Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Catholic University of America, 620 Michigan Ave., NE, Washington, DC 20064, USA; Rostov State University, Rostov State University, Rostov-on-Don, 344090 Russian Federation
Catholic University of America, Department of Physics 620 Michigan Ave, NE, Washington, DC 20064, USA; Rostov State University, 5 Zorge St., Rostov-on-Don, CA 344090 Russian Federation
Max-Planck-Institut für Aeronomie, Katlenburg-Lindau, Germany
AN SSSR, Institut Kosmicheskikh Issledovanii, Moscow, USSR
Rostovskii Gosudarstvennyi Universitet, Rostov-on-Don, USSR
Institute for Physics, Southern Federal University of Russia, Rostov-on-Don, Russian Federation
Rostov State University Rostov-on Don, Russia
Department of Astrophysics, Rostov State University, Rostov-on-Don, Russia
Rostov State University, Space Physics Department 5 Zorge St., Rostov-on-Don, 344090 Russian Federation
Research Institute of Physics, Rostov State University, Rostov-on-Don, 344090 Russian Federation Physics Department, Rostov State University, Rostov-on-Don, 344000, Russia
Rostov State University, Department of Astrophysics ul. Zorge 5, Rostov-on-Don, 344104 Russian Federation
Rostov State University Rostov-on-Don 344104, Russia
Rostov State University
AN SSSR, Vychislitel'nyi Tsentr, Moscow, USSR
Rostov State University Space Physics Department, Zorge St. 20, Apt. 64, Rostov-on-Don, 344090 Russian Federation
A proxy for determining solar wind dynamic pressure at Mars using Mars Global Surveyor data
Characteristics of Mini-Magnetospheres Formed by Paleo-Magnetic Fields of Mars
Characteristics of Near-Polar Atmosphere/Thermosphere of Mars at Altitudes of 125 145 km: The Data of a Radio Occultation Experiment onboard the Mars Global Surveyor Spacecraft
Comparative study of numerical simulations of the solar wind interaction with Venus
Conditions in the Martian ionosphere/atmosphere from a comparison of a thermospheric model with radio occultation data
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