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The Cosmic-Ray Extremely Distributed Observatory (CREDO) is a project dedicated to global studies of extremely extended cosmic-ray phenomena, the cosmic-ray ensembles (CRE), beyond the capabilities of existing detectors and observatories.…

Cloud computing offers an opportunity to run compute-resource intensive climate models at scale by parallelising model runs such that datasets useful to the exoplanet community can be produced efficiently. To better understand the…

A New QCD facility at the M2 beam line of the CERN SPS COMPASS++/AMBER

High Energy Physics - Experiment · Physics 2019-01-28 B. Adams , C. A. Aidala , R. Akhunzyanov , G. D. Alexeev , M. G. Alexeev , A. Amoroso , V. Andrieux , N. V. Anfimov , V. Anosov , A. Antoshkin , K. Augsten , W. Augustyniak , C. D. R. Azevedo , A. Azhibekov , B. Badelek , F. Balestra , M. Ball , J. Barth , R. Beck , Y. Bedfer , J. Berenguer Antequera , J. C. Bernauer , J. Bernhard , M. Bodlak , P. Bordalo , F. Bradamante , A. Bressan , M. Buchele , V. E. Burtsev , W. -C. Chang , C. Chatterjee , X. Chen , M. Chiosso , A. G. Chumakov , S. -U. Chung , A. Cicuttin , P. Correia , M. L. Crespo , S. Dalla Torre , S. S. Dasgupta , S. Dasgupta , N. Dashyan , I. Denisenko , O. Yu. Denisov , L. Dhara , N. d'Hose , F. Donato , S. V. Donskov , N. Doshita , Ch. Dreisbach , W. Dunnweber , R. R. Dusaev , M. Dziewiecki , A. Dzyuba , A. Efremov , P. Egelhof , A. Elagin , P. D. Eversheim , M. Faessler , J. Fedotova , A. Ferrero , M. Finger , M. Finger , H. Fischer , C. Franco , J. M. Friedrich , V. Frolov , A. Futch , F. Gautheron , O. P. Gavrichtchouk , S. Gerassimov , S. Gevorkyan , Y. Ghandilyan , J. Giarra , I. Gnesi , M. Gorzellik , A. Grasso , A. Gridin , M. Grosse Perdekamp , B. Grube , R. I. Gushterski , A. Guskov , D. Hahne , G. Hamar , D. von Harrach , X. He , R. Heitz , F. Herrmann , N. Horikawa , C. -Y. Hsieh , S. Huber , A. Inglessi , A. Ilyichev , T. Isataev , S. Ishimoto , A. Ivanov , N. Ivanov , Yu. Ivanshin , T. Iwata , M. Jandek , V. Jary , C. -M. Jen , R. Joosten , P. Joerg , K. Juraskova , E. Kabuss , A. Kabyshev , F. Kaspar , A. Kerbizi , B. Ketzer , G. V. Khaustov , Yu. A. Khokhlov , M. Kim , O. Kiselev , Yu. Kisselev , F. Klein , J. H. Koivuniemi , V. N. Kolosov , K. Kondo , I. Konorov , V. F. Konstantinov , A. M. Kotzinian , O. M. Kouznetsov , A. Koval , Z. Kral , M. Kraemer , F. Krinner , Y. Kulinich , F. Kunne , K. Kurek , R. P. Kurjata , K. Kuterbekov , I. I. Kuznetsov , A. Kveton , E. A. Levchenko , S. Levorato , Y. -S. Lian , Y. Liang , J. Lichtenstadt , P. -J. Lin , K. Liu , M. X. Liu , R. Longo , W. Lorenzon , M. Losekamm , V. E. Lyubovitskij , E. Maev , A. Maggiora , A. Magnon , V. Makarenko , N. Makins , N. Makke , G. K. Mallot , A. Maltsev , S. A. Mamon , B. Marianski , A. Martin , H. Marukyan , J. Marzec , N. Masi , J. Matousek , H. Matsuda , G. Mattson , G. V. Meshcheryakov , W. Meyer , M. Meyer , Yu. V. Mikhailov , M. Mikhasenko , M. Minot , E. Mitrofanov , N. Mitrofanov , Y. Miyachi , A. Moretti , A. Nagaytsev , C. Naim , D. Neyret , G. Nigmatkulov , A. Mkrtchyan , H. Mkrtchyan , J. Novy , W. -D. Nowak , F. Nozzoli , G. Nukazuka , A. S. Nunes , A. G. Olshevsky , I. Orlov , J. D. Osborn , M. Ostrick , D. Panzieri , B. Parsamyan , S. Paul , J. -C. Peng , F. Pereira , D. V. Peshekhonov , M. Pesek , M. Peskova , N. Pierre , S. Platchkov , J. Pochodzalla , V. A. Polyakov , T. Poeschl , J. Pretz , M. Quaresma , C. Quintans , S. Ramos , R. Raymond , G. Reicherz , C. Riedl , D. I. Ryabchikov , A. Rybnikov , A. Rychter , R. Salac , V. D. Samoylenko , A. Sandacz , S. Sarkar , M. Sarsour , I. A. Savin , G. Sbrizzai , H. Schmieden , E. Seder , A. Selyunin , H. Simon , L. Sinha , S. Sirtl , M. Slunecka , J. Smolik , A. Srnka , D. Steffen , M. Stolarski , O. Subrt , M. Sulc , H. Suzuki , A. Szabelski , P. Sznajder , M. Tasevsky , V. Tchekhovski , S. Tessaro , F. Tessarotto , A. Thiel , J. Tomsa , F. Tosello , V. Tskhay , S. Uhl , B. I. Vasilishin , A. Vassiliev , A. Vauth , B. M. Veit , B. Ventura , J. Veloso , A. Vidon , M. Virius , A. Vorobyev , M. Wagner , S. Wallner , M. Wilfert , Z. Xiao , N. Xu , J. Yang , K. Zaremba , P. Zavada , M. Zavertyaev , E. Zemlyanichkina , H. Zhao , Y. Zhao , N. Zhuravlev , M. Ziembicki , P. Zuccon

The analysis of clouds in the earth's atmosphere is important for a variety of applications, viz. weather reporting, climate forecasting, and solar energy generation. In this paper, we focus our attention on the impact of cloud on the total…

Atmospheric and Oceanic Physics · Physics 2017-03-17 Soumyabrata Dev , Shilpa Manandhar , Feng Yuan , Yee Hui Lee , Stefan Winkler

Cosmic rays are a fundamental source of ionization for molecular and diffuse clouds, influencing their chemical, thermal, and dynamical evolution. The amount of cosmic rays inside a cloud also determines the $\gamma$-ray flux produced by…

High Energy Astrophysical Phenomena · Physics 2015-06-17 G. Morlino , S. Gabici

The availability of new Cloud Platform offered by Google motivated us to propose nine Proof of Concepts (PoC) aiming to demonstrated and test the capabilities of the platform in the context of scientifically-driven tasks and requirements.…

Instrumentation and Methods for Astrophysics · Physics 2019-03-11 M. Landoni , G. Taffoni , A. Bignamini , R. Smareglia

Multi-cloud concept has broaden the world of cloud computing and has become a buzzword today. The word Multi-cloud envisions utilization of services from multiple heterogeneous cloud providers via a single architecture at customer premises.…

Distributed, Parallel, and Cluster Computing · Computer Science 2021-08-31 Deepika Saxena , Rishabh Gupta , Ashutosh Kumar Singh

The crucial part of electromagnetic phenomena in many atmospheric processes is verified by systematized data. The multilayered charged system of clouds represents some dynamically equilibrium structure kept by the ionic and polarization…

Plasma Physics · Physics 2024-02-16 S. N. Artekha , A. V. Belyan

We present a brief summary of various aspects of the electron-cloud effect (ECE) in accelerators. For further details, the reader is encouraged to refer to the proceedings of many prior workshops, either dedicated to EC or with significant…

Accelerator Physics · Physics 2013-10-08 M. A. Furman

Astroparticle physics and cosmology allow us to scan the universe through multiple messengers. It is the combination of these probes that improves our understanding of the universe, both in its composition and its dynamics. Unlike other…

Instrumentation and Methods for Astrophysics · Physics 2015-06-19 K. Louedec

We will here discuss how the gamma-ray emission from molecular clouds can be used to probe the cosmic ray flux in distant regions of the Galaxy and to constrain the highly unknown cosmic ray diffusion coefficient. In particular we will…

Cosmic rays produce molecular cluster ions as they pass through the lower atmosphere. Neutral molecular clusters such as dimers and complexes are expected to make a small contribution to the radiative balance, but atmospheric absorption by…

Atmospheric and Oceanic Physics · Physics 2013-03-08 K. L. Aplin , M. Lockwood

Remote sensing of atmosphere is conventionally done via a study of extinction / scattering of light from natural (Sun, Moon) or artificial (laser) sources. Cherenkov emission from extensive air showers generated by cosmic rays provides one…

Instrumentation and Methods for Astrophysics · Physics 2015-06-19 A. Neronov , D. Malyshev , A. Dmytriiev

Recent observations of galaxy clusters in radio and X-ray indicate that cosmic rays and magnetic fields may be energetically important in the intracluster medium. According to the estimates based on theses observational studies, the…

Astrophysics · Physics 2015-06-24 Dongsu Ryu , Hyesung Kang

This report examines the open questions that remain unsolved following the measurements with antineutrons ($\bar n$) as probes conducted up to the 1990s at the LEAR facility at CERN. It also presents suggestions for possible new experiments…

Nuclear Experiment · Physics 2026-01-19 A. Filippi

Clusters of galaxies, the largest collapsed structures in the Universe, are located at the intersection of extended filaments of baryons and dark matter. Cosmological accretion onto clusters through large scale filaments adds material at…

New particle acceleration schemes open up exciting opportunities, potentially providing more compact or higher-energy accelerators. The AWAKE experiment at CERN is currently taking data to establish the method of proton-driven plasma…

Accelerator Physics · Physics 2019-09-04 M. Wing

In this revue are presented several present activities and experiments at Alomar observatory and BEO Moussala and the possibility to investigate the influence of cosmic ray on climate parameters and the impact of cosmic ray to climate…

Space Physics · Physics 2007-05-23 Alexander Mishev

Cloud computing has permeated into the information technology industry in the last few years, and it is emerging nowadays in scientific environments. Science user communities are demanding a broad range of computing power to satisfy the…

Distributed, Parallel, and Cluster Computing · Computer Science 2017-09-26 Álvaro López García , Enol Fernández-del-Castillo , Pablo Orviz Fernández , Isabel Campos Plasencia , Jesús Marco de Lucas

Atmospheric neutrinos produced by cosmic-ray interactions around the globe provide a beam for the study of neutrino properties. They are also a background in searches for neutrinos of astrophysical origin. Both aspects are addressed in this…

High Energy Astrophysical Phenomena · Physics 2019-10-22 Thomas K. Gaisser
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