Astronomy and Astrophysics – Astronomy
Scientist
Astronomy and Astrophysics
Astronomy
Scientist
Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation, IZMIRAN;, Research Institute for Astronomy and Astrophysics of Maragah
Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation, Russian Academy of Sciences, 142092, Troitsk Moscow Region, Russia
AN SSSR, Institut Zemnogo Magnetizma, Ionosfery i Rasprostraneniia Radiovoln, Akademgorodok, USSR
Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation, IZMIRAN
IZMIRAN, Akademgorodok, USSR
Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation, Russian Academy of Sciences, Troitsk Moscow Region, 142190 Russia
IZMIRAN, Troitsk, Russia
Akademiia Nauk SSSR, Institut Zemnogo Magnetizma, Ionosfery i Rasprostraneniia Radiovoln, Troitsk, USSR
IZMIRAN, Troitsk, USSR
IZMIRAN, Akademgorodok, Russia
AN SSSR, IZMIRAN, Akademgorodok, USSR
Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation, Russian Academy of Sciences;, Research Institute for Astronomy and Astrophysics of Maragha
Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation, Russian Academy of Sciences
CNRS, Inst. d'Astrophysique, Paris, France; IZMIRAN, Akademgorodok, Russia
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
IZMIRAN;, Research Institute for Astronomy and Astrophysics of Maragha
A critical height of quiescent prominences before eruption
CME stimulated by eruptive prominence
Condensation of combustion products in the exhaust plumes of rocket engines in the upper atmosphere
Coronal Mass Ejections and Eruptive Prominences: Mutual Spatial Arrangement
Coronal mass ejections caused by filament eruptions.
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