Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Scientist
Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation, Troitsk / Moscow, Russia
Akademiia Nauk SSSR, Fizicheskii Institut, Moscow, USSR
AN SSSR, Institut Zemnogo Magnetizma, Ionosfery i Rasprostraneniia Radiovoln, Akademgorodok, USSR
Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation, Russian Academy of Sciences
IZMIRAN
Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radiowave Propagation, Russian Academy of Sciences
AN SSSR, Institut Zemnogo Magnetizma, Ionosfery i Rasprostraneniia Radiovoln, Troitsk, USSR
Akademiia Nauk SSSR, Institut Zemnogo Magnetizma, Ionosfery i Rasprostraneniia Radiovoln, Troitsk, USSR
IZMIRAN, Troitsk town, Moscow region, Russian Federation
Russian Academy of Sciences, IZMIRAN, Moscow 142190, Russia Federation
Russian Academy of Sciences, IZMIRAN, 142190 Moscow, Russia
IZMIRAN, Russian Academy of Sciences, Troitsk, Russia
IZMIRAN, Troitsk, Russia
Pushkov Institute of Terrestrial Magnetism, the Ionosphere and Radio Wave Propagation, Russian Academy of Sciences
Akademiia Nauk SSSR, Institut Zemnogo Magnetizma, Ionosfery i Rasprostraneniia Radiovoln, Akademgorodok, USSR
Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation, Russian Academy of Sciences
Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation, Russian Academy of Sciences, 142190, Moscow Region, Troitsk, IZMIRAN, Russia
Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation, Rusian Academy of Sciences.
A solar spectroscopic absolute abundance of argon from RESIK
A Year Later: Solar, Heliospheric, and Magnetospheric Disturbances in November 2004
Allowance for the geometry of solar wind interaction with the Earth's magnetic field in geoeffective parameters and in the prediction of geomagnetic activity
Aurora triggering by high-power radio emission from the SURA facility as observed on board the International Space Station.
Basic results of the CORONAS-F solar observations
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