Boron and Carbon Isotopes in the PAMELA Experiment

Autor: W. Menn, G. I. Vasilyev, E. A. Bogomolov

Publikováno v: Bulletin of the Russian Academy of Sciences: Physics. 85:341-344

An attempt is made to determine the 11B/10B ratio in the ~0.1 to 1.0 GeV/nucleon region of energies using the 2006–2014 PAMELA data on the rigidity and velocity of detected nuclei and estimate for the first time the 14C/12C ratio at energies of ~0.

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::33af36b8d190cac3241d97c637c2742c
https://doi.org/10.3103/s1062873821040080

Boron Isotopes in the PAMELA Experiment

Autor: G. I. Vasilyev, E. A. Bogomolov, W. Menn, S. A. Voronov

Publikováno v: Physics of Atomic Nuclei. 82:704-709

Analysis of the isotope composition of nuclei in galactic cosmic rays (GCR) in the PAMELA orbital international experiment allows studying the problems of cosmic-ray origin and propagation in our Galaxy. PAMELA magnetic spectrometer data provided the

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::e64d7080b5ae66fb97088bb3d5d8cde2
https://doi.org/10.1134/s1063778819660086

2H and 3He Isotopes in Solar Flares, According to the PAMELA Data for 2006–2014

Autor: E. A. Bogomolov, G. I. Vasilyev, W. Menn

Publikováno v: Bulletin of the Russian Academy of Sciences: Physics. 83:523-526

Results are presented for the first time from the PAMELA orbital experiment of 2006–2014. Observations record 2H isotopes with energies above ~50 MeV/nucleon and 3He isotopes with energies above ~90 MeV/nucleon in solar flares. Time-of-flight analy

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::a8711e39c648ed26b4ff2b18511f0884
https://doi.org/10.3103/s1062873819050113

Time dependence of the flux of helium nuclei in cosmic rays measured by the pamela experiment between 2006 july and 2009 december

Autor: A. N. Kvashnin, M. Simon, Mark Pearce, S. B. Ricciarini, Per Carlson, N. Marcelli, P. Papini, E. Vannuccini, O. Adriani, W. Menn, M. D. Ngobeni, F. Cafagna, Sergey Koldobskiy, G. C. Barbarino, V. Bonvicini, Y. I. Stozhkov, N. Zampa, G. A. Bazilevskaya, Andrea Vacchi, P. Spillantini, V. V. Mikhailov, E. Mocchiutti, V. V. Malakhov, M. Bongi, Alfonso Monaco, Alessandro Sotgiu, R. Sparvoli, G. Osteria, A. Bruno, M. Merge, O. P. M. Aslam, Matteo Martucci, S. A. Voronov, Roberto Bellotti, S. V. Koldashov, E. A. Bogomolov, A. M. Galper, Marco Ricci, A. Lenni, D. Campana, G. I. Vasilyev, Marco Casolino, C. De Santis, Alexey Leonov, Y. T. Yurkin, Driaan Bisschoff, Riccardo Munini, Nicola Mori, L. Marcelli, A. G. Mayorov, G. Castellini, M. S. Potgieter, G. Zampa, Beatrice Panico, P. Picozza, Mirko Boezio

Publikováno v: The Astrophysical journal 893 (2020). doi:10.3847/1538-4357/ab80c2
info:cnr-pdr/source/autori:Marcelli N.; Boezio M.; Lenni A.; Menn W.; Munini R.; Aslam O.P.M.; Bisschoff D.; Ngobeni M.D.; Potgieter M.S.; Adriani O.; Barbarino G.C.; Bazilevskaya G.A.; Bellotti R.; Bogomolov E.A.; Bongi M.; Bonvicini V.; Bruno A.; Cafagna F.; Campana D.; Carlson P.; Casolino M.; Castellini G.; De Santis C.; Galper A.M.; Koldashov S.V.; Koldobskiy S.; Kvashnin A.N.; Leonov A.A.; Malakhov V.V.; Marcelli L.; Martucci M.; Mayorov A.G.; Merg M.; Mocchiutti E.; Monaco A.; Mori N.; Mikhailov V.V.; Osteria G.; Panico B.; Papini P.; Pearce M.; Picozza P.; Ricci M.; Ricciarini S.B.; Simon M.; Sotgiu A.; Sparvoli R.; Spillantini P.; Stozhkov Y.I.; Vacchi A.; Vannuccini E.; Vasilyev G.I.; Voronov S.A.; Yurkin Y.T.; Zampa G.; Zampa N./titolo:Time dependence of the flux of helium nuclei in cosmic rays measured by the pamela experiment between 2006 july and 2009 december/doi:10.3847%2F1538-4357%2Fab80c2/rivista:The Astrophysical journal/anno:2020/pagina_da:/pagina_a:/intervallo_pagine:/volume:893

Precise time-dependent measurements of the Z = 2 component in the cosmic radiation provide crucial information about the propagation of charged particles through the heliosphere. The PAMELA experiment, with its long flight duration (2006 June 15-2016

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fa5b7fa577c0937c81137a887b53551e
http://hdl.handle.net/11368/2970845

Influence of the temperature of the photosphere and deeper layers of the Sun on the spectra of gamma quanta with energies above 511 keV during solar flares

Autor: G I Vasilyev

Publikováno v: Journal of Physics: Conference Series. 2103:012010

Gamma-ray quanta, which occur during solar flares due to the interaction of accelerated protons with the photosphere and deeper layers of the sun, enter interplanetary space from a thickness of several tens of g/cm2. In the presented work, gamma quan

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::5a5af9b4814028f56505d83d0f89bb80
https://doi.org/10.1088/1742-6596/2103/1/012010