Zobrazeno 1 - 10
of 709
pro vyhledávání: '"PAMELA detector"'
Autor:
Todor Stanev
Publikováno v:
High Energy Cosmic Rays ISBN: 9783030715663
High Energy Cosmic Rays ISBN: 9783540851479
High Energy Cosmic Rays ISBN: 9783540851479
As we discussed in the previous chapter, primary cosmic rays interact with the atmosphere and produce fluxes of secondary, tertiary, etc. particles. All these particles together create a cascade, called an air shower. In principle, measurements of ai
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::914866d3b2fd8f1f7dee1272a532a267
https://doi.org/10.1007/978-3-030-71567-0_6
https://doi.org/10.1007/978-3-030-71567-0_6
Autor:
Todor Stanev
Publikováno v:
High Energy Cosmic Rays ISBN: 9783030715663
High Energy Cosmic Rays ISBN: 9783540851479
High Energy Cosmic Rays ISBN: 9783540851479
Once accelerated at supernova shocks, cosmic rays have to propagate through the interstellar medium before we detect them. The interstellar medium contains matter, magnetic fields and radiation fields, all of which are targets for cosmic ray interact
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f4f2cc811b875e6b0781072ebfdb8f8e
https://doi.org/10.1007/978-3-030-71567-0_4
https://doi.org/10.1007/978-3-030-71567-0_4
Autor:
A. M. Galper, P. Spillantini
Publikováno v:
Physics of Particles and Nuclei. 48:710-719
The satellite borne Pamela instrument is dedicated to the precise and high statistics study of cosmic-ray fluxes over a four decades energy range. Pamela experiment is the last step of the ‘Russian-Italian Mission’ (RIM) program established in 19
Autor:
A. Bruno
Publikováno v:
Space Weather. 15:1191-1202
The EPEAD and HEPAD instruments on the GOES spacecraft have served over many years as monitors of the solar particles intensities, surveying the Sun and measuring in situ its effect on the near-Earth solar-terrestrial environment. However, the recons
Autor:
R. I. Budaev, Yu V. Bogomolov, S. A. Rodenko, A. F. Mosichkin, A. M. Shitova, K. M. Belotsky, A. M. Galper, A. G. Mayorov, V. V. Alekseev, A. A. Okrugin, V. V. Malakhov, M. A. Mayorova, Alexander Kuznetsov, A. D. Lukyanov, A. A. Kirillov, O. A. Dunaeva
Publikováno v:
Physics of Particles and Nuclei. 48:687-690
The paper provides a review of the results of precision measurements of the fluxes of different charged components of galactic cosmic rays (positrons and antiprotons, protons and helium nuclei) in modern experiments with magnetic spectrometers PAMELA
Autor:
Pim Schellart, Stijn Buitink, Katie Mulrey, Anna Nelles, Satyendra Thoudam, Tobias Winchen, Heino Falcke, Arthur Corstanje, T. N. G. Trinh, Jörg P. Rachen, S. ter Veen, Jörg R. Hörandel, Laura Rossetto, Olaf Scholten, Antonio Bonardi, Pragati Mitra
Publikováno v:
EPJ Web of Conferences, 136, 1-6
EPJ Web of Conferences, Vol 136, p 02001 (2017)
6th Roma International Conference on Astroparticle Physics: RICAP16, 136
EPJ Web of Conferences, 136, pp. 1-6
EPJ Web of Conferences, Vol 136, p 02001 (2017)
6th Roma International Conference on Astroparticle Physics: RICAP16, 136
EPJ Web of Conferences, 136, pp. 1-6
High-energy cosmic rays, impinging on the atmosphere of the Earth initiate cascades of secondary particles, the extensive air showers. The electrons and positrons in the air shower emit electromagnetic radiation. This emission is detected with the LO
Publikováno v:
Kinematics and Physics of Celestial Bodies. 33:1-12
The process of heliospheric modulation of intensity of galactic cosmic rays is investigated by solving the transport equation. The spatial-energetic distribution of cosmic rays in the present epoch and in the past is analyzed. It is demonstrated that
Autor:
A. G. Mayorov, S. A. Rodenko
Publikováno v:
Bulletin of the Lebedev Physics Institute. 43:323-327
The PAMELA experiment on the study of cosmic rays in a wide energy range was performed onboard the Resurs-DK1 spacecraft from June 2006 to February 2016. The data on antiproton fluxes in the near-Earth space play an important role for this field of p
Autor:
Hisanori Takamaru, Harufumi Tsuchiya, Chihiro Kato, Ernesto Ortiz, M. Anzorena, J. F. Valdés-Galicia, Masayoshi Kozai, Kyoko Watanabe, D. Lopez, Y. Nagai, O. Musalem, T. K. Sako, Yutaka Matsubara, Rocío García, Hiroshi Kojima, Luis Xavier Gonzalez, Y. Sasai, Tatsumi Koi, Yoshitaka Itow, Kazuoki Munakata, Shoichi Shibata, A. Hurtado
Publikováno v:
Advances in Space Research. 58:2018-2025
In this work we report the flux of protons and neutral emission measured at the top of the Sierra Negra volcano at 4600 m.a.s.l. (575 g/cm 2 ), in Eastern Mexico. As an example of the capability of the mini-SciCR as a cosmic ray detector we present t
Publikováno v:
Astronomy Letters. 43:703-705
Three particles with energies of 36, 35, and 58 EeV arrived from one sky region were recorded by two EAS arrays during a day. The events are assumed to have been produced by the beam of particles that resulted from the interaction of cosmic rays with