Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Scientist
Institute for Problems in Mechanics of the Russian Academy of Sciences, Prospect Vernadskogo 101, 117526 Moscow, Russia
Institute for Problems in Mechanics of the Russian Academy of Sciences, Prospect Vernadskogo 101-1, 119526 Moscow, Russia
AN SSSR, Institut Kosmicheskikh Issledovanii, Moscow, USSR
Akademiia Nauk SSSR, Institut Kosmicheskikh Issledovanii, Moscow, USSR
Institute for Problems in Mechanics of the Russian Academy of Sciences, Prospect Vernadskogo 101-1, 117526 Moscow, Russia
Institute for Problems in Mechanics, Russian Academy of Sciences, Pr. Vernadskogo 101-1, Moscow 119526, Russia
Institute for Problems in Mechanics of the Russian Academy of Sciences, Prospect Vernadskogo, 101 117526 Moscow, Russia
RAN, Inst. Problem Mekhaniki, Moscow, Russia
Institute for Problems in Mechanics of the Russian Academy of Sciences, Prospect Vernadskogo, 101, 117526 Moscow, Russia
Institute for Problems in Mechanics, Russian Academy of Sciences
AN SSSR, Institut Problem Mekhaniki, Moscow, USSR
Institute for Problems in Mechanics of the Russian Academy of Sciences, Pr. Vernadskogo 101-1, 119526 Moscow, Russia
Russian Academy of Sciences, Moscow, Russia
Institute for Problems in Mechanics, Russian Academy of Sciences, Prospect Vernadskogo 101-1, 119526 Moscow, Russia
Institute for Problems in Mechanics, Russian Academy of Sciences, Prospect Vernadskogo 101-1, Moscow 119526, Russia
Institut für Astrophysik und Extraterrestrische Forschung der Universität Bonn
Institute for Problems in Mechanics, Russian Academy of Sciences, Prospect Vernadskogo 101-1, 11952
A hydrodynamic description of particle accelerating shocks.
A three-fluid model of the solar wind termination shock including a continuous production of anomalous cosmic rays.
A two-fluid model of the solar wind termination shock modified by shock-generated cosmic rays including energy losses
Acceleration of Pick-up Ions at the Solar Wind Termination Shock
Acceleration of pickup interstellar protons by shock waves in corotating solar wind regions
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