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description Publicationkeyboard_double_arrow_right Article , Conference object 2023Publisher:Oxford University Press (OUP) Meryame Jabbade; Abdellatif Nachab; Elmokhtar Elouardi; Abdel-Mjid Nourreddine; Ezzoura Errami; Mohammed Benjelloun; Mohammed Fahad;doi: 10.1093/rpd/ncad172
pmid: 37934986
Abstract A study of the influence of moisture content on the radon exhalation rate from phosphate samples (with and without consideration of the back diffusion effect) was performed using the sealed cup technique. The mass exhalation rate was found to increase with an increase in moisture content, reaching a maximum value of 2.414 ± 0.034 Bq kg−1 h−1 with a moisture content of 10%. However, the mass exhalation rate decreased with a continued increase in moisture content above 25%. The mass exhalation rate was also measured at different temperatures between −10 and 50°C. The obtained results show that the mass exhalation rate increases linearly with temperature. We point out that all the obtained values of radon exhalation rate are lower than the world average radon exhalation rate (57.6 Bq m−2 h−1).
Radiation Protection... arrow_drop_down Radiation Protection DosimetryArticle . 2023 . Peer-reviewedLicense: OUP Standard Publication ReuseData sources: CrossrefMémoires en Sciences de l'Information et de la CommunicationConference object . 2022add 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 Routesbronze 0 citations 0 popularity Average influence Average impulse Average Powered by BIP!more_vert Radiation Protection... arrow_drop_down Radiation Protection DosimetryArticle . 2023 . Peer-reviewedLicense: OUP Standard Publication ReuseData sources: CrossrefMémoires en Sciences de l'Information et de la CommunicationConference object . 2022add 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 Conference object 2023 France EnglishPublisher:HAL CCSD Authors: Melleton, Jérémie; Pizzocolo, Francesco; Bertrand, Guillaume;Melleton, Jérémie; Pizzocolo, Francesco; Bertrand, Guillaume;International audience; The underground holds indispensable resources for European society, but they need a careful management relying on shared knowledge. To address transnational and continental-scale subsurface problems, geoscientific data need to be harmonized beyond national borders.Started in September 2022 for a duration of five years and based on these principles, GSEU has the following objectives:-To develop pan-European harmonised data and related information services with a focus on critical raw materials, geothermal energy resources and subsurface storage capacities for sustainable energy carriers and CO2 sequestration, groundwater dynamics and quality, geological and climate change information for coastal vulnerability assessment and geological baseline information;-To establish the European Centre of Excellence on Sustainable Resource Management to promote the deployment of the United Nations Framework Classification for Resources (UNFC) and the United Nations Resource Management System (UNRMS);-To develop the geological data infrastructure - building on the existing EGDI - to provide permanent access to and dissemination of the data and information services developed under the project;-To provide a common European Geological Knowledge Base Platform as the single open access portal to the project results and to the underlying data and information collections and infrastructures of partners at national and regional level;-To further strengthen the network of national and regional geological survey organisations to provide geological knowledge and services in a sustainable manner.
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For further information contact us at helpdesk@openaire.eu0 citations 0 popularity Average influence Average impulse Average Powered by BIP!more_vert 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=od______3379::c6bb98df75483087e3c32dfeed9d53f6&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Conference object , Article 2023 FrancePublisher:Cellule MathDoc/CEDRAM Authors: Daviet, Sylvie; Schleyer-Lindenmann, Alexandra; Raynal, Jean-Claude; Batteau, Pierre; +1 AuthorsDaviet, Sylvie; Schleyer-Lindenmann, Alexandra; Raynal, Jean-Claude; Batteau, Pierre; Noack, Yves;La trajectoire prise par le Bassin Minier de Provence, situé entre Aix en Provence et Marseille, s’explique par sa longue histoire minière, brutalement interrompue par la fermeture des mines en 2003. Nous approchons cet espace avec une perspective globale, englobant les dimensions sociales, économiques et environnementales de ce socio-écosystème. En conclusion, nous proposons des scénarios d’évolution du territoire et des perspectives de recherche, en soulignant le rôle croissant de la transition énergétique, particulièrement dans le contexte de la reconversion de la centrale thermique au charbon. The trajectory taken by the Provence Coalfield (or Bassin Minier de Provence), located between Aix-en-Provence and Marseille, is explained by its long mining history, disrupted by the closure of the mine in 2003. We approach this space from a global perspective, considering the social, economic and environmental dimensions of the socio-ecosystem. The conclusion puts forward scenarios for the evolution of the territory and the perspectives for research, underlining the growing role of the energy transition, especially in the context of the closure of the coal-fired power plant.
add 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 Routesgold 0 citations 0 popularity Average influence Average impulse Average Powered by BIP!more_vert add 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 Preprint , Conference object , Article 2023 FrancePublisher:Sissa Medialab Authors: Casolino, Marco; Parizot, Etienne;Casolino, Marco; Parizot, Etienne;Ultra High Energy Cosmic Rays (UHECRs) offer a unique chance to study the universe at energies inaccessible by man-made accelerators. Observations by ground based observatories have clarified several characteristics of these particles, but their origin, nature, and acceleration mechanisms are still unclear, mostly due to their extremely low flux. Space-based observatories have the potential for an increase in statistics, up to several orders of magnitude, and would be able to cover the whole sky, allowing for a direct comparison of spectra and direction of arrival, but the detector design poses several formidable technical challenges. The JEM-EUSO program has been addressing this problem, trying to open the road of space-based UHECR observations. Several missions have already been completed (on the ground: EUSO-TA; with stratospheric ballons: EUSO-Balloon, EUSO-SPB1 and EUSO-SPB2; in space: TUS\cite{Klimov2017}, MINI-EUSO). Others are under study (K-EUSO) or proposed for the next decade (POEMMA)\cite{Olinto_2021}. In this work we report on the status of the JEM-EUSO program and the technology developed so far.
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For further information contact us at helpdesk@openaire.euAccess RoutesGreen 1 citations 1 popularity Average influence Average impulse Average Powered by BIP!more_vert add 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 Conference object , Preprint , Article 2023 FrancePublisher:Sissa Medialab Battisti, Matteo; Bertaina, Mario; Arnone, Enrico; Sammartino, Gaetano; Pretto, Giulia;The Mini-EUSO telescope is the first space-based detector of the JEM-EUSO program. It was launched for the International Space Station on August 22$^{nd}$, 2019 to observe from the ISS orbit ($\sim$420 km altitude) various phenomena occurring in the Earth's atmosphere through a UV-transparent window located in the Russian Zvezda Module. The dimension of the window defines and constrains the dimension of the optics, based on a set of two Fresnel lenses of 25 cm diameter each, almost two orders of magnitude smaller than the system foreseen for a larger space-based detector, like the original JEM-EUSO detector or the future POEMMA. As a consequence, the energy threshold of Mini-EUSO is very high, above $10^{21} $eV. Nevertheless, a series of events that resemble the shape and the time duration of EAS-induced events have been detected in Mini-EUSO data. This contribution presents the most interesting cases, showing that the vast majority of the EAS-like events can be traced back to ground sources repeatedly flashing and triggered many times by Mini-EUSO. Some non-repeated EAS-like events are also present. In these cases, it is possible to exclude their cosmic origin through the comparison with simulated events. Since it is clear that those events can not be originated by a UHECR, we decided to rename them "Short Light Transients" or SLTs. Finally, it was possible to associate some of the SLTs with atmospheric activity. This analysis confirms the validity of the JEM-EUSO detection principle and shows that it is possible for a space-based detector to distinguish between events induced by UHECRs and events with a different origin. arXiv admin note: text overlap with arXiv:2309.10630
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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 add 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 Conference object 2023 FrancePublisher:Sissa Medialab Funded by:EC | ChETEC-INFRA, ANR | UnivEarthS, ANR | Université de ParisEC| ChETEC-INFRA ,ANR| UnivEarthS ,ANR| Université de ParisCerisy, L; Pedrajas, A.L.; Lastoria, C; Perrin-Terrin, M; Brunner, J; Dabhi, V;doi: 10.22323/1.444.1191
International audience; One of the main goals of KM3NeT/ORCA is to measure atmospheric neutrino oscillation parameters with competitive precision. To achieve this goal, good discrimination between track-like and shower-like events is necessary, with particular focus on the measurement of the tau neutrino normalisation. The track-like signal is mainly carried by muon neutrinos from charged current interactions, while the shower-like signal comes from charged current interactions of electron and tau neutrinos, and neutral current interactions of all flavours. A Random Grid Search algorithm is optimised to separate these channels and its performance is compared with machine learning methods using boosted decision trees. This contribution will report on the technical aspects of the algorithm and the performance of the particle identification with data recorded in 2020 and 2021 using an early six-lines configuration of the ORCA detector (ORCA6).
HAL AMU; Mémoires en... arrow_drop_down HAL AMU; Mémoires en Sciences de l'Information et de la CommunicationConference object . 2023License: CC BY NC NDFull-Text: https://hal.science/hal-04186231/documentadd 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.eu0 citations 0 popularity Average influence Average impulse Average Powered by BIP!more_vert HAL AMU; Mémoires en... arrow_drop_down HAL AMU; Mémoires en Sciences de l'Information et de la CommunicationConference object . 2023License: CC BY NC NDFull-Text: https://hal.science/hal-04186231/documentadd 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 Conference object , Article , Preprint 2023 FrancePublisher:Sissa Medialab Funded by:IRC, UKRI | Improved Loss Modelling o..., UKRI | RootDetect: Remote Detect...IRC ,UKRI| Improved Loss Modelling of SMC Components ,UKRI| RootDetect: Remote Detection and Precision Management of Root HealthFederica Bradascio; Felix Aharonian; Faical Ait-Benkhali; Jann Aschersleben; Michael Backes; Victor Barbosa Martins; Rowan William Batzofin; Yvonne Becherini; David Berge; Konrad Bernloehr; Markus Boettcher; Catherine Boisson; Julien Bolmont; Mathieu Bony (de); Benedetta Bruno; Tomasz Bulik; Christopher Burger-Scheidlin; Sabrina Casanova; Rahul Cecil; Jelena Celic; Matteo Cerruti; Tej Bahadur Chand; Sunil Chandra; Andrew Chen; James Okwe Chibueze; Ogochukwu Chibueze; Garret Cotter; Jean Damascene Mbarubucyeye; Isak Delberth Davids; Anton Dmytriiev; Victor Doroshenko; Kathrin Egberts; Jean-Pierre ERNENWEIN; Steven Fegan; Gerard Fontaine; Matthias Fuessling; Stefan Funk; Stefano Gabici; Shahede Ghafourizadeh; Gianluca Giavitto; Dorit Glawion; Jean-Francois Glicenstein; Guillaume Grolleron; Tim Holch; Markus Holler; Marek Jamrozy; Felix Jankowsky; Vikas Joshi; Eli Kasai; Krzysztof Katarzynski; Rukaiya Khatoon; Bruno Khelifi; Nukri Komin; Karl Kosack; Dmitriy Kostunin; Rodrigo Guedes Lang; Sebastien Le Stum; Franziska Leitl; Anne Lemiere; Jean-Philippe Lenain; Fabian Leuschner; Jonathan Mackey; Denys Malyshev; Vincent Marandon; Peter David Marinos; Ramin Marx; Abhay Mehta; Alison Mitchell; Rafal Moderski; Lars Mohrmann; Alessandro Montanari; Thomas Murach; Mathieu Naurois (de); Jacek Niemiec; Paul O'Brien; Stefan Ohm; Laura Olivera-Nieto; Emma Ona-Wilhelmi (de); Michal Ostrowski; Sebastian Panny; Michael Panter; Giada Peron; Dmitry Prokhorov; Gerd PUEHLHOFER; Andreas Quirrenbach; Maxime Regeard; Olaf Reimer; Matthieu Renaud; Frank Rieger; Bronislaw Rudak; Vardan Sahakian; Heiko Salzmann; Manami Sasaki; Fabian Schuessler; Jimmy N.S. Shapopi; Andreas Specovius; Samuel Spencer; Simon Steinmassl; Constantin Steppa; Katrin Streil; Tadayuki Takahashi; Takaaki Tanaka; Charles Thorpe-Morgan; Christopher van Eldik; Manuela Vecchi; Johannes Veh; Tina Wach; Richard White; Davit Zargaryan; Andrzej Zdziarski; Andreas Zech; Natalia Żywucka; Rasha Abbasi; Markus Ackermann; Jenni Adams; Sanjib Agarwalla; Juanan Aguilar; Markus Ahlers; Jean-Marco Alameddine; Najia Moureen Binte Amin; Karen Andeen; Gisela Anton; Carlos Argüelles; Yosuke Ashida; Sofia Athanasiadou; Spencer Axani; Xinhua Bai; Aswathi Balagopal V; Moreno Baricevic; Steve Barwick; Vedant Basu; Ryan Bay; James Beatty; Julia Becker Tjus; Jakob Beise; Chiara Bellenghi; Charlotte Benning; Segev BenZvi; David Berley; Elisa Bernardini; Dave Besson; Erik Blaufuss; Summer Blot; Federico Bontempo; Julia Book; Caterina Boscolo Meneguolo; Sebastian BOSER; Olga Botner; Jakob Bottcher; Etienne Bourbeau; Jim Braun; Bennett Brinson; Jannes Brostean-Kaiser; Ryan T. Burley; Raffaela Busse; Delaney Butterfield; Michael Campana; Kiara Carloni; Erin Carnie-Bronca; Sharmistha Chattopadhyay; Thien Nhan Chau; Chujie Chen; Zheyang Chen; Dmitry Chirkin; Seowon Choi; Brian Clark; Lew Classen; Alan Coleman; Gabriel Collin; Amy Connolly; Janet Conrad; Paul Coppin; Pablo Correa; Doug Cowen; Pranav Dave; Catherine DE CLERCQ; James DeLaunay; Diyaselis Delgado Lopez; Shuyang Deng; Kunal Deoskar; Abhishek Desai; Paolo Desiati; Krijn de Vries; Gwenhaël de Wasseige; Tyce DeYoung; Alejandro Diaz; Juan Carlos Diaz-Velez; Markus Dittmer; Alba Domi; Hrvoje Dujmovic; Michael DuVernois; Thomas Ehrhardt; Philipp Eller; Enrico Ellinger; Sharif El Mentawi; Dominik Elsässer; Ralph Engel; Hannah Erpenbeck; John Evans; Paul Evenson; Paras Koundal; Carsten Rott; Lisa Johanna Schumacher; Fabian Schüssler;The evidence for multi-messenger photon and neutrino emission from the blazar TXS 0506+056 has demonstrated the importance of realtime follow-up of neutrino events by various ground- and space-based facilities. The effort of H.E.S.S. and other experiments in coordinating observations to obtain quasi-simultaneous multiwavelength flux and spectrum measurements has been critical in measuring the chance coincidence with the high-energy neutrino event IC-170922A and constraining theoretical models. For about a decade, the H.E.S.S. transient program has included a search for gamma-ray emission associated with high-energy neutrino alerts, looking for gamma-ray activity from known sources and newly detected emitters consistent with the neutrino location. In this contribution, we present an overview of follow-up activities for realtime neutrino alerts with H.E.S.S. in 2021 and 2022. Our analysis includes both public IceCube neutrino alerts and alerts exchanged as part of a joint H.E.S.S.-IceCube program. We focus on interesting coincidences observed with gamma-ray sources, particularly highlighting the significant detection of PKS 0625-35, an AGN previously detected by H.E.S.S., and three IceCube neutrinos. Presented at the 38th International Cosmic Ray Conference (ICRC2023). See arXiv:2307.13047 for all IceCube contributions
arXiv.org e-Print Ar... arrow_drop_down Mémoires en Sciences de l'Information et de la Communication; HAL-CEAConference object . 2023https://doi.org/10.48550/arxiv...Article . 2023License: 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 0 citations 0 popularity Average influence Average impulse Average Powered by BIP!more_vert arXiv.org e-Print Ar... arrow_drop_down Mémoires en Sciences de l'Information et de la Communication; HAL-CEAConference object . 2023https://doi.org/10.48550/arxiv...Article . 2023License: 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 Conference object , Other literature type 2023 FrancePublisher:MDPI AG Funded by:EC | ENUBETEC| ENUBETFrancesco Terranova; F. Acerbi; I. Angelis; L. Bomben; M. Bonesini; F. Bramati; A. Branca; C. Brizzolari; G. Brunetti; S. Capelli; S. Carturan; M. G. Catanesi; S. Cecchini; F. Cindolo; G. Cogo; G. Collazuol; F. Dal Corso; C. Delogu; G. De Rosa; A. Falcone; A. Gola; L. Halić; F. Iacob; C. Jollet; A. Kallitsopoulou; B. Klicek; Y. Kudenko; Ch. Lampoudis; M. Laveder; P. Legou; A. Longhin; L. Ludovici; E. Lutsenko; L. Magaletti; G. Mandrioli; A. Margotti; V. Mascagna; S. Marangoni; N. Mauri; L. Meazza; A. Meregaglia; M. Mezzetto; A. Paoloni; T. Papaevangelou; M. Pari; E. G. Parozzi; L. Pasqualini; G. Paternoster; L. Patrizii; M. Pozzato; M. Prest; F. Pupilli; E. Radicioni; A. C. Ruggeri; D. Sampsonidis; C. Scian; G. Sirri; M. Stipcevic; M. Tenti; M. Torti; S. E. Tzamarias; E. Vallazza; L. Votano;International audience; Monitored neutrino beams are facilities where beam diagnostics enable the counting and identification of charged leptons in the decay tunnel of a narrow band beam. These facilities can monitor neutrino production at the single particle level (flux precision %) and provide information about the neutrino energy at the 10% level. The ENUBET Collaboration has demonstrated that lepton monitoring might be achieved not only by employing kaon decays but also by identifying muons from the decays and positrons from the decay-in-flight of muons before the hadron dump. As a consequence, beam monitoring can be performed using the ENUBET technique even when the kaon production yield is kinematically suppressed. This finding opens up a wealth of opportunities for measuring neutrino cross-sections below 1 GeV. In this paper, we investigate this opportunity at the European Spallation Source (ESS), which is an ideal facility to measure and cross-sections in the 0.2–1 GeV range. We also describe the planned activities for the design of this beam at the ESS within the framework of the ESSSB+ design study, which was approved by the EU in July 2022.
CERN Document Server arrow_drop_down https://doi.org/10.3390/psf202...Conference object . 2023 . Peer-reviewedLicense: CC BYData sources: CrossrefMémoires en Sciences de l'Information et de la Communication; HAL-CEAConference object . 2022add 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 Routeshybrid 0 citations 0 popularity Average influence Average impulse Average Powered by BIP!more_vert CERN Document Server arrow_drop_down https://doi.org/10.3390/psf202...Conference object . 2023 . Peer-reviewedLicense: CC BYData sources: CrossrefMémoires en Sciences de l'Information et de la Communication; HAL-CEAConference object . 2022add 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 Conference object 2023 FrancePublisher:Sissa Medialab Funded by:ANR | MMUniverseANR| MMUniverseDolgikh, Konstantin Alexandrovich; Korochkin, A; Rubtsov, G; Semikoz, D; Tkachev, I;doi: 10.22323/1.444.0452
International audience; UHECR propagation in a turbulent intergalactic magnetic field in the small-angle scattering regime is well understood for propagation distances much larger than the field coherence scale. The diffusion theory doesn't work and unexpected effects may appear for propagation over smaller distances, from a few and up to 10-20 coherence scales. We study the propagation of UHECRs in this regime, which may be relevant for intermediate mass UHECR nuclei and nG scale intergalactic magnetic fields with 1 Mpc coherence scale. We found that the trajectories form a non-trivial caustic-like pattern with strong deviation from isotropy. In this regime we've found different observable cases of distortions of the source energy spectrum and the images of a source. Thus, measurements of the flux, direction and energy spectrum from a source at a given distance will depend on the position of the observer. In the future, these facts may explain Telescope Array observations.
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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.eu0 citations 0 popularity Average influence Average impulse Average Powered by BIP!more_vert add 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=10.22323/1.444.0452&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Conference object 2023Publisher:Sissa Medialab Funded by:EC | ChETEC-INFRA, ANR | UnivEarthS, ANR | Université de ParisEC| ChETEC-INFRA ,ANR| UnivEarthS ,ANR| Université de ParisAuthors: Bailly-Salins, Louis;Bailly-Salins, Louis;doi: 10.22323/1.444.0203
International audience; The KM3NeT collaboration operates two water Cherenkov neutrino telescopes in the Mediterranean sea, ORCA and ARCA. The flux of atmospheric muons produced in cosmic ray air showers forms a background to the main objectives of KM3NeT/ORCA and KM3NeT/ARCA, respectively measuring atmospheric neutrino oscillations and detecting neutrinos from astrophysical sources. A small portion of the atmospheric muons stops inside the detector’s instrumented volume. The stopping muons are 5% of the muons reconstructed using the 6 first strings deployed for ORCA. This still amounts to 1000 events per hour. We present two methods for selecting them, applied on both simulations and data. The first method uses simple cuts on a set of reconstructed variables. The second method uses a machine learning model to classify muons as “stopping” or “crossing”. Both methods allow to reach a high selection purity, close to 95%. Detecting stopping muons can serve many purposes like studying muon decay via the detection of Michel electrons or estimating the flux of atmospheric muons at sea level. This work highlights the accurate reconstruction capabilities of ORCA. The median error on the reconstructed stopping point of selected muons is less than 5 meters, and the median angular deviation is 1° . This is to be compared with the 20 meters horizontal distance between strings and the 9 meters vertical distance between optical modules. Another important result is the excellent agreement between distribution of stopping muons selected in data and in simulations.}
Mémoires en Sciences... arrow_drop_down Mémoires en Sciences de l'Information et de la CommunicationConference object . 2023add 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.eu0 citations 0 popularity Average influence Average impulse Average Powered by BIP!more_vert Mémoires en Sciences... arrow_drop_down Mémoires en Sciences de l'Information et de la CommunicationConference object . 2023add 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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description Publicationkeyboard_double_arrow_right Article , Conference object 2023Publisher:Oxford University Press (OUP) Meryame Jabbade; Abdellatif Nachab; Elmokhtar Elouardi; Abdel-Mjid Nourreddine; Ezzoura Errami; Mohammed Benjelloun; Mohammed Fahad;doi: 10.1093/rpd/ncad172
pmid: 37934986
Abstract A study of the influence of moisture content on the radon exhalation rate from phosphate samples (with and without consideration of the back diffusion effect) was performed using the sealed cup technique. The mass exhalation rate was found to increase with an increase in moisture content, reaching a maximum value of 2.414 ± 0.034 Bq kg−1 h−1 with a moisture content of 10%. However, the mass exhalation rate decreased with a continued increase in moisture content above 25%. The mass exhalation rate was also measured at different temperatures between −10 and 50°C. The obtained results show that the mass exhalation rate increases linearly with temperature. We point out that all the obtained values of radon exhalation rate are lower than the world average radon exhalation rate (57.6 Bq m−2 h−1).
Radiation Protection... arrow_drop_down Radiation Protection DosimetryArticle . 2023 . Peer-reviewedLicense: OUP Standard Publication ReuseData sources: CrossrefMémoires en Sciences de l'Information et de la CommunicationConference object . 2022add 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 Routesbronze 0 citations 0 popularity Average influence Average impulse Average Powered by BIP!more_vert Radiation Protection... arrow_drop_down Radiation Protection DosimetryArticle . 2023 . Peer-reviewedLicense: OUP Standard Publication ReuseData sources: CrossrefMémoires en Sciences de l'Information et de la CommunicationConference object . 2022add 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 Conference object 2023 France EnglishPublisher:HAL CCSD Authors: Melleton, Jérémie; Pizzocolo, Francesco; Bertrand, Guillaume;Melleton, Jérémie; Pizzocolo, Francesco; Bertrand, Guillaume;International audience; The underground holds indispensable resources for European society, but they need a careful management relying on shared knowledge. To address transnational and continental-scale subsurface problems, geoscientific data need to be harmonized beyond national borders.Started in September 2022 for a duration of five years and based on these principles, GSEU has the following objectives:-To develop pan-European harmonised data and related information services with a focus on critical raw materials, geothermal energy resources and subsurface storage capacities for sustainable energy carriers and CO2 sequestration, groundwater dynamics and quality, geological and climate change information for coastal vulnerability assessment and geological baseline information;-To establish the European Centre of Excellence on Sustainable Resource Management to promote the deployment of the United Nations Framework Classification for Resources (UNFC) and the United Nations Resource Management System (UNRMS);-To develop the geological data infrastructure - building on the existing EGDI - to provide permanent access to and dissemination of the data and information services developed under the project;-To provide a common European Geological Knowledge Base Platform as the single open access portal to the project results and to the underlying data and information collections and infrastructures of partners at national and regional level;-To further strengthen the network of national and regional geological survey organisations to provide geological knowledge and services in a sustainable manner.
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For further information contact us at helpdesk@openaire.eu0 citations 0 popularity Average influence Average impulse Average Powered by BIP!more_vert 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=od______3379::c6bb98df75483087e3c32dfeed9d53f6&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Conference object , Article 2023 FrancePublisher:Cellule MathDoc/CEDRAM Authors: Daviet, Sylvie; Schleyer-Lindenmann, Alexandra; Raynal, Jean-Claude; Batteau, Pierre; +1 AuthorsDaviet, Sylvie; Schleyer-Lindenmann, Alexandra; Raynal, Jean-Claude; Batteau, Pierre; Noack, Yves;La trajectoire prise par le Bassin Minier de Provence, situé entre Aix en Provence et Marseille, s’explique par sa longue histoire minière, brutalement interrompue par la fermeture des mines en 2003. Nous approchons cet espace avec une perspective globale, englobant les dimensions sociales, économiques et environnementales de ce socio-écosystème. En conclusion, nous proposons des scénarios d’évolution du territoire et des perspectives de recherche, en soulignant le rôle croissant de la transition énergétique, particulièrement dans le contexte de la reconversion de la centrale thermique au charbon. The trajectory taken by the Provence Coalfield (or Bassin Minier de Provence), located between Aix-en-Provence and Marseille, is explained by its long mining history, disrupted by the closure of the mine in 2003. We approach this space from a global perspective, considering the social, economic and environmental dimensions of the socio-ecosystem. The conclusion puts forward scenarios for the evolution of the territory and the perspectives for research, underlining the growing role of the energy transition, especially in the context of the closure of the coal-fired power plant.
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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 Routesgold 0 citations 0 popularity Average influence Average impulse Average Powered by BIP!more_vert add 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 , Conference object , Article 2023 FrancePublisher:Sissa Medialab Authors: Casolino, Marco; Parizot, Etienne;Casolino, Marco; Parizot, Etienne;Ultra High Energy Cosmic Rays (UHECRs) offer a unique chance to study the universe at energies inaccessible by man-made accelerators. Observations by ground based observatories have clarified several characteristics of these particles, but their origin, nature, and acceleration mechanisms are still unclear, mostly due to their extremely low flux. Space-based observatories have the potential for an increase in statistics, up to several orders of magnitude, and would be able to cover the whole sky, allowing for a direct comparison of spectra and direction of arrival, but the detector design poses several formidable technical challenges. The JEM-EUSO program has been addressing this problem, trying to open the road of space-based UHECR observations. Several missions have already been completed (on the ground: EUSO-TA; with stratospheric ballons: EUSO-Balloon, EUSO-SPB1 and EUSO-SPB2; in space: TUS\cite{Klimov2017}, MINI-EUSO). Others are under study (K-EUSO) or proposed for the next decade (POEMMA)\cite{Olinto_2021}. In this work we report on the status of the JEM-EUSO program and the technology developed so far.
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For further information contact us at helpdesk@openaire.euAccess RoutesGreen 1 citations 1 popularity Average influence Average impulse Average Powered by BIP!more_vert add 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 Conference object , Preprint , Article 2023 FrancePublisher:Sissa Medialab Battisti, Matteo; Bertaina, Mario; Arnone, Enrico; Sammartino, Gaetano; Pretto, Giulia;The Mini-EUSO telescope is the first space-based detector of the JEM-EUSO program. It was launched for the International Space Station on August 22$^{nd}$, 2019 to observe from the ISS orbit ($\sim$420 km altitude) various phenomena occurring in the Earth's atmosphere through a UV-transparent window located in the Russian Zvezda Module. The dimension of the window defines and constrains the dimension of the optics, based on a set of two Fresnel lenses of 25 cm diameter each, almost two orders of magnitude smaller than the system foreseen for a larger space-based detector, like the original JEM-EUSO detector or the future POEMMA. As a consequence, the energy threshold of Mini-EUSO is very high, above $10^{21} $eV. Nevertheless, a series of events that resemble the shape and the time duration of EAS-induced events have been detected in Mini-EUSO data. This contribution presents the most interesting cases, showing that the vast majority of the EAS-like events can be traced back to ground sources repeatedly flashing and triggered many times by Mini-EUSO. Some non-repeated EAS-like events are also present. In these cases, it is possible to exclude their cosmic origin through the comparison with simulated events. Since it is clear that those events can not be originated by a UHECR, we decided to rename them "Short Light Transients" or SLTs. Finally, it was possible to associate some of the SLTs with atmospheric activity. This analysis confirms the validity of the JEM-EUSO detection principle and shows that it is possible for a space-based detector to distinguish between events induced by UHECRs and events with a different origin. arXiv admin note: text overlap with arXiv:2309.10630
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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 add 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 Conference object 2023 FrancePublisher:Sissa Medialab Funded by:EC | ChETEC-INFRA, ANR | UnivEarthS, ANR | Université de ParisEC| ChETEC-INFRA ,ANR| UnivEarthS ,ANR| Université de ParisCerisy, L; Pedrajas, A.L.; Lastoria, C; Perrin-Terrin, M; Brunner, J; Dabhi, V;doi: 10.22323/1.444.1191
International audience; One of the main goals of KM3NeT/ORCA is to measure atmospheric neutrino oscillation parameters with competitive precision. To achieve this goal, good discrimination between track-like and shower-like events is necessary, with particular focus on the measurement of the tau neutrino normalisation. The track-like signal is mainly carried by muon neutrinos from charged current interactions, while the shower-like signal comes from charged current interactions of electron and tau neutrinos, and neutral current interactions of all flavours. A Random Grid Search algorithm is optimised to separate these channels and its performance is compared with machine learning methods using boosted decision trees. This contribution will report on the technical aspects of the algorithm and the performance of the particle identification with data recorded in 2020 and 2021 using an early six-lines configuration of the ORCA detector (ORCA6).
HAL AMU; Mémoires en... arrow_drop_down HAL AMU; Mémoires en Sciences de l'Information et de la CommunicationConference object . 2023License: CC BY NC NDFull-Text: https://hal.science/hal-04186231/documentadd 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.eu0 citations 0 popularity Average influence Average impulse Average Powered by BIP!more_vert HAL AMU; Mémoires en... arrow_drop_down HAL AMU; Mémoires en Sciences de l'Information et de la CommunicationConference object . 2023License: CC BY NC NDFull-Text: https://hal.science/hal-04186231/documentadd 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 Conference object , Article , Preprint 2023 FrancePublisher:Sissa Medialab Funded by:IRC, UKRI | Improved Loss Modelling o..., UKRI | RootDetect: Remote Detect...IRC ,UKRI| Improved Loss Modelling of SMC Components ,UKRI| RootDetect: Remote Detection and Precision Management of Root HealthFederica Bradascio; Felix Aharonian; Faical Ait-Benkhali; Jann Aschersleben; Michael Backes; Victor Barbosa Martins; Rowan William Batzofin; Yvonne Becherini; David Berge; Konrad Bernloehr; Markus Boettcher; Catherine Boisson; Julien Bolmont; Mathieu Bony (de); Benedetta Bruno; Tomasz Bulik; Christopher Burger-Scheidlin; Sabrina Casanova; Rahul Cecil; Jelena Celic; Matteo Cerruti; Tej Bahadur Chand; Sunil Chandra; Andrew Chen; James Okwe Chibueze; Ogochukwu Chibueze; Garret Cotter; Jean Damascene Mbarubucyeye; Isak Delberth Davids; Anton Dmytriiev; Victor Doroshenko; Kathrin Egberts; Jean-Pierre ERNENWEIN; Steven Fegan; Gerard Fontaine; Matthias Fuessling; Stefan Funk; Stefano Gabici; Shahede Ghafourizadeh; Gianluca Giavitto; Dorit Glawion; Jean-Francois Glicenstein; Guillaume Grolleron; Tim Holch; Markus Holler; Marek Jamrozy; Felix Jankowsky; Vikas Joshi; Eli Kasai; Krzysztof Katarzynski; Rukaiya Khatoon; Bruno Khelifi; Nukri Komin; Karl Kosack; Dmitriy Kostunin; Rodrigo Guedes Lang; Sebastien Le Stum; Franziska Leitl; Anne Lemiere; Jean-Philippe Lenain; Fabian Leuschner; Jonathan Mackey; Denys Malyshev; Vincent Marandon; Peter David Marinos; Ramin Marx; Abhay Mehta; Alison Mitchell; Rafal Moderski; Lars Mohrmann; Alessandro Montanari; Thomas Murach; Mathieu Naurois (de); Jacek Niemiec; Paul O'Brien; Stefan Ohm; Laura Olivera-Nieto; Emma Ona-Wilhelmi (de); Michal Ostrowski; Sebastian Panny; Michael Panter; Giada Peron; Dmitry Prokhorov; Gerd PUEHLHOFER; Andreas Quirrenbach; Maxime Regeard; Olaf Reimer; Matthieu Renaud; Frank Rieger; Bronislaw Rudak; Vardan Sahakian; Heiko Salzmann; Manami Sasaki; Fabian Schuessler; Jimmy N.S. Shapopi; Andreas Specovius; Samuel Spencer; Simon Steinmassl; Constantin Steppa; Katrin Streil; Tadayuki Takahashi; Takaaki Tanaka; Charles Thorpe-Morgan; Christopher van Eldik; Manuela Vecchi; Johannes Veh; Tina Wach; Richard White; Davit Zargaryan; Andrzej Zdziarski; Andreas Zech; Natalia Żywucka; Rasha Abbasi; Markus Ackermann; Jenni Adams; Sanjib Agarwalla; Juanan Aguilar; Markus Ahlers; Jean-Marco Alameddine; Najia Moureen Binte Amin; Karen Andeen; Gisela Anton; Carlos Argüelles; Yosuke Ashida; Sofia Athanasiadou; Spencer Axani; Xinhua Bai; Aswathi Balagopal V; Moreno Baricevic; Steve Barwick; Vedant Basu; Ryan Bay; James Beatty; Julia Becker Tjus; Jakob Beise; Chiara Bellenghi; Charlotte Benning; Segev BenZvi; David Berley; Elisa Bernardini; Dave Besson; Erik Blaufuss; Summer Blot; Federico Bontempo; Julia Book; Caterina Boscolo Meneguolo; Sebastian BOSER; Olga Botner; Jakob Bottcher; Etienne Bourbeau; Jim Braun; Bennett Brinson; Jannes Brostean-Kaiser; Ryan T. Burley; Raffaela Busse; Delaney Butterfield; Michael Campana; Kiara Carloni; Erin Carnie-Bronca; Sharmistha Chattopadhyay; Thien Nhan Chau; Chujie Chen; Zheyang Chen; Dmitry Chirkin; Seowon Choi; Brian Clark; Lew Classen; Alan Coleman; Gabriel Collin; Amy Connolly; Janet Conrad; Paul Coppin; Pablo Correa; Doug Cowen; Pranav Dave; Catherine DE CLERCQ; James DeLaunay; Diyaselis Delgado Lopez; Shuyang Deng; Kunal Deoskar; Abhishek Desai; Paolo Desiati; Krijn de Vries; Gwenhaël de Wasseige; Tyce DeYoung; Alejandro Diaz; Juan Carlos Diaz-Velez; Markus Dittmer; Alba Domi; Hrvoje Dujmovic; Michael DuVernois; Thomas Ehrhardt; Philipp Eller; Enrico Ellinger; Sharif El Mentawi; Dominik Elsässer; Ralph Engel; Hannah Erpenbeck; John Evans; Paul Evenson; Paras Koundal; Carsten Rott; Lisa Johanna Schumacher; Fabian Schüssler;The evidence for multi-messenger photon and neutrino emission from the blazar TXS 0506+056 has demonstrated the importance of realtime follow-up of neutrino events by various ground- and space-based facilities. The effort of H.E.S.S. and other experiments in coordinating observations to obtain quasi-simultaneous multiwavelength flux and spectrum measurements has been critical in measuring the chance coincidence with the high-energy neutrino event IC-170922A and constraining theoretical models. For about a decade, the H.E.S.S. transient program has included a search for gamma-ray emission associated with high-energy neutrino alerts, looking for gamma-ray activity from known sources and newly detected emitters consistent with the neutrino location. In this contribution, we present an overview of follow-up activities for realtime neutrino alerts with H.E.S.S. in 2021 and 2022. Our analysis includes both public IceCube neutrino alerts and alerts exchanged as part of a joint H.E.S.S.-IceCube program. We focus on interesting coincidences observed with gamma-ray sources, particularly highlighting the significant detection of PKS 0625-35, an AGN previously detected by H.E.S.S., and three IceCube neutrinos. Presented at the 38th International Cosmic Ray Conference (ICRC2023). See arXiv:2307.13047 for all IceCube contributions
arXiv.org e-Print Ar... arrow_drop_down Mémoires en Sciences de l'Information et de la Communication; HAL-CEAConference object . 2023https://doi.org/10.48550/arxiv...Article . 2023License: 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 0 citations 0 popularity Average influence Average impulse Average Powered by BIP!more_vert arXiv.org e-Print Ar... arrow_drop_down Mémoires en Sciences de l'Information et de la Communication; HAL-CEAConference object . 2023https://doi.org/10.48550/arxiv...Article . 2023License: 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 Conference object , Other literature type 2023 FrancePublisher:MDPI AG Funded by:EC | ENUBETEC| ENUBETFrancesco Terranova; F. Acerbi; I. Angelis; L. Bomben; M. Bonesini; F. Bramati; A. Branca; C. Brizzolari; G. Brunetti; S. Capelli; S. Carturan; M. G. Catanesi; S. Cecchini; F. Cindolo; G. Cogo; G. Collazuol; F. Dal Corso; C. Delogu; G. De Rosa; A. Falcone; A. Gola; L. Halić; F. Iacob; C. Jollet; A. Kallitsopoulou; B. Klicek; Y. Kudenko; Ch. Lampoudis; M. Laveder; P. Legou; A. Longhin; L. Ludovici; E. Lutsenko; L. Magaletti; G. Mandrioli; A. Margotti; V. Mascagna; S. Marangoni; N. Mauri; L. Meazza; A. Meregaglia; M. Mezzetto; A. Paoloni; T. Papaevangelou; M. Pari; E. G. Parozzi; L. Pasqualini; G. Paternoster; L. Patrizii; M. Pozzato; M. Prest; F. Pupilli; E. Radicioni; A. C. Ruggeri; D. Sampsonidis; C. Scian; G. Sirri; M. Stipcevic; M. Tenti; M. Torti; S. E. Tzamarias; E. Vallazza; L. Votano;International audience; Monitored neutrino beams are facilities where beam diagnostics enable the counting and identification of charged leptons in the decay tunnel of a narrow band beam. These facilities can monitor neutrino production at the single particle level (flux precision %) and provide information about the neutrino energy at the 10% level. The ENUBET Collaboration has demonstrated that lepton monitoring might be achieved not only by employing kaon decays but also by identifying muons from the decays and positrons from the decay-in-flight of muons before the hadron dump. As a consequence, beam monitoring can be performed using the ENUBET technique even when the kaon production yield is kinematically suppressed. This finding opens up a wealth of opportunities for measuring neutrino cross-sections below 1 GeV. In this paper, we investigate this opportunity at the European Spallation Source (ESS), which is an ideal facility to measure and cross-sections in the 0.2–1 GeV range. We also describe the planned activities for the design of this beam at the ESS within the framework of the ESSSB+ design study, which was approved by the EU in July 2022.
CERN Document Server arrow_drop_down https://doi.org/10.3390/psf202...Conference object . 2023 . Peer-reviewedLicense: CC BYData sources: CrossrefMémoires en Sciences de l'Information et de la Communication; HAL-CEAConference object . 2022add 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 Routeshybrid 0 citations 0 popularity Average influence Average impulse Average Powered by BIP!more_vert CERN Document Server arrow_drop_down https://doi.org/10.3390/psf202...Conference object . 2023 . Peer-reviewedLicense: CC BYData sources: CrossrefMémoires en Sciences de l'Information et de la Communication; HAL-CEAConference object . 2022add 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 Conference object 2023 FrancePublisher:Sissa Medialab Funded by:ANR | MMUniverseANR| MMUniverseDolgikh, Konstantin Alexandrovich; Korochkin, A; Rubtsov, G; Semikoz, D; Tkachev, I;doi: 10.22323/1.444.0452
International audience; UHECR propagation in a turbulent intergalactic magnetic field in the small-angle scattering regime is well understood for propagation distances much larger than the field coherence scale. The diffusion theory doesn't work and unexpected effects may appear for propagation over smaller distances, from a few and up to 10-20 coherence scales. We study the propagation of UHECRs in this regime, which may be relevant for intermediate mass UHECR nuclei and nG scale intergalactic magnetic fields with 1 Mpc coherence scale. We found that the trajectories form a non-trivial caustic-like pattern with strong deviation from isotropy. In this regime we've found different observable cases of distortions of the source energy spectrum and the images of a source. Thus, measurements of the flux, direction and energy spectrum from a source at a given distance will depend on the position of the observer. In the future, these facts may explain Telescope Array observations.
add 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.eu0 citations 0 popularity Average influence Average impulse Average Powered by BIP!more_vert add 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 Conference object 2023Publisher:Sissa Medialab Funded by:EC | ChETEC-INFRA, ANR | UnivEarthS, ANR | Université de ParisEC| ChETEC-INFRA ,ANR| UnivEarthS ,ANR| Université de ParisAuthors: Bailly-Salins, Louis;Bailly-Salins, Louis;doi: 10.22323/1.444.0203
International audience; The KM3NeT collaboration operates two water Cherenkov neutrino telescopes in the Mediterranean sea, ORCA and ARCA. The flux of atmospheric muons produced in cosmic ray air showers forms a background to the main objectives of KM3NeT/ORCA and KM3NeT/ARCA, respectively measuring atmospheric neutrino oscillations and detecting neutrinos from astrophysical sources. A small portion of the atmospheric muons stops inside the detector’s instrumented volume. The stopping muons are 5% of the muons reconstructed using the 6 first strings deployed for ORCA. This still amounts to 1000 events per hour. We present two methods for selecting them, applied on both simulations and data. The first method uses simple cuts on a set of reconstructed variables. The second method uses a machine learning model to classify muons as “stopping” or “crossing”. Both methods allow to reach a high selection purity, close to 95%. Detecting stopping muons can serve many purposes like studying muon decay via the detection of Michel electrons or estimating the flux of atmospheric muons at sea level. This work highlights the accurate reconstruction capabilities of ORCA. The median error on the reconstructed stopping point of selected muons is less than 5 meters, and the median angular deviation is 1° . This is to be compared with the 20 meters horizontal distance between strings and the 9 meters vertical distance between optical modules. Another important result is the excellent agreement between distribution of stopping muons selected in data and in simulations.}
Mémoires en Sciences... arrow_drop_down Mémoires en Sciences de l'Information et de la CommunicationConference object . 2023add 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=10.22323/1.444.0203&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eu0 citations 0 popularity Average influence Average impulse Average Powered by BIP!more_vert Mémoires en Sciences... arrow_drop_down Mémoires en Sciences de l'Information et de la CommunicationConference object . 2023add 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=10.22323/1.444.0203&type=result"></script>'); --> </script>
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