the northern and southern hemispheres, it was designed to reach unprecedented sensitivity and energy resolution. Understanding and correcting for systematic biases on the absolute energy scale and instrument response functions will be a crucial issue for the performance of CTA. The LUPM group and the Spanish/Italian/Slovenian collaboration are currently building two Raman LIDAR prototypes for the online atmospheric calibration along the line of sight of the CTA. Requirements for such a solution include the ability to characterize aerosol extinction at two wavelengths to distances of 30 km with an accuracy better than 5%, within time scales of about a minute, steering capabilities and close interaction with the CTA array control and data acquisition system as well as other auxiliary instruments. Our Raman LIDARs have design features that make them different from those used in atmospheric science and are characterized by large collecting mirrors (2.5 m2), liquid light guides that collect the light at the focal plane and transport it to the readout system, reduced acquisition time and highly precise Raman spectrometers. The Raman LIDARs will participate in a cross calibration and characterization campaign of the atmosphere at the CTA North site at La Palma, together with other site characterization instruments. After a one year test period there, an in depth evaluation of the solutions adopted by the two projects will lead to a final Raman LIDAR design proposal for both CTA sites.
Recolector de Cienci... arrow_drop_down Recolector de Ciencia Abierta, RECOLECTA; idUS. Depósito de Investigación de la Universidad de Sevilla.Conference object . 2020 . 2019License: CC BY NC NDFull-Text: https://pos.sissa.it/358/814/pdfhttps://doi.org/10.48550/arxiv...Article . 2019License: arXiv Non-Exclusive DistributionData sources: DataciteHAL - UPEC / UPEM; HAL-Pasteur; HAL-InsermConference object . 2019add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.48550/arxiv.1909.09342&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen 0 citations 0 popularity Average influence Average impulse Average Powered by BIP!more_vert Recolector de Cienci... arrow_drop_down Recolector de Ciencia Abierta, RECOLECTA; idUS. Depósito de Investigación de la Universidad de Sevilla.Conference object . 2020 . 2019License: CC BY NC NDFull-Text: https://pos.sissa.it/358/814/pdfhttps://doi.org/10.48550/arxiv...Article . 2019License: arXiv Non-Exclusive DistributionData sources: DataciteHAL - UPEC / UPEM; HAL-Pasteur; HAL-InsermConference object . 2019add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.48550/arxiv.1909.09342&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint 2022 ItalyPublisher:EDP Sciences A. Bemporad; V. Andretta; R. Susino; S. Mancuso; D. Spadaro; M. Mierla; D. Berghmans; E. D’Huys; A. N. Zhukov; D.-C. Talpeanu; R. Colaninno; P. Hess; J. Koza; S. Jejčič; P. Heinzel; E. Antonucci; V. Da Deppo; S. Fineschi; F. Frassati; G. Jerse; F. Landini; G. Naletto; G. Nicolini; M. Pancrazzi; M. Romoli; C. Sasso; A. Slemer; M. Stangalini; L. Teriaca;On February 12, 2021 two subsequent eruptions occurred above the West limb, as seen along the Sun-Earth line. The first event was a typical slow Coronal Mass Ejection (CME), followed $\sim 7$ hours later by a smaller and collimated prominence eruption, originating Southward with respect to the CME, followed by a plasma blob. These events were observed not only by SOHO and STEREO-A missions, but also by the suite of remote sensing instruments on-board Solar Orbiter (SolO). This work shows how data acquired by the Full Sun Imager (FSI), Metis coronagraph, and Heliospheric Imager (SoloHI) from the SolO perspective can be combined to study the eruptions and the different source regions. Moreover, we show how Metis data can be analyzed to provide new information about solar eruptions. Different 3D reconstruction methods were applied to the data acquired by different spacecraft including remote sensing instruments on-board SolO. Images acquired by both Metis channels in the Visible Light (VL) and H I Lyman$-\alpha$ line (UV) were combined to derive physical information on the expanding plasma. The polarization ratio technique was also applied for the first time to the Metis images acquired in the VL channel. The two eruptions were followed in 3D from their source region to their expansion in the intermediate corona. Thanks to the combination of VL and UV Metis data, the formation of a post-CME Current Sheet (CS) was followed for the first time in the intermediate corona. The plasma temperature gradient across a post-CME blob propagating along the CS was also measured for the first time. Application of the polarization ratio technique to Metis data shows that, thanks to the combination of four different polarization measurements, the errors are reduced by $\sim 5-7$\%, thus better constraining the 3D distribution of plasma. Comment: 15 pages, 14 figures, accepted for publication on A&A
Flore (Florence Rese... arrow_drop_down Flore (Florence Research Repository); Astronomy and AstrophysicsArticle . 2022 . Peer-reviewedLicense: EDP Sciences Copyright and Publication Licensing PolicyFlore (Florence Research Repository)Article . 2022Data sources: Flore (Florence Research Repository)https://doi.org/10.48550/arxiv...Article . 2022License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1051/0004-6361/202243162&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen 6 citations 6 popularity Top 10% influence Average impulse Top 10% Powered by BIP!more_vert Flore (Florence Rese... arrow_drop_down Flore (Florence Research Repository); Astronomy and AstrophysicsArticle . 2022 . Peer-reviewedLicense: EDP Sciences Copyright and Publication Licensing PolicyFlore (Florence Research Repository)Article . 2022Data sources: Flore (Florence Research Repository)https://doi.org/10.48550/arxiv...Article . 2022License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Other literature type , Preprint 2020 Belgium, Italy, Italy, Italy, Netherlands, Italy, Italy, Italy, Italy, Brazil, Italy, Germany, France, Belgium, Czech Republic, Spain, GermanyPublisher:IOP Publishing Funded by:NSF | Pierre Auger ProjectNSF| Pierre Auger ProjectAuthors: Marco Aglietta; Jaime Alvarez-Muñiz; R. Alves Batista; Gioacchino Alex Anastasi; +214 AuthorsMarco Aglietta; Jaime Alvarez-Muñiz; R. Alves Batista; Gioacchino Alex Anastasi; Luis A. Anchordoqui; B. Andrada; P.R. Araújo Ferreira; Hernán Asorey; Pedro Assis; Gualberto Avila; Alena Bakalova; F. C. T. Barbato; K.-H. Becker; Jose A. Bellido; Corinne Berat; M. E. Bertaina; Xavier Bertou; Peter L. Biermann; Teresa Bister; Jonathan Biteau; A. Blanco; Carla Bleve; Martina Bohacova; Denise Boncioli; Carla Bonifazi; L. Bonneau Arbeletche; Nataliia Borodai; Jeffrey Brack; Thomas Bretz; A. Bridgeman; Peter Buchholz; Antonio Bueno; Stijn Buitink; Mario Buscemi; Karen S. Caballero-Mora; Lorenzo Caccianiga; Fabrizia Canfora; Rossella Caruso; Antonella Castellina; G. Cataldi; Lorenzo Cazon; Jose Chinellato; J. Chudoba; Roger W Clay; Roberta Colalillo; Alan Coleman; Giovanni Consolati; Fernando Contreras; Fabio Convenga; Corbin Covault; Kai Daumiller; Bruce R. Dawson; R. M. de Almeida; J. de Jesús; S. J. De Jong; G. De Mauro; J. de Oliveira; D. de Oliveira Franco; J. Debatin; A. Di Matteo; R.C. dos Anjos; Jan Ebr; Italo Epicoco; Martin Erdmann; G. Farrar; A. C. Fauth; N. Fazzini; Francesco Fenu; Juan Manuel Figueira; Tomáš Fodran; Toshihiro Fujii; Cristina Galea; H. Gemmeke; Flavia Gesualdi; Alexandru Gherghel-Lascu; Ugo Giaccari; Jonas Glombitza; G. Golup; Juan Pablo Gongora; Nicolás González; Dariusz Gora; Alessio Gorgi; Marvin Gottowik; F. Guarino; G. P. Guedes; Eleonora Guido; M. R. Hampel; D. Harari; Violet M. Harvey; A. Haungs; Thomas Hebbeker; D. Heck; C. Hojvat; Pavel Horvath; Miroslav Hrabovský; T. Huege; A. Insolia; Paula Gina Isar; Jeffrey A. Johnsen; Jakub Juryšek; B. Keilhauer; Julian Kemp; B. L. Lago; Vladimir Lenok; A. Letessier-Selvon; D. Lo Presti; L. Lopes; A. Machado Payeras; Dusan Mandat; B. C. Manning; Sullivan Marafico; Ioana Codrina Maris; G. Marsella; H. Martinez; Massimo Mastrodicasa; John Matthews; Eric Mayotte; P.O. Mazur; G. Medina-Tanco; A. Menshikov; Kevin-Druis Merenda; Stanislav Michal; M. I. Micheletti; Lino Miramonti; Silvia Mollerach; C. Morello; Miguel Mostafa; Alfred Müller; M. A. Muller; W. M. Namasaka; Mihai Niculescu-Oglinzanu; Marcus Niechciol; D. Nosek; M. Palatka; J. Pallotta; M.P. Panetta; Philipp Papenbreer; G. Parente; A. Parra; F. Pedreira; Rodrigo Pelayo; Jesús Peña-Rodríguez; J. Perez Armand; Christine Peters; S. Petrera; T. Pierog; Valerio Pirronello; M. Platino; M. Pothast; S. Querchfeld; Maximilian Reininghaus; F. Riehn; M. Risse; Vincenzo Rizi; W. Rodrigues de Carvalho; J. Rodriguez Rojo; Markus Roth; Esteban Roulet; A. C. Rovero; P. Ruehl; F. Salamida; G. Salina; E. Santos; Fred Sarazin; Raul Sarmento; Christian Sarmiento-Cano; P. Savina; C. M. Schäfer; V. Scherini; M. Schimp; Felix Schlüter; Frank G. Schröder; S. Schröder; André Schulz; S. J. Sciutto; Marina Scornavacche; R. C. Shellard; Günter Sigl; Gaia Silli; Octavian Sima; Radomir Smida; Paul Sommers; Julien Souchard; R. Squartini; Maximilian Stadelmaier; Samo Stanič; J. Stasielak; J. Šupík; Charles Timmermans; Olena Tkachenko; B. Tome; G. Torralba Elipe; Andres Travaini; Petr Travnicek; Caterina Trimarelli; M. Trini; Matias Tueros; Ralf Ulrich; M. Urban; Lukáš Vaclavek; Martin Vacula; A. van Vliet; E. Varela; B. Vargas Cárdenas; Carlo Ventura; I.D. Vergara Quispe; Luis Villaseñor; Marc Weber; A. Weindl; L. R. Wiencke; M. Wirtz; David Wittkowski; B. Wundheiler; A. Yushkov; Orazio Zapparrata; Enrique Zas; M. Zavrtanik; Francesca Zuccarello;doi: 10.1088/1748-0221/15/10/p10021 , 10.5445/ir/1000125360 , 10.48550/arxiv.2007.09035 , 10.18154/rwth-2021-02045
handle: 11245.1/25389f08-b24d-4f82-bc0b-d164100f717f , 11311/1152632 , 11370/f58e1a6c-b4a8-453b-8710-48cf4e4f7433 , 10481/66661 , 20.500.14017/635365e9-9a46-46aa-9417-1bac709feb8f , 11697/153436 , 20.500.11769/497650 , 2066/230078 , 10447/469211 , 11588/826320 , 11104/0316156 , https://repository.ubn.ru.nl/handle/2066/230078 , 2318/1803310 , 11587/447686
doi: 10.1088/1748-0221/15/10/p10021 , 10.5445/ir/1000125360 , 10.48550/arxiv.2007.09035 , 10.18154/rwth-2021-02045
handle: 11245.1/25389f08-b24d-4f82-bc0b-d164100f717f , 11311/1152632 , 11370/f58e1a6c-b4a8-453b-8710-48cf4e4f7433 , 10481/66661 , 20.500.14017/635365e9-9a46-46aa-9417-1bac709feb8f , 11697/153436 , 20.500.11769/497650 , 2066/230078 , 10447/469211 , 11588/826320 , 11104/0316156 , https://repository.ubn.ru.nl/handle/2066/230078 , 2318/1803310 , 11587/447686
Cosmic rays arriving at Earth collide with the upper parts of the atmosphere, thereby inducing extensive air showers. When secondary particles from the cascade arrive at the ground, they are measured by surface detector arrays. We describe the methods applied to the measurements of the surface detector of the Pierre Auger Observatory to reconstruct events with zenith angles less than 60 using the timing and signal information recorded using the water-Cherenkov detector stations. In addition, we assess the accuracy of these methods in reconstructing the arrival directions of the primary cosmic ray particles and the sizes of the induced showers. Czech Republic Grant MSMT CR LTT18004 LM2015038 LM2018102 CZ.02.1.01/0.0/0.0/16_013/0001402 CZ.02.1.01/0.0/0.0/18_046/0016010 CZ.02.1.01/0.0/0.0/17_049/0008422 Portugal - FEDER funds within Programa Operacional Factores de Competitividade through Fundacao para a Ciencia e a Tecnologia (COMPETE) Romania - Romanian Ministry of Education and Research, the Program Nucleu within PNCDI III PN-III-P11.2-PCCDI-2017-0839/19PCCDI/2018 Poland - National Science Centre 2013/08/M/ST9/00322 2016/23/B/ST9/01635 HARMONIA 52013/10/M/ST9/00062 UMO-2016/22/M/ST9/00198 Romania - Romanian Ministry of Education and Research, the Program Nucleu within MCI PN19150201/16N/2019 PN19060102 United States Department of Energy (DOE) DE-AC02-07CH11359 DE-FR02-04ER41300 DEFG02-99ER41107 DE-SC0011689 Fundacao de Amparo a Pesquisa do Estado de Sao Paulo (FAPESP) 2019/10151-2 2010/07359-6 1999/05404-3 Germany - Min-isterium fur Innovation, Wissenschaft und Forschung des Landes Nordrhein-Westfalen Spain - Ministerio de Economía, Industria y Competitividad FPA2017-85114-P FPA2017-85197-P Carlos Chagas Filho Foundation for Research Support of the State of Rio de Janeiro (FAPERJ) Germany - Ministerium fur Wissenschaft, Forschung und Kunst des Landes Baden-Wurttemberg Argentina - Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET) French National Research Agency (ANR) LABEX ANR-10-LABX-63 ANR11-IDEX-0004-02 Brazil - Ministerio da Ciencia, Tecnologia, Inovacoes e Comunicacoes (MCTIC) Argentina - Agencia Nacional de Promoción Científica y Tecnológica (ANPCyT) Spain - RENATARedNacional Tematica de Astroparticulas FPA2015-68783-REDT Italy - Ministero dell'Istruzione, dell'Universita e della Ricerca (MIUR) France - Departement Physique Nucleaire et Corpusculaire (PNC-IN2P3/CNRS) Slovenian Research Agency - Slovenia P1-0031 P1-0385 I0-0033 N1-0111 National Council for Scientific and Technological Development (CNPq) Germany - Helmholtz-Gemeinschaft Deutscher Forschungszentren (HGF) Poland - Ministry of Science and Higher Education DIR/WK/2018/11 Germany - Helmholtz Alliance for Astroparticle Physics (HAP) The Netherlands - Ministry of Education, Culture and Science France - Departement Sciences de l'Univers (SDU-INSU/CNRS) Consejo Nacional de Ciencia y Tecnología (CONACyT) 167733 U.S.A. - European Particle Physics Latin American Network Spain - Maria de MaeztuUnit of Excellence MDM-2016-0692 México - Universidad Nacional Autónoma de México (UNAM) Netherlands Organization for Scientific Research (NWO) Italy - Istituto Nazionale di Fisica Nucleare (INFN) Brazil - Financiadora de Estudos e Projetos (FINEP) Centre National de la Recherche Scientifique (CNRS) The Netherlands - Dutch national e-infrastructure Italy - Istituto Nazionale di Astrofisica (INAF) Argentina - Comisión Nacional de Energía Atómica Federal Ministry of Education & Research (BMBF) Argentina - Gobierno de la Provincia de Mendoza Germany - Finanzministerium Baden-Wurttemberg Italy - Ministero degli Affari Esteri (MAE) National Science Foundation (NSF) 0450696 Spain - Xunta de Galicia ED431C 2017/07 Australia - Australian Research Council France - Conseil Regional Ile-de-France Argentina - Municipalidad de Malargue France - Centre de Calcul IN2P3/CNRS Italy - CETEMPS Center of Excellence Portugal - Portuguese national funds Junta de Andalucía SOMM17/6104/UGR U.S.A. - Marie Curie-IRSES/EPLANET The Netherlands - SURF Cooperative German Research Foundation (DFG) U.S.A. - Grainger Foundation Argentina - Valle Las Lenas México - PAPIIT DGAPA-UNAM Argentina - NDM Holdings Spain - Feder Funds U.S.A. - UNESCO
NARCIS arrow_drop_down Archivio Istituzionale della Ricerca - Università degli Studi dell Aquila; Archivio Istituzionale della Ricerca- Università del Salento; Journal of Instrumentation; Archivio istituzionale della ricerca - Università di Palermo; Recolector de Ciencia Abierta, RECOLECTA; IRIS - Università degli Studi di Catania; METIS Research Information System; Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual) - Universidade de São Paulo (USP); Archivio della ricerca - Università degli studi di Napoli Federico II; RE.PUBLIC@POLIMI Research Publications at Politecnico di MilanoArticle . 2020License: CC BYData sources: Archivio Istituzionale della Ricerca - Università degli Studi dell Aquila; Archivio Istituzionale della Ricerca- Università del Salento; Universiteit van Amsterdam (UvA) Institutional Repository UvA-DARE; University of Groningen Research Portal; Archivio istituzionale della ricerca - Università di Palermo; Recolector de Ciencia Abierta, RECOLECTA; IRIS - Università degli Studi di Catania; LAReferencia - Red Federada de Repositorios Institucionales de Publicaciones Científicas Latinoamericanas; METIS Research Information System; Archivio della ricerca - Università degli studi di Napoli Federico II; RE.PUBLIC@POLIMI Research Publications at Politecnico di MilanoOA@INAF - Istituto Nazionale di AstrofisicaArticle . 2020Data sources: OA@INAF - Istituto Nazionale di AstrofisicaRepository of the Czech Academy of SciencesArticle . 2020Data sources: Repository of the Czech Academy of SciencesRepository of the Czech Academy of SciencesArticle . 2020Data sources: Repository of the Czech Academy of SciencesRadboud Repository; Journal of InstrumentationArticle . 2020Vrije Universiteit Brussel Research PortalOther literature type . 2020Data sources: Vrije Universiteit Brussel Research PortalIRIS - Università degli Studi di CataniaArticle . 2020Data sources: IRIS - Università degli Studi di CataniaRecolector de Ciencia Abierta, RECOLECTA; Repositorio Institucional Universidad de GranadaOther literature type . Article . 2021 . 2020add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1088/1748-0221/15/10/p10021&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen hybrid 9 citations 9 popularity Top 10% influence Average impulse Top 10% Powered by BIP!more_vert NARCIS arrow_drop_down Archivio Istituzionale della Ricerca - Università degli Studi dell Aquila; Archivio Istituzionale della Ricerca- Università del Salento; Journal of Instrumentation; Archivio istituzionale della ricerca - Università di Palermo; Recolector de Ciencia Abierta, RECOLECTA; IRIS - Università degli Studi di Catania; METIS Research Information System; Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual) - Universidade de São Paulo (USP); Archivio della ricerca - Università degli studi di Napoli Federico II; RE.PUBLIC@POLIMI Research Publications at Politecnico di MilanoArticle . 2020License: CC BYData sources: Archivio Istituzionale della Ricerca - Università degli Studi dell Aquila; Archivio Istituzionale della Ricerca- Università del Salento; Universiteit van Amsterdam (UvA) Institutional Repository UvA-DARE; University of Groningen Research Portal; Archivio istituzionale della ricerca - Università di Palermo; Recolector de Ciencia Abierta, RECOLECTA; IRIS - Università degli Studi di Catania; LAReferencia - Red Federada de Repositorios Institucionales de Publicaciones Científicas Latinoamericanas; METIS Research Information System; Archivio della ricerca - Università degli studi di Napoli Federico II; RE.PUBLIC@POLIMI Research Publications at Politecnico di MilanoOA@INAF - Istituto Nazionale di AstrofisicaArticle . 2020Data sources: OA@INAF - Istituto Nazionale di AstrofisicaRepository of the Czech Academy of SciencesArticle . 2020Data sources: Repository of the Czech Academy of SciencesRepository of the Czech Academy of SciencesArticle . 2020Data sources: Repository of the Czech Academy of SciencesRadboud Repository; Journal of InstrumentationArticle . 2020Vrije Universiteit Brussel Research PortalOther literature type . 2020Data sources: Vrije Universiteit Brussel Research PortalIRIS - Università degli Studi di CataniaArticle . 2020Data sources: IRIS - Università degli Studi di CataniaRecolector de Ciencia Abierta, RECOLECTA; Repositorio Institucional Universidad de GranadaOther literature type . Article . 2021 . 2020add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1088/1748-0221/15/10/p10021&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Preprint , Article 2020Publisher:Elsevier BV Authors: Rok Vogrinčič; Alejandro Lara; Andrea Borgazzi; Jean-Pierre Raulin;Rok Vogrinčič; Alejandro Lara; Andrea Borgazzi; Jean-Pierre Raulin;The altitude of the ionospheric lower layer (D-region) is highly influenced by the solar UV flux affecting in turn, the propagation of Very Low Frequency (VLF) signals inside the waveguide formed between this layer and the Earth surface. A rapid change of the solar irradiance, as during a solar eclipse, can help to understand the details of the energy transfer of the solar radiation onto the ionospheric D-layer. Using the "Latin American VLF Network" (LAVNet-Mex) receiver station in Mexico City, Mexico, we detected the phase and amplitude changes of the VLF signals transmitted by the NDK station at 25.2 kHz in North Dakota, USA during the August 21, 2017, solar eclipse. As the Sunlight was eclipsed, the rate of ionization in the ionosphere (D-region) was reduced and the effective reflection height increased, causing a considerable drop of the phase and amplitude of the observed VLF waves. The corresponding waveguide path is 3007.15 km long and crossed almost perpendicularly the total eclipse path. Circumstantially, at the time of the total eclipse, a C3 flare took place allowing us to isolate the flare flux from the background flux of a large portion of the disk. In this work, we report the observations and present a new model of the ionospheric effects of the eclipse and flare. The model is based on a detailed setup of the degree of Moon shadow that affects the entire Great Circle Path (GCP). During the eclipse, the maximum phase variation was -63.36$^{\circ}$ at 18:05 UT which, according to our model, accounts for a maximum increase of the reflection height of 9.3 km. Comment: 23 pages, 5 figures, appendix A and B, accepted for publication in Advances in Space Research
arXiv.org e-Print Ar... arrow_drop_down Advances in Space ResearchArticle . 2020 . Peer-reviewedLicense: Elsevier TDMData sources: Crossrefhttps://doi.org/10.48550/arxiv...Article . 2019License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1016/j.asr.2019.10.032&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen bronze 7 citations 7 popularity Top 10% influence Average impulse Top 10% Powered by BIP!more_vert arXiv.org e-Print Ar... arrow_drop_down Advances in Space ResearchArticle . 2020 . Peer-reviewedLicense: Elsevier TDMData sources: Crossrefhttps://doi.org/10.48550/arxiv...Article . 2019License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1016/j.asr.2019.10.032&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Other literature type , Article , Preprint 2021 Italy, Belgium, Germany, Brazil, Italy, Italy, Italy, Netherlands, Italy, Belgium, Italy, France, ItalyPublisher:IOP Publishing Funded by:NSF | Pierre Auger ProjectNSF| Pierre Auger ProjectA. Aab; P. Abreu; Marco Aglietta; Jaime Alvarez-Muñiz; R. Alves Batista; Gioacchino Alex Anastasi; Belén Andrada; Sofia Andringa; Carla Aramo; P.R. Araújo Ferreira; J. C. Arteaga Velázquez; Hernán Asorey; Pedro Assis; Alena Bakalova; Alexandru Balaceanu; K.-H. Becker; Jose A. Bellido; Corinne Berat; M. E. Bertaina; Xavier Bertou; Peter L. Biermann; J. Biteau; Jonathan Blazek; Carla Bleve; Martina Bohacova; Denise Boncioli; L. Bonneau Arbeletche; Nataliia Borodai; Ana Martina Botti; Jeffrey Brack; Thomas Bretz; Florian Lukas Briechle; Peter Buchholz; Antonio Bueno; Stijn Buitink; Mario Buscemi; Karen S. Caballero-Mora; Lorenzo Caccianiga; Ioana Caracas; Rossella Caruso; Antonella Castellina; Fernando Catalani; G. Cataldi; Lorenzo Cazon; Magdalena Cerdá; Jose Chinellato; Ladislav Chytka; Roger W Clay; A.C. Cobos Cerutti; Roberta Colalillo; Alan Coleman; Maria Rita Coluccia; Rúben Conceição; Giovanni Consolati; Fernando Contreras; Fabio Convenga; Corbin Covault; Sergio Dasso; Bruce R. Dawson; R. M. de Almeida; J. de Jesús; G. De Mauro; J. R. T. de Mello Neto; I. De Mitri; E. De Vito; Carola Dobrigkeit; Ralph Engel; Italo Epicoco; Martin Erdmann; Carlos Escobar; A. Etchegoyen; John Farmer; N. Fazzini; Francesco Fenu; Juan Manuel Figueira; Tomáš Fodran; Toshihiro Fujii; A. Fuster; Cristina Galea; B. García; A.L. Garcia Vegas; Flavia Gesualdi; Marco Giammarchi; M. Giller; Jonas Glombitza; G. Golup; M. Gómez Berisso; Juan Pablo Gongora; N. González; Isabel Goos; Dariusz Gora; A. Gorgi; Trent D. Grubb; F. Guarino; G. P. Guedes; Eleonora Guido; Matías Rolf Hampel; Violet M. Harvey; G. C. Hill; Jörg R. Hörandel; Pavel Horvath; A. Insolia; Paula Gina Isar; Petr Janecek; Jakub Juryšek; Alex Kääpä; K. H. Kampert; B. Keilhauer; Julian Kemp; J. Kleinfeller; Rodrigo Guedes Lang; Vladimir Lenok; Antoine Letessier-Selvon; D. Lo Presti; R. López; A. Lucero; Jon Paul Lundquist; G. Mancarella; P. Mantsch; Sullivan Marafico; A. G. Mariazzi; G. Marsella; D. Martello; H. Martinez; John Matthews; G. Matthiae; Eric Mayotte; G. Medina-Tanco; D. Melo; Lino Miramonti; Silvia Mollerach; C. Morello; Katie Mulrey; Roberto Mussa; L. Nellen; Mihai Niculescu-Oglinzanu; Marcus Niechciol; D. Nitz; Luis A. Nunez; M. Palatka; J. Pallotta; A. Parra; J. Pkala; Rodrigo Pelayo; J. Perez Armand; C. Pérez Bertolli; L. Perrone; S. Petrera; T. Pierog; M. Pimenta; Valerio Pirronello; M. Platino; Bjarni Pont; Paolo Privitera; A. Puyleart; Maximilian Reininghaus; F. Riehn; Vincenzo Rizi; W. Rodrigues de Carvalho; Esteban Roulet; P. Ruehl; F. Salamida; Humberto Ibarguen Salazar; G. Salina; J.D. Sanabria Gomez; Fred Sarazin; Raul Sarmento; Christian Sarmiento-Cano; R. Sato; P. Savina; V. Scherini; H. Schieler; M. Schimassek; M. Schimp; Felix Schlüter; Petr Schovanek; Frank G. Schröder; Josina Schulte; A. Segreto; R. C. Shellard; Günter Sigl; Octavian Sima; Radomir Smida; Julien Souchard; Maximilian Stadelmaier; Denis Stanca; Samo Stanič; P. Stassi; A. Streich; M. Suárez-Durán; Tristan Sudholz; T. Suomijärvi; A. Taboada; Olena Tkachenko; P. Tobiska; B. Tome; Matias Tueros; Lukáš Vaclavek; Martin Vacula; J. F. Valdés Galicia; L. Valore; K. C. V. Varma; Darko Veberič; Carlo Ventura; I.D. Vergara Quispe; Valerio Verzi; Hernan Wahlberg; A. Weindl; L. R. Wiencke; Tobias Winchen; M. Wirtz; David Wittkowski; B. Wundheiler; Orazio Zapparrata; Enrique Zas; L. Zehrer; A. Zepeda; R. Cunniffe; J. Eliášek; I. Ebrová; M. Jelínek; P. Kubánek;handle: 11697/168859 , https://repository.ubn.ru.nl/handle/2066/236331 , 11370/00e93631-ebe4-4486-9374-69d5c5d23fb8 , 2066/236331 , 20.500.11769/526700 , 11588/890389 , 11311/1180491 , 2318/1803397 , 11587/458358 , 11245.1/12cefc58-b28a-4488-92a4-53315dbceed2 , 20.500.14017/a580ffd4-97ef-41c7-9d62-48b63eb0c0d6
handle: 11697/168859 , https://repository.ubn.ru.nl/handle/2066/236331 , 11370/00e93631-ebe4-4486-9374-69d5c5d23fb8 , 2066/236331 , 20.500.11769/526700 , 11588/890389 , 11311/1180491 , 2318/1803397 , 11587/458358 , 11245.1/12cefc58-b28a-4488-92a4-53315dbceed2 , 20.500.14017/a580ffd4-97ef-41c7-9d62-48b63eb0c0d6
FRAM (F/Photometric Robotic Atmospheric Monitor) is a robotic telescope operated at the Pierre Auger Observatory in Argentina for the purposes of atmospheric monitoring using stellar photometry. As a passive system which does not produce any light that could interfere with the observations of the fluorescence telescopes of the observatory, it complements the active monitoring systems that use lasers. We discuss the applications of stellar photometry for atmospheric monitoring at optical observatories in general and the particular modes of operation employed by the Auger FRAM. We describe in detail the technical aspects of FRAM, the hardware and software requirements for a successful operation of a robotic telescope for such a purpose and their implementation within the FRAM system. Published version, 27 pages, 8 figures
NARCIS arrow_drop_down Archivio Istituzionale della Ricerca - Università degli Studi dell Aquila; Archivio Istituzionale (AperTO); Archivio Istituzionale della Ricerca- Università del Salento; Journal of Instrumentation; IRIS - Università degli Studi di Catania; METIS Research Information System; Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual) - Universidade de São Paulo (USP); RE.PUBLIC@POLIMI Research Publications at Politecnico di MilanoArticle . 2021Data sources: Archivio Istituzionale della Ricerca - Università degli Studi dell Aquila; Archivio Istituzionale (AperTO); Archivio Istituzionale della Ricerca- Università del Salento; Universiteit van Amsterdam (UvA) Institutional Repository UvA-DARE; University of Groningen Research Portal; IRIS - Università degli Studi di Catania; LAReferencia - Red Federada de Repositorios Institucionales de Publicaciones Científicas Latinoamericanas; METIS Research Information System; RE.PUBLIC@POLIMI Research Publications at Politecnico di MilanoPublikationsserver der RWTH Aachen UniversityPreprint . 2021Data sources: Publikationsserver der RWTH Aachen UniversityIRIS - Università degli Studi di CataniaArticle . 2021Data sources: IRIS - Università degli Studi di CataniaJournal of Instrumentation; Archivio della ricerca - Università degli studi di Napoli Federico IIArticle . 2021 . Peer-reviewedLicense: IOP Copyright PoliciesVrije Universiteit Brussel Research PortalOther literature type . 2021Data sources: Vrije Universiteit Brussel Research Portaladd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.euAccess RoutesGreen bronze 0 citations 0 popularity Average influence Average impulse Average Powered by BIP!more_vert NARCIS arrow_drop_down Archivio Istituzionale della Ricerca - Università degli Studi dell Aquila; Archivio Istituzionale (AperTO); Archivio Istituzionale della Ricerca- Università del Salento; Journal of Instrumentation; IRIS - Università degli Studi di Catania; METIS Research Information System; Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual) - Universidade de São Paulo (USP); RE.PUBLIC@POLIMI Research Publications at Politecnico di MilanoArticle . 2021Data sources: Archivio Istituzionale della Ricerca - Università degli Studi dell Aquila; Archivio Istituzionale (AperTO); Archivio Istituzionale della Ricerca- Università del Salento; Universiteit van Amsterdam (UvA) Institutional Repository UvA-DARE; University of Groningen Research Portal; IRIS - Università degli Studi di Catania; LAReferencia - Red Federada de Repositorios Institucionales de Publicaciones Científicas Latinoamericanas; METIS Research Information System; RE.PUBLIC@POLIMI Research Publications at Politecnico di MilanoPublikationsserver der RWTH Aachen UniversityPreprint . 2021Data sources: Publikationsserver der RWTH Aachen UniversityIRIS - Università degli Studi di CataniaArticle . 2021Data sources: IRIS - Università degli Studi di CataniaJournal of Instrumentation; Archivio della ricerca - Università degli studi di Napoli Federico IIArticle . 2021 . Peer-reviewedLicense: IOP Copyright PoliciesVrije Universiteit Brussel Research PortalOther literature type . 2021Data sources: Vrije Universiteit Brussel Research Portaladd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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description Publicationkeyboard_double_arrow_right Article , Other literature type , Preprint 2018 Sweden, Italy, Italy, Italy, Switzerland, United KingdomPublisher:American Astronomical Society Funded by:EC | GAIA-ESO-MWEC| GAIA-ESO-MWMariagrazia Franchini; Carlo Morossi; Paolo Di Marcantonio; Miguel Chavez; Gerry Gilmore; Sofia Randich; Ettore Flaccomio; Sergey E. Koposov; Andreas J. Korn; Amelia Bayo; Giovanni Carraro; Andrew R. Casey; E. Franciosini; A. Hourihane; Paula Jofre; Carmela Lardo; James R. Lewis; Laura Magrini; L. Morbidelli; G. G. Sacco; Clare Worley; Tomaz Zwitter;We present a high resolution synthetic spectral library, INTRIGOSS, designed for studying FGK stars. The library is based on atmosphere models computed with specified individual element abundances via ATLAS12 code. Normalized SPectra (NSP) and surface Flux SPectra (FSP), in the 4830-5400 A, wavelength range, were computed with the SPECTRUM code. INTRIGOSS uses the solar composition by Grevesse et al. 2007 and four [alpha/Fe] abundance ratios and consists of 15,232 spectra. The synthetic spectra are computed with astrophysical gf-values derived by comparing synthetic predictions with a very high SNR solar spectrum and the UVES-U580 spectra of five cool giants. The validity of the NSPs is assessed by using the UVES-U580 spectra of 2212 stars observed in the framework of the Gaia-ESO Survey and characterized by homogeneous and accurate atmospheric parameter values and by detailed chemical compositions. The greater accuracy of NSPs with respect to spectra from the AMBRE, GES_Grid, PHOENIX, C14, and B17 synthetic spectral libraries is demonstrated by evaluating the consistency of the predictions of the different libraries for the UVES-U580 sample stars. The validity of the FSPs is checked by comparing their prediction with both observed spectral energy distribution and spectral indices. The comparison of FSPs with SEDs derived from ELODIE, INDO--U.S., and MILES libraries indicates that the former reproduce the observed flux distributions within a few percent and without any systematic trend. The good agreement between observational and synthetic Lick/SDSS indices shows that the predicted blanketing of FSPs well reproduces the observed one, thus confirming the reliability of INTRIGOSS FSPs. Comment: 32 pages, 12 figures
Edinburgh Research E... arrow_drop_down OA@INAF - Istituto Nazionale di AstrofisicaArticle . 2018Data sources: OA@INAF - Istituto Nazionale di AstrofisicaPublikationer från Uppsala UniversitetArticle . 2018 . Peer-reviewedData sources: Publikationer från Uppsala UniversitetInfoscience - EPFL scientific publicationsOther literature typeData sources: Infoscience - EPFL scientific publicationshttps://doi.org/10.48550/arxiv...Article . 2018License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.euAccess RoutesGreen hybrid 9 citations 9 popularity Top 10% influence Average impulse Top 10% Powered by BIP!visibility 8visibility views 8 download downloads 6 Powered bymore_vert Edinburgh Research E... arrow_drop_down OA@INAF - Istituto Nazionale di AstrofisicaArticle . 2018Data sources: OA@INAF - Istituto Nazionale di AstrofisicaPublikationer från Uppsala UniversitetArticle . 2018 . Peer-reviewedData sources: Publikationer från Uppsala UniversitetInfoscience - EPFL scientific publicationsOther literature typeData sources: Infoscience - EPFL scientific publicationshttps://doi.org/10.48550/arxiv...Article . 2018License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint 2018Publisher:MDPI AG Authors: Soebur Razzaque; Lili Yang;Soebur Razzaque; Lili Yang;The origin of sub-TeV gamma rays detected by Fermi-LAT from the Fermi bubbles at the Galactic center is still unknown. In a hadronic model, acceleration of protons and/or nuclei and their subsequent interactions with gas in the bubble volume can produce observed gamma rays. Such interactions naturally produce high-energy neutrinos, and detection of those can discriminate between a hadronic and a leptonic origin of gamma rays. Additional constraints on the Fermi bubbles gamma-ray flux in the TeV range from recent HAWC observations restrict hadronic model parameters, which in turn disfavor Fermi bubbles as the origin of a large fraction of neutrino events detected by IceCube along the bubble directions. We revisit our hadronic model and discuss future constraints on parameters from observations in very high-energy gamma rays and neutrinos. Comment: 9 pages, 4 figures. Invited article submitted to MDPI journal Galaxies for its special issue, Searching for Connections among the Fermi Bubbles, the Galactic Center GeV Excess, and Loop I, edited by D. Malyshev
Galaxies arrow_drop_down GalaxiesOther literature type . Article . 2018 . Peer-reviewedLicense: CC BYFull-Text: http://www.mdpi.com/2075-4434/6/2/47/pdfhttps://doi.org/10.48550/arxiv...Article . 2018License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.euAccess RoutesGreen gold 9 citations 9 popularity Top 10% influence Average impulse Average Powered by BIP!more_vert Galaxies arrow_drop_down GalaxiesOther literature type . Article . 2018 . Peer-reviewedLicense: CC BYFull-Text: http://www.mdpi.com/2075-4434/6/2/47/pdfhttps://doi.org/10.48550/arxiv...Article . 2018License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Preprint , Article 2020 Czech Republic, France, ItalyPublisher:EDP Sciences Ester Antonucci; Marco Romoli; Vincenzo Andretta; Silvano Fineschi; Petr Heinzel; J. Daniel Moses; Giampiero Naletto; Gianalfredo Nicolini; D. Spadaro; Luca Teriaca; A. Berlicki; Gerardo Capobianco; Giuseppe Crescenzio; Vania Da Deppo; Mauro Focardi; Fabio Frassetto; K. Heerlein; Federico Landini; Enrico Magli; A. M. Malvezzi; Giuseppe Massone; Radek Melich; Piergiorgio Nicolosi; Giancarlo Noci; Maurizio Pancrazzi; Maria G. Pelizzo; Luca Poletto; Clementina Sasso; Udo Schühle; Sami K. Solanki; Leonard Strachan; Roberto Susino; Giuseppe Tondello; Michela Uslenghi; Joachim Woch; Lucia Abbo; Alessandro Bemporad; Marta Casti; S. Dolei; Catia Grimani; Mauro Messerotti; Marco Ricci; Thomas Straus; Daniele Telloni; Paola Zuppella; Frédéric Auchère; Roberto Bruno; Angela Ciaravella; Alain Jody Corso; Miguel Alvarez Copano; Regina Aznar Cuadrado; Raffaella D'Amicis; R. Enge; Alessio Gravina; Sonja Jejčič; Philippe Lamy; A. C. Lanzafame; Thimo Meierdierks; Ioanna Papagiannaki; Hardi Peter; German Fernandez Rico; M.G. Sertsu; Jan Staub; Kanaris Tsinganos; Marco Velli; Rita Ventura; Enrico Verroi; Jean-Claude Vial; Sébastien Vivès; Antonio Volpicelli; Stephan Werner; Andreas Zerr; Barbara Negri; Marco Castronuovo; Alessandro Gabrielli; R. Bertacin; Rita Carpentiero; Silvia Natalucci; F. Marliani; Marco Cesa; Philippe Laget; Danilo Morea; Stefano Pieraccini; Paolo Radaelli; Paolo Sandri; Paolo Sarra; Stefano Cesare; Felice Del Forno; Ernesto Massa; Mauro Montabone; Sergio Mottini; Daniele Quattropani; Tiziano Schillaci; Roberto Boccardo; Rosario Brando; Arianna Pandi; Cristian Baietto; Riccardo Bertone; Alberto Álvarez-Herrero; Pilar García Parejo; María Cebollero; Mauro Amoruso; Vito Centonze;handle: 2318/1834172 , 11576/2669637 , 20.500.11769/491734 , 11583/2847550 , 2158/1217265 , 11577/3352909 , 11104/0313131
Aims. Metis is the first solar coronagraph designed for a space mission and is capable of performing simultaneous imaging of the off-limb solar corona in both visible and UV light. The observations obtained with Metis aboard the Solar Orbiter ESA-NASA observatory will enable us to diagnose, with unprecedented temporal coverage and spatial resolution, the structures and dynamics of the full corona in a square field of view (FoV) of ±2.9° in width, with an inner circular FoV at 1.6°, thus spanning the solar atmosphere from 1.7R⊙to about 9R⊙, owing to the eccentricity of the spacecraft orbit. Due to the uniqueness of the Solar Orbiter mission profile, Metis will be able to observe the solar corona from a close (0.28 AU, at the closest perihelion) vantage point, achieving increasing out-of-ecliptic views with the increase of the orbit inclination over time. Moreover, observations near perihelion, during the phase of lower rotational velocity of the solar surface relative to the spacecraft, allow longer-term studies of the off-limb coronal features, thus finally disentangling their intrinsic evolution from effects due to solar rotation.Methods. Thanks to a novel occultation design and a combination of a UV interference coating of the mirrors and a spectral bandpass filter, Metis images the solar corona simultaneously in the visible light band, between 580 and 640 nm, and in the UV H ILyman-αline at 121.6 nm. The visible light channel also includes a broadband polarimeter able to observe the linearly polarised component of the K corona. The coronal images in both the UV H ILyman-αand polarised visible light are obtained at high spatial resolution with a spatial scale down to about 2000 km and 15 000 km at perihelion, in the cases of the visible and UV light, respectively. A temporal resolution down to 1 s can be achieved when observing coronal fluctuations in visible light.Results. The Metis measurements, obtained from different latitudes, will allow for complete characterisation of the main physical parameters and dynamics of the electron and neutral hydrogen/proton plasma components of the corona in the region where the solar wind undergoes the acceleration process and where the onset and initial propagation of coronal mass ejections (CMEs) take place. The near-Sun multi-wavelength coronal imaging performed with Metis, combined with the unique opportunities offered by the Solar Orbiter mission, can effectively address crucial issues of solar physics such as: the origin and heating/acceleration of the fast and slow solar wind streams; the origin, acceleration, and transport of the solar energetic particles; and the transient ejection of coronal mass and its evolution in the inner heliosphere, thus significantly improving our understanding of the region connecting the Sun to the heliosphere and of the processes generating and driving the solar wind and coronal mass ejections.Conclusions. This paper presents the scientific objectives and requirements, the overall optical design of the Metis instrument, the thermo-mechanical design, and the processing and power unit; reports on the results of the campaigns dedicated to integration, alignment, and tests, and to the characterisation of the instrument performance; describes the operation concept, data handling, and software tools; and, finally, the diagnostic techniques to be applied to the data, as well as a brief description of the expected scientific products. The performance of the instrument measured during calibrations ensures that the scientific objectives of Metis can be pursued with success.
Archivio Istituziona... arrow_drop_down Archivio Istituzionale (AperTO); Archivio istituzionale della ricerca - Università di Padova; IRIS - Università degli Studi di Catania; Astronomy and Astrophysics; Publications Open Repository TOrino; Archivio istituzionale della ricerca - Università di UrbinoArticle . 2020 . 2019 . Peer-reviewedLicense: EDP Sciences Copyright and Publication Licensing PolicyRepository of the Czech Academy of SciencesArticle . 2020Data sources: Repository of the Czech Academy of SciencesRepository of the Czech Academy of SciencesArticle . 2020Data sources: Repository of the Czech Academy of SciencesIRIS - Università degli Studi di CataniaArticle . 2020Data sources: IRIS - Università degli Studi di CataniaMémoires en Sciences de l'Information et de la CommunicationArticle . 2020Flore (Florence Research Repository)Article . 2020Data sources: Flore (Florence Research Repository)https://doi.org/10.48550/arxiv...Article . 2019License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.euAccess RoutesGreen bronze 114 citations 114 popularity Top 1% influence Top 10% impulse Top 1% Powered by BIP!more_vert Archivio Istituziona... arrow_drop_down Archivio Istituzionale (AperTO); Archivio istituzionale della ricerca - Università di Padova; IRIS - Università degli Studi di Catania; Astronomy and Astrophysics; Publications Open Repository TOrino; Archivio istituzionale della ricerca - Università di UrbinoArticle . 2020 . 2019 . Peer-reviewedLicense: EDP Sciences Copyright and Publication Licensing PolicyRepository of the Czech Academy of SciencesArticle . 2020Data sources: Repository of the Czech Academy of SciencesRepository of the Czech Academy of SciencesArticle . 2020Data sources: Repository of the Czech Academy of SciencesIRIS - Università degli Studi di CataniaArticle . 2020Data sources: IRIS - Università degli Studi di CataniaMémoires en Sciences de l'Information et de la CommunicationArticle . 2020Flore (Florence Research Repository)Article . 2020Data sources: Flore (Florence Research Repository)https://doi.org/10.48550/arxiv...Article . 2019License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint 2019Publisher:Oxford University Press (OUP) U. Munari; Joshi; Debabrata Banerjee; Klemen Čotar; Sergei Yu. Shugarov; Rajka Jurdana-Šepić; R. Belligoli; A Bergamini; M. Graziani; G. L. Righetti; A. Vagnozzi; P. Valisa;We have been monitoring, at high cadence, the photometric and spectroscopic evolution of VES 263 following the discovery in 2018 of a brightening labeled as event Gaia-18azl. VES 263 is so far a neglected emission-line object discovered in the 1960s on objective prism plates, tentatively classified as a semi-regular AGB cool giant by automated analysis of ASASSN lightcurves. We have discovered that VES 263 is a bonafide massive pre-Main Sequence object (~12 Msun), of the Herbig AeBe type. It is located at 1.68+/-0.07 kpc distance, within the Cyg OB2 star-forming region, and it is highly reddened (E(B-V)=1.80+/-0.05) by interstellar extinction. In quiescence, the spectral energy distribution is dominated by the 20,000 K photospheric emission from the central B1II star, and at wavelenghts >=6 micron by emission from circumstellar warm dust (Tdust up to 400 K). The 2018-19 eruption was caused by a marked brightening of the accretion disk around the B1II star as traced by the evolution with time of the integrated flux and the double-peaked profile of emission lines. At the peak of the eruption, the disk has a bulk temperature of ~7500 K and a luminosity L>=860 Lsun, corresponding to a mass accretion rate >=1.1x10(-5) Msun/yr. Spectroscopic signature of possible bipolar jets (at -700 and +700 km/s) of variable intensity are found. We have reconstructed from Harvard, Moscow and Sonneberg photographic plates the photometric history of VES 263 from 1896 to 1995, showing through 1953-1969 a state much brighter than current eruption. To appear in MNRAS
Monthly Notices of t... arrow_drop_down Monthly Notices of the Royal Astronomical SocietyArticle . 2019 . Peer-reviewedLicense: OUP Standard Publication ReuseData sources: Crossrefhttps://doi.org/10.48550/arxiv...Article . 2019License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.euAccess RoutesGreen hybrid 5 citations 5 popularity Top 10% influence Average impulse Average Powered by BIP!more_vert Monthly Notices of t... arrow_drop_down Monthly Notices of the Royal Astronomical SocietyArticle . 2019 . Peer-reviewedLicense: OUP Standard Publication ReuseData sources: Crossrefhttps://doi.org/10.48550/arxiv...Article . 2019License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1093/mnras/stz2078&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint , Conference object 2019Embargo end date: 01 Jan 2019 Spain, FrancePublisher:arXiv Ballester, Otger; Blanch, Oscar; Boix, Joan; Bregeon, Johan; Brun, Patrick; Çolak, §ıdıka Merve; Doro, Michele; Da Deppo, Vania; Font, Lluís; Gabella, Omar; García-Tenorio García-Balmaseda, Rafael; Gaug, Markus; Maggio, Camilla; Martínez, Manel Cruz; Martínez, Óscar; Adrover, Pere Munar; Ramos, Raúl; Rivoire, Stephane; Staniˇc, Samo; Villar, David; Vasileiadis, George; Wang, Longlong; Zavrtanik, Marko;International audience; The Cherenkov Telescope Array (CTA) is the next generation ground based observatory for gamma ray astronomy at very high energies. Employing more than 100 Imaging Atmospheric Cherenkov Telescopes in the northern and southern hemispheres, it was designed to reach unprecedented sensitivity and energy resolution. Understanding and correcting for systematic biases on the absolute energy scale and instrument response functions will be a crucial issue for the performance of CTA. The LUPM group and the Spanish/Italian/Slovenian collaboration are currently building two Raman LIDAR prototypes for the online atmospheric calibration along the line of sight of the CTA. Requirements for such a solution include the ability to characterize aerosol extinction at two wavelengths to distances of 30 km with an accuracy better than 5%, within time scales of about a minute, steering capabilities and close interaction with the CTA array control and data acquisition system as well as other auxiliary instruments. Our Raman LIDARs have design features that make them different from those used in atmospheric science and are characterized by large collecting mirrors (2.5 m2), liquid light guides that collect the light at the focal plane and transport it to the readout system, reduced acquisition time and highly precise Raman spectrometers. The Raman LIDARs will participate in a cross calibration and characterization campaign of the atmosphere at the CTA North site at La Palma, together with other site characterization instruments. After a one year test period there, an in depth evaluation of the solutions adopted by the two projects will lead to a final Raman LIDAR design proposal for both CTA sites.
Recolector de Cienci... arrow_drop_down Recolector de Ciencia Abierta, RECOLECTA; idUS. Depósito de Investigación de la Universidad de Sevilla.Conference object . 2020 . 2019License: CC BY NC NDFull-Text: https://pos.sissa.it/358/814/pdfhttps://doi.org/10.48550/arxiv...Article . 2019License: arXiv Non-Exclusive DistributionData sources: DataciteHAL - UPEC / UPEM; HAL-Pasteur; HAL-InsermConference object . 2019add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.euAccess RoutesGreen 0 citations 0 popularity Average influence Average impulse Average Powered by BIP!more_vert Recolector de Cienci... arrow_drop_down Recolector de Ciencia Abierta, RECOLECTA; idUS. Depósito de Investigación de la Universidad de Sevilla.Conference object . 2020 . 2019License: CC BY NC NDFull-Text: https://pos.sissa.it/358/814/pdfhttps://doi.org/10.48550/arxiv...Article . 2019License: arXiv Non-Exclusive DistributionData sources: DataciteHAL - UPEC / UPEM; HAL-Pasteur; HAL-InsermConference object . 2019add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint 2022 ItalyPublisher:EDP Sciences A. Bemporad; V. Andretta; R. Susino; S. Mancuso; D. Spadaro; M. Mierla; D. Berghmans; E. D’Huys; A. N. Zhukov; D.-C. Talpeanu; R. Colaninno; P. Hess; J. Koza; S. Jejčič; P. Heinzel; E. Antonucci; V. Da Deppo; S. Fineschi; F. Frassati; G. Jerse; F. Landini; G. Naletto; G. Nicolini; M. Pancrazzi; M. Romoli; C. Sasso; A. Slemer; M. Stangalini; L. Teriaca;On February 12, 2021 two subsequent eruptions occurred above the West limb, as seen along the Sun-Earth line. The first event was a typical slow Coronal Mass Ejection (CME), followed $\sim 7$ hours later by a smaller and collimated prominence eruption, originating Southward with respect to the CME, followed by a plasma blob. These events were observed not only by SOHO and STEREO-A missions, but also by the suite of remote sensing instruments on-board Solar Orbiter (SolO). This work shows how data acquired by the Full Sun Imager (FSI), Metis coronagraph, and Heliospheric Imager (SoloHI) from the SolO perspective can be combined to study the eruptions and the different source regions. Moreover, we show how Metis data can be analyzed to provide new information about solar eruptions. Different 3D reconstruction methods were applied to the data acquired by different spacecraft including remote sensing instruments on-board SolO. Images acquired by both Metis channels in the Visible Light (VL) and H I Lyman$-\alpha$ line (UV) were combined to derive physical information on the expanding plasma. The polarization ratio technique was also applied for the first time to the Metis images acquired in the VL channel. The two eruptions were followed in 3D from their source region to their expansion in the intermediate corona. Thanks to the combination of VL and UV Metis data, the formation of a post-CME Current Sheet (CS) was followed for the first time in the intermediate corona. The plasma temperature gradient across a post-CME blob propagating along the CS was also measured for the first time. Application of the polarization ratio technique to Metis data shows that, thanks to the combination of four different polarization measurements, the errors are reduced by $\sim 5-7$\%, thus better constraining the 3D distribution of plasma. Comment: 15 pages, 14 figures, accepted for publication on A&A
Flore (Florence Rese... arrow_drop_down Flore (Florence Research Repository); Astronomy and AstrophysicsArticle . 2022 . Peer-reviewedLicense: EDP Sciences Copyright and Publication Licensing PolicyFlore (Florence Research Repository)Article . 2022Data sources: Flore (Florence Research Repository)https://doi.org/10.48550/arxiv...Article . 2022License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.euAccess RoutesGreen 6 citations 6 popularity Top 10% influence Average impulse Top 10% Powered by BIP!more_vert Flore (Florence Rese... arrow_drop_down Flore (Florence Research Repository); Astronomy and AstrophysicsArticle . 2022 . Peer-reviewedLicense: EDP Sciences Copyright and Publication Licensing PolicyFlore (Florence Research Repository)Article . 2022Data sources: Flore (Florence Research Repository)https://doi.org/10.48550/arxiv...Article . 2022License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Other literature type , Preprint 2020 Belgium, Italy, Italy, Italy, Netherlands, Italy, Italy, Italy, Italy, Brazil, Italy, Germany, France, Belgium, Czech Republic, Spain, GermanyPublisher:IOP Publishing Funded by:NSF | Pierre Auger ProjectNSF| Pierre Auger ProjectAuthors: Marco Aglietta; Jaime Alvarez-Muñiz; R. Alves Batista; Gioacchino Alex Anastasi; +214 AuthorsMarco Aglietta; Jaime Alvarez-Muñiz; R. Alves Batista; Gioacchino Alex Anastasi; Luis A. Anchordoqui; B. Andrada; P.R. Araújo Ferreira; Hernán Asorey; Pedro Assis; Gualberto Avila; Alena Bakalova; F. C. T. Barbato; K.-H. Becker; Jose A. Bellido; Corinne Berat; M. E. Bertaina; Xavier Bertou; Peter L. Biermann; Teresa Bister; Jonathan Biteau; A. Blanco; Carla Bleve; Martina Bohacova; Denise Boncioli; Carla Bonifazi; L. Bonneau Arbeletche; Nataliia Borodai; Jeffrey Brack; Thomas Bretz; A. Bridgeman; Peter Buchholz; Antonio Bueno; Stijn Buitink; Mario Buscemi; Karen S. Caballero-Mora; Lorenzo Caccianiga; Fabrizia Canfora; Rossella Caruso; Antonella Castellina; G. Cataldi; Lorenzo Cazon; Jose Chinellato; J. Chudoba; Roger W Clay; Roberta Colalillo; Alan Coleman; Giovanni Consolati; Fernando Contreras; Fabio Convenga; Corbin Covault; Kai Daumiller; Bruce R. Dawson; R. M. de Almeida; J. de Jesús; S. J. De Jong; G. De Mauro; J. de Oliveira; D. de Oliveira Franco; J. Debatin; A. Di Matteo; R.C. dos Anjos; Jan Ebr; Italo Epicoco; Martin Erdmann; G. Farrar; A. C. Fauth; N. Fazzini; Francesco Fenu; Juan Manuel Figueira; Tomáš Fodran; Toshihiro Fujii; Cristina Galea; H. Gemmeke; Flavia Gesualdi; Alexandru Gherghel-Lascu; Ugo Giaccari; Jonas Glombitza; G. Golup; Juan Pablo Gongora; Nicolás González; Dariusz Gora; Alessio Gorgi; Marvin Gottowik; F. Guarino; G. P. Guedes; Eleonora Guido; M. R. Hampel; D. Harari; Violet M. Harvey; A. Haungs; Thomas Hebbeker; D. Heck; C. Hojvat; Pavel Horvath; Miroslav Hrabovský; T. Huege; A. Insolia; Paula Gina Isar; Jeffrey A. Johnsen; Jakub Juryšek; B. Keilhauer; Julian Kemp; B. L. Lago; Vladimir Lenok; A. Letessier-Selvon; D. Lo Presti; L. Lopes; A. Machado Payeras; Dusan Mandat; B. C. Manning; Sullivan Marafico; Ioana Codrina Maris; G. Marsella; H. Martinez; Massimo Mastrodicasa; John Matthews; Eric Mayotte; P.O. Mazur; G. Medina-Tanco; A. Menshikov; Kevin-Druis Merenda; Stanislav Michal; M. I. Micheletti; Lino Miramonti; Silvia Mollerach; C. Morello; Miguel Mostafa; Alfred Müller; M. A. Muller; W. M. Namasaka; Mihai Niculescu-Oglinzanu; Marcus Niechciol; D. Nosek; M. Palatka; J. Pallotta; M.P. Panetta; Philipp Papenbreer; G. Parente; A. Parra; F. Pedreira; Rodrigo Pelayo; Jesús Peña-Rodríguez; J. Perez Armand; Christine Peters; S. Petrera; T. Pierog; Valerio Pirronello; M. Platino; M. Pothast; S. Querchfeld; Maximilian Reininghaus; F. Riehn; M. Risse; Vincenzo Rizi; W. Rodrigues de Carvalho; J. Rodriguez Rojo; Markus Roth; Esteban Roulet; A. C. Rovero; P. Ruehl; F. Salamida; G. Salina; E. Santos; Fred Sarazin; Raul Sarmento; Christian Sarmiento-Cano; P. Savina; C. M. Schäfer; V. Scherini; M. Schimp; Felix Schlüter; Frank G. Schröder; S. Schröder; André Schulz; S. J. Sciutto; Marina Scornavacche; R. C. Shellard; Günter Sigl; Gaia Silli; Octavian Sima; Radomir Smida; Paul Sommers; Julien Souchard; R. Squartini; Maximilian Stadelmaier; Samo Stanič; J. Stasielak; J. Šupík; Charles Timmermans; Olena Tkachenko; B. Tome; G. Torralba Elipe; Andres Travaini; Petr Travnicek; Caterina Trimarelli; M. Trini; Matias Tueros; Ralf Ulrich; M. Urban; Lukáš Vaclavek; Martin Vacula; A. van Vliet; E. Varela; B. Vargas Cárdenas; Carlo Ventura; I.D. Vergara Quispe; Luis Villaseñor; Marc Weber; A. Weindl; L. R. Wiencke; M. Wirtz; David Wittkowski; B. Wundheiler; A. Yushkov; Orazio Zapparrata; Enrique Zas; M. Zavrtanik; Francesca Zuccarello;doi: 10.1088/1748-0221/15/10/p10021 , 10.5445/ir/1000125360 , 10.48550/arxiv.2007.09035 , 10.18154/rwth-2021-02045
handle: 11245.1/25389f08-b24d-4f82-bc0b-d164100f717f , 11311/1152632 , 11370/f58e1a6c-b4a8-453b-8710-48cf4e4f7433 , 10481/66661 , 20.500.14017/635365e9-9a46-46aa-9417-1bac709feb8f , 11697/153436 , 20.500.11769/497650 , 2066/230078 , 10447/469211 , 11588/826320 , 11104/0316156 , https://repository.ubn.ru.nl/handle/2066/230078 , 2318/1803310 , 11587/447686
doi: 10.1088/1748-0221/15/10/p10021 , 10.5445/ir/1000125360 , 10.48550/arxiv.2007.09035 , 10.18154/rwth-2021-02045
handle: 11245.1/25389f08-b24d-4f82-bc0b-d164100f717f , 11311/1152632 , 11370/f58e1a6c-b4a8-453b-8710-48cf4e4f7433 , 10481/66661 , 20.500.14017/635365e9-9a46-46aa-9417-1bac709feb8f , 11697/153436 , 20.500.11769/497650 , 2066/230078 , 10447/469211 , 11588/826320 , 11104/0316156 , https://repository.ubn.ru.nl/handle/2066/230078 , 2318/1803310 , 11587/447686
Cosmic rays arriving at Earth collide with the upper parts of the atmosphere, thereby inducing extensive air showers. When secondary particles from the cascade arrive at the ground, they are measured by surface detector arrays. We describe the methods applied to the measurements of the surface detector of the Pierre Auger Observatory to reconstruct events with zenith angles less than 60 using the timing and signal information recorded using the water-Cherenkov detector stations. In addition, we assess the accuracy of these methods in reconstructing the arrival directions of the primary cosmic ray particles and the sizes of the induced showers. Czech Republic Grant MSMT CR LTT18004 LM2015038 LM2018102 CZ.02.1.01/0.0/0.0/16_013/0001402 CZ.02.1.01/0.0/0.0/18_046/0016010 CZ.02.1.01/0.0/0.0/17_049/0008422 Portugal - FEDER funds within Programa Operacional Factores de Competitividade through Fundacao para a Ciencia e a Tecnologia (COMPETE) Romania - Romanian Ministry of Education and Research, the Program Nucleu within PNCDI III PN-III-P11.2-PCCDI-2017-0839/19PCCDI/2018 Poland - National Science Centre 2013/08/M/ST9/00322 2016/23/B/ST9/01635 HARMONIA 52013/10/M/ST9/00062 UMO-2016/22/M/ST9/00198 Romania - Romanian Ministry of Education and Research, the Program Nucleu within MCI PN19150201/16N/2019 PN19060102 United States Department of Energy (DOE) DE-AC02-07CH11359 DE-FR02-04ER41300 DEFG02-99ER41107 DE-SC0011689 Fundacao de Amparo a Pesquisa do Estado de Sao Paulo (FAPESP) 2019/10151-2 2010/07359-6 1999/05404-3 Germany - Min-isterium fur Innovation, Wissenschaft und Forschung des Landes Nordrhein-Westfalen Spain - Ministerio de Economía, Industria y Competitividad FPA2017-85114-P FPA2017-85197-P Carlos Chagas Filho Foundation for Research Support of the State of Rio de Janeiro (FAPERJ) Germany - Ministerium fur Wissenschaft, Forschung und Kunst des Landes Baden-Wurttemberg Argentina - Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET) French National Research Agency (ANR) LABEX ANR-10-LABX-63 ANR11-IDEX-0004-02 Brazil - Ministerio da Ciencia, Tecnologia, Inovacoes e Comunicacoes (MCTIC) Argentina - Agencia Nacional de Promoción Científica y Tecnológica (ANPCyT) Spain - RENATARedNacional Tematica de Astroparticulas FPA2015-68783-REDT Italy - Ministero dell'Istruzione, dell'Universita e della Ricerca (MIUR) France - Departement Physique Nucleaire et Corpusculaire (PNC-IN2P3/CNRS) Slovenian Research Agency - Slovenia P1-0031 P1-0385 I0-0033 N1-0111 National Council for Scientific and Technological Development (CNPq) Germany - Helmholtz-Gemeinschaft Deutscher Forschungszentren (HGF) Poland - Ministry of Science and Higher Education DIR/WK/2018/11 Germany - Helmholtz Alliance for Astroparticle Physics (HAP) The Netherlands - Ministry of Education, Culture and Science France - Departement Sciences de l'Univers (SDU-INSU/CNRS) Consejo Nacional de Ciencia y Tecnología (CONACyT) 167733 U.S.A. - European Particle Physics Latin American Network Spain - Maria de MaeztuUnit of Excellence MDM-2016-0692 México - Universidad Nacional Autónoma de México (UNAM) Netherlands Organization for Scientific Research (NWO) Italy - Istituto Nazionale di Fisica Nucleare (INFN) Brazil - Financiadora de Estudos e Projetos (FINEP) Centre National de la Recherche Scientifique (CNRS) The Netherlands - Dutch national e-infrastructure Italy - Istituto Nazionale di Astrofisica (INAF) Argentina - Comisión Nacional de Energía Atómica Federal Ministry of Education & Research (BMBF) Argentina - Gobierno de la Provincia de Mendoza Germany - Finanzministerium Baden-Wurttemberg Italy - Ministero degli Affari Esteri (MAE) National Science Foundation (NSF) 0450696 Spain - Xunta de Galicia ED431C 2017/07 Australia - Australian Research Council France - Conseil Regional Ile-de-France Argentina - Municipalidad de Malargue France - Centre de Calcul IN2P3/CNRS Italy - CETEMPS Center of Excellence Portugal - Portuguese national funds Junta de Andalucía SOMM17/6104/UGR U.S.A. - Marie Curie-IRSES/EPLANET The Netherlands - SURF Cooperative German Research Foundation (DFG) U.S.A. - Grainger Foundation Argentina - Valle Las Lenas México - PAPIIT DGAPA-UNAM Argentina - NDM Holdings Spain - Feder Funds U.S.A. - UNESCO
NARCIS arrow_drop_down Archivio Istituzionale della Ricerca - Università degli Studi dell Aquila; Archivio Istituzionale della Ricerca- Università del Salento; Journal of Instrumentation; Archivio istituzionale della ricerca - Università di Palermo; Recolector de Ciencia Abierta, RECOLECTA; IRIS - Università degli Studi di Catania; METIS Research Information System; Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual) - Universidade de São Paulo (USP); Archivio della ricerca - Università degli studi di Napoli Federico II; RE.PUBLIC@POLIMI Research Publications at Politecnico di MilanoArticle . 2020License: CC BYData sources: Archivio Istituzionale della Ricerca - Università degli Studi dell Aquila; Archivio Istituzionale della Ricerca- Università del Salento; Universiteit van Amsterdam (UvA) Institutional Repository UvA-DARE; University of Groningen Research Portal; Archivio istituzionale della ricerca - Università di Palermo; Recolector de Ciencia Abierta, RECOLECTA; IRIS - Università degli Studi di Catania; LAReferencia - Red Federada de Repositorios Institucionales de Publicaciones Científicas Latinoamericanas; METIS Research Information System; Archivio della ricerca - Università degli studi di Napoli Federico II; RE.PUBLIC@POLIMI Research Publications at Politecnico di MilanoOA@INAF - Istituto Nazionale di AstrofisicaArticle . 2020Data sources: OA@INAF - Istituto Nazionale di AstrofisicaRepository of the Czech Academy of SciencesArticle . 2020Data sources: Repository of the Czech Academy of SciencesRepository of the Czech Academy of SciencesArticle . 2020Data sources: Repository of the Czech Academy of SciencesRadboud Repository; Journal of InstrumentationArticle . 2020Vrije Universiteit Brussel Research PortalOther literature type . 2020Data sources: Vrije Universiteit Brussel Research PortalIRIS - Università degli Studi di CataniaArticle . 2020Data sources: IRIS - Università degli Studi di CataniaRecolector de Ciencia Abierta, RECOLECTA; Repositorio Institucional Universidad de GranadaOther literature type . Article . 2021 . 2020add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.euAccess RoutesGreen hybrid 9 citations 9 popularity Top 10% influence Average impulse Top 10% Powered by BIP!more_vert NARCIS arrow_drop_down Archivio Istituzionale della Ricerca - Università degli Studi dell Aquila; Archivio Istituzionale della Ricerca- Università del Salento; Journal of Instrumentation; Archivio istituzionale della ricerca - Università di Palermo; Recolector de Ciencia Abierta, RECOLECTA; IRIS - Università degli Studi di Catania; METIS Research Information System; Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual) - Universidade de São Paulo (USP); Archivio della ricerca - Università degli studi di Napoli Federico II; RE.PUBLIC@POLIMI Research Publications at Politecnico di MilanoArticle . 2020License: CC BYData sources: Archivio Istituzionale della Ricerca - Università degli Studi dell Aquila; Archivio Istituzionale della Ricerca- Università del Salento; Universiteit van Amsterdam (UvA) Institutional Repository UvA-DARE; University of Groningen Research Portal; Archivio istituzionale della ricerca - Università di Palermo; Recolector de Ciencia Abierta, RECOLECTA; IRIS - Università degli Studi di Catania; LAReferencia - Red Federada de Repositorios Institucionales de Publicaciones Científicas Latinoamericanas; METIS Research Information System; Archivio della ricerca - Università degli studi di Napoli Federico II; RE.PUBLIC@POLIMI Research Publications at Politecnico di MilanoOA@INAF - Istituto Nazionale di AstrofisicaArticle . 2020Data sources: OA@INAF - Istituto Nazionale di AstrofisicaRepository of the Czech Academy of SciencesArticle . 2020Data sources: Repository of the Czech Academy of SciencesRepository of the Czech Academy of SciencesArticle . 2020Data sources: Repository of the Czech Academy of SciencesRadboud Repository; Journal of InstrumentationArticle . 2020Vrije Universiteit Brussel Research PortalOther literature type . 2020Data sources: Vrije Universiteit Brussel Research PortalIRIS - Università degli Studi di CataniaArticle . 2020Data sources: IRIS - Università degli Studi di CataniaRecolector de Ciencia Abierta, RECOLECTA; Repositorio Institucional Universidad de GranadaOther literature type . Article . 2021 . 2020add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Preprint , Article 2020Publisher:Elsevier BV Authors: Rok Vogrinčič; Alejandro Lara; Andrea Borgazzi; Jean-Pierre Raulin;Rok Vogrinčič; Alejandro Lara; Andrea Borgazzi; Jean-Pierre Raulin;The altitude of the ionospheric lower layer (D-region) is highly influenced by the solar UV flux affecting in turn, the propagation of Very Low Frequency (VLF) signals inside the waveguide formed between this layer and the Earth surface. A rapid change of the solar irradiance, as during a solar eclipse, can help to understand the details of the energy transfer of the solar radiation onto the ionospheric D-layer. Using the "Latin American VLF Network" (LAVNet-Mex) receiver station in Mexico City, Mexico, we detected the phase and amplitude changes of the VLF signals transmitted by the NDK station at 25.2 kHz in North Dakota, USA during the August 21, 2017, solar eclipse. As the Sunlight was eclipsed, the rate of ionization in the ionosphere (D-region) was reduced and the effective reflection height increased, causing a considerable drop of the phase and amplitude of the observed VLF waves. The corresponding waveguide path is 3007.15 km long and crossed almost perpendicularly the total eclipse path. Circumstantially, at the time of the total eclipse, a C3 flare took place allowing us to isolate the flare flux from the background flux of a large portion of the disk. In this work, we report the observations and present a new model of the ionospheric effects of the eclipse and flare. The model is based on a detailed setup of the degree of Moon shadow that affects the entire Great Circle Path (GCP). During the eclipse, the maximum phase variation was -63.36$^{\circ}$ at 18:05 UT which, according to our model, accounts for a maximum increase of the reflection height of 9.3 km. Comment: 23 pages, 5 figures, appendix A and B, accepted for publication in Advances in Space Research
arXiv.org e-Print Ar... arrow_drop_down Advances in Space ResearchArticle . 2020 . Peer-reviewedLicense: Elsevier TDMData sources: Crossrefhttps://doi.org/10.48550/arxiv...Article . 2019License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.euAccess RoutesGreen bronze 7 citations 7 popularity Top 10% influence Average impulse Top 10% Powered by BIP!more_vert arXiv.org e-Print Ar... arrow_drop_down Advances in Space ResearchArticle . 2020 . Peer-reviewedLicense: Elsevier TDMData sources: Crossrefhttps://doi.org/10.48550/arxiv...Article . 2019License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Other literature type , Article , Preprint 2021 Italy, Belgium, Germany, Brazil, Italy, Italy, Italy, Netherlands, Italy, Belgium, Italy, France, ItalyPublisher:IOP Publishing Funded by:NSF | Pierre Auger ProjectNSF| Pierre Auger ProjectA. Aab; P. Abreu; Marco Aglietta; Jaime Alvarez-Muñiz; R. Alves Batista; Gioacchino Alex Anastasi; Belén Andrada; Sofia Andringa; Carla Aramo; P.R. Araújo Ferreira; J. C. Arteaga Velázquez; Hernán Asorey; Pedro Assis; Alena Bakalova; Alexandru Balaceanu; K.-H. Becker; Jose A. Bellido; Corinne Berat; M. E. Bertaina; Xavier Bertou; Peter L. Biermann; J. Biteau; Jonathan Blazek; Carla Bleve; Martina Bohacova; Denise Boncioli; L. Bonneau Arbeletche; Nataliia Borodai; Ana Martina Botti; Jeffrey Brack; Thomas Bretz; Florian Lukas Briechle; Peter Buchholz; Antonio Bueno; Stijn Buitink; Mario Buscemi; Karen S. Caballero-Mora; Lorenzo Caccianiga; Ioana Caracas; Rossella Caruso; Antonella Castellina; Fernando Catalani; G. Cataldi; Lorenzo Cazon; Magdalena Cerdá; Jose Chinellato; Ladislav Chytka; Roger W Clay; A.C. Cobos Cerutti; Roberta Colalillo; Alan Coleman; Maria Rita Coluccia; Rúben Conceição; Giovanni Consolati; Fernando Contreras; Fabio Convenga; Corbin Covault; Sergio Dasso; Bruce R. Dawson; R. M. de Almeida; J. de Jesús; G. De Mauro; J. R. T. de Mello Neto; I. De Mitri; E. De Vito; Carola Dobrigkeit; Ralph Engel; Italo Epicoco; Martin Erdmann; Carlos Escobar; A. Etchegoyen; John Farmer; N. Fazzini; Francesco Fenu; Juan Manuel Figueira; Tomáš Fodran; Toshihiro Fujii; A. Fuster; Cristina Galea; B. García; A.L. Garcia Vegas; Flavia Gesualdi; Marco Giammarchi; M. Giller; Jonas Glombitza; G. Golup; M. Gómez Berisso; Juan Pablo Gongora; N. González; Isabel Goos; Dariusz Gora; A. Gorgi; Trent D. Grubb; F. Guarino; G. P. Guedes; Eleonora Guido; Matías Rolf Hampel; Violet M. Harvey; G. C. Hill; Jörg R. Hörandel; Pavel Horvath; A. Insolia; Paula Gina Isar; Petr Janecek; Jakub Juryšek; Alex Kääpä; K. H. Kampert; B. Keilhauer; Julian Kemp; J. Kleinfeller; Rodrigo Guedes Lang; Vladimir Lenok; Antoine Letessier-Selvon; D. Lo Presti; R. López; A. Lucero; Jon Paul Lundquist; G. Mancarella; P. Mantsch; Sullivan Marafico; A. G. Mariazzi; G. Marsella; D. Martello; H. Martinez; John Matthews; G. Matthiae; Eric Mayotte; G. Medina-Tanco; D. Melo; Lino Miramonti; Silvia Mollerach; C. Morello; Katie Mulrey; Roberto Mussa; L. Nellen; Mihai Niculescu-Oglinzanu; Marcus Niechciol; D. Nitz; Luis A. Nunez; M. Palatka; J. Pallotta; A. Parra; J. Pkala; Rodrigo Pelayo; J. Perez Armand; C. Pérez Bertolli; L. Perrone; S. Petrera; T. Pierog; M. Pimenta; Valerio Pirronello; M. Platino; Bjarni Pont; Paolo Privitera; A. Puyleart; Maximilian Reininghaus; F. Riehn; Vincenzo Rizi; W. Rodrigues de Carvalho; Esteban Roulet; P. Ruehl; F. Salamida; Humberto Ibarguen Salazar; G. Salina; J.D. Sanabria Gomez; Fred Sarazin; Raul Sarmento; Christian Sarmiento-Cano; R. Sato; P. Savina; V. Scherini; H. Schieler; M. Schimassek; M. Schimp; Felix Schlüter; Petr Schovanek; Frank G. Schröder; Josina Schulte; A. Segreto; R. C. Shellard; Günter Sigl; Octavian Sima; Radomir Smida; Julien Souchard; Maximilian Stadelmaier; Denis Stanca; Samo Stanič; P. Stassi; A. Streich; M. Suárez-Durán; Tristan Sudholz; T. Suomijärvi; A. Taboada; Olena Tkachenko; P. Tobiska; B. Tome; Matias Tueros; Lukáš Vaclavek; Martin Vacula; J. F. Valdés Galicia; L. Valore; K. C. V. Varma; Darko Veberič; Carlo Ventura; I.D. Vergara Quispe; Valerio Verzi; Hernan Wahlberg; A. Weindl; L. R. Wiencke; Tobias Winchen; M. Wirtz; David Wittkowski; B. Wundheiler; Orazio Zapparrata; Enrique Zas; L. Zehrer; A. Zepeda; R. Cunniffe; J. Eliášek; I. Ebrová; M. Jelínek; P. Kubánek;handle: 11697/168859 , https://repository.ubn.ru.nl/handle/2066/236331 , 11370/00e93631-ebe4-4486-9374-69d5c5d23fb8 , 2066/236331 , 20.500.11769/526700 , 11588/890389 , 11311/1180491 , 2318/1803397 , 11587/458358 , 11245.1/12cefc58-b28a-4488-92a4-53315dbceed2 , 20.500.14017/a580ffd4-97ef-41c7-9d62-48b63eb0c0d6
handle: 11697/168859 , https://repository.ubn.ru.nl/handle/2066/236331 , 11370/00e93631-ebe4-4486-9374-69d5c5d23fb8 , 2066/236331 , 20.500.11769/526700 , 11588/890389 , 11311/1180491 , 2318/1803397 , 11587/458358 , 11245.1/12cefc58-b28a-4488-92a4-53315dbceed2 , 20.500.14017/a580ffd4-97ef-41c7-9d62-48b63eb0c0d6
FRAM (F/Photometric Robotic Atmospheric Monitor) is a robotic telescope operated at the Pierre Auger Observatory in Argentina for the purposes of atmospheric monitoring using stellar photometry. As a passive system which does not produce any light that could interfere with the observations of the fluorescence telescopes of the observatory, it complements the active monitoring systems that use lasers. We discuss the applications of stellar photometry for atmospheric monitoring at optical observatories in general and the particular modes of operation employed by the Auger FRAM. We describe in detail the technical aspects of FRAM, the hardware and software requirements for a successful operation of a robotic telescope for such a purpose and their implementation within the FRAM system. Published version, 27 pages, 8 figures
NARCIS arrow_drop_down Archivio Istituzionale della Ricerca - Università degli Studi dell Aquila; Archivio Istituzionale (AperTO); Archivio Istituzionale della Ricerca- Università del Salento; Journal of Instrumentation; IRIS - Università degli Studi di Catania; METIS Research Information System; Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual) - Universidade de São Paulo (USP); RE.PUBLIC@POLIMI Research Publications at Politecnico di MilanoArticle . 2021Data sources: Archivio Istituzionale della Ricerca - Università degli Studi dell Aquila; Archivio Istituzionale (AperTO); Archivio Istituzionale della Ricerca- Università del Salento; Universiteit van Amsterdam (UvA) Institutional Repository UvA-DARE; University of Groningen Research Portal; IRIS - Università degli Studi di Catania; LAReferencia - Red Federada de Repositorios Institucionales de Publicaciones Científicas Latinoamericanas; METIS Research Information System; RE.PUBLIC@POLIMI Research Publications at Politecnico di MilanoPublikationsserver der RWTH Aachen UniversityPreprint . 2021Data sources: Publikationsserver der RWTH Aachen UniversityIRIS - Università degli Studi di CataniaArticle . 2021Data sources: IRIS - Università degli Studi di CataniaJournal of Instrumentation; Archivio della ricerca - Università degli studi di Napoli Federico IIArticle . 2021 . Peer-reviewedLicense: IOP Copyright PoliciesVrije Universiteit Brussel Research PortalOther literature type . 2021Data sources: Vrije Universiteit Brussel Research Portaladd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.euAccess RoutesGreen bronze 0 citations 0 popularity Average influence Average impulse Average Powered by BIP!more_vert NARCIS arrow_drop_down Archivio Istituzionale della Ricerca - Università degli Studi dell Aquila; Archivio Istituzionale (AperTO); Archivio Istituzionale della Ricerca- Università del Salento; Journal of Instrumentation; IRIS - Università degli Studi di Catania; METIS Research Information System; Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual) - Universidade de São Paulo (USP); RE.PUBLIC@POLIMI Research Publications at Politecnico di MilanoArticle . 2021Data sources: Archivio Istituzionale della Ricerca - Università degli Studi dell Aquila; Archivio Istituzionale (AperTO); Archivio Istituzionale della Ricerca- Università del Salento; Universiteit van Amsterdam (UvA) Institutional Repository UvA-DARE; University of Groningen Research Portal; IRIS - Università degli Studi di Catania; LAReferencia - Red Federada de Repositorios Institucionales de Publicaciones Científicas Latinoamericanas; METIS Research Information System; RE.PUBLIC@POLIMI Research Publications at Politecnico di MilanoPublikationsserver der RWTH Aachen UniversityPreprint . 2021Data sources: Publikationsserver der RWTH Aachen UniversityIRIS - Università degli Studi di CataniaArticle . 2021Data sources: IRIS - Università degli Studi di CataniaJournal of Instrumentation; Archivio della ricerca - Università degli studi di Napoli Federico IIArticle . 2021 . Peer-reviewedLicense: IOP Copyright PoliciesVrije Universiteit Brussel Research PortalOther literature type . 2021Data sources: Vrije Universiteit Brussel Research Portaladd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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