Zobrazeno 1 - 10
of 56
pro vyhledávání: '"Vladimir Slemzin"'
Autor:
Yulia Shugay, Vladimir Kalegaev, Ksenia Kaportseva, Vladimir Slemzin, Denis Rodkin, Valeriy Eremeev
Publikováno v:
Universe, Vol 8, Iss 11, p 565 (2022)
Solar wind (SW) disturbances associated with coronal mass ejections (CMEs) cause significant geomagnetic storms, which may lead to the malfunction or damage of sensitive on-ground and space-based critical infrastructure. CMEs are formed in the solar
Externí odkaz:
https://doaj.org/article/ac4ec86b0ac64a68881059defc89a793
Autor:
Luc Damé, Mustapha Meftah, Alain Hauchecorne, Philippe Keckhut, Alain Sarkissian, Marion Marchand, Abdenour Irbah, Éric Quémerais, Slimane Bekki, Thomas Foujols, Matthieu Kretzschmar, Gaël Cessateur, Alexander Shapiro, Werner Schmutz, Sergey Kuzin, Vladimir Slemzin, Alexander Urnov, Sergey Bogachev, José Merayo, Peter Brauer, Kanaris Tsinganos, Antonis Paschalis, Ayman Mahrous, Safinaz Khaled, Ahmed Ghitas, Besheir Marzouk, Amal Zaki, Ahmed A. Hady, Rangaiah Kariyappa
Publikováno v:
Journal of Advanced Research, Vol 4, Iss 3, Pp 235-251 (2013)
We present the ambitions of the SWUSV (Space Weather and Ultraviolet Solar Variability) Microsatellite Mission that encompasses three major scientific objectives: (1) Space Weather including the prediction and detection of major eruptions and coronal
Externí odkaz:
https://doaj.org/article/48da8f43380e4facb46aa583409817b5
The state of the space environment plays a significant role for forecasting of geomagnetic storms produced by disturbances of the solar wind (SW). Coronal mass ejections (CMEs) passing through the heliosphere often have a prolonged (up to several day
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::475d82c1348c90302e0d9745be19d316
http://arxiv.org/abs/2203.06976
http://arxiv.org/abs/2203.06976
Publikováno v:
Bulletin of the Lebedev Physics Institute. 47:92-96
The geoeffectiveness of single and complex transient structures of the solar wind (SW), formed by coronal mass ejections (CMEs) and associated Forbush decreases (FDs) in the cosmic ray flux is considered. By the example of the period of 2010–2011,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c8cb69f5fbdefb157a4c0924fa0d18db
https://doi.org/10.3103/s1068335620030069
https://doi.org/10.3103/s1068335620030069
Publikováno v:
Plasma Physics Reports. 45:889-920
A review of studies of coronal mass ejections (CMEs) and the propagation of the resulting interplanetary coronal mass ejections (ICMEs) in the heliosphere is presented. The main parameters of ICMEs, their differences from other types of solar wind (S
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::44947dadae097d24e0f864777f125437
https://doi.org/10.1134/s1063780x19100076
https://doi.org/10.1134/s1063780x19100076
Autor:
D. G. Rodkin, Igor Veselovsky, K. B. Kaportseva, Vladimir Slemzin, A. T. Lukashenko, Yu. S. Shugay
Publikováno v:
Cosmic Research. 57:18-28
The paper considers the classification of solar wind streams in magnetohydrodynamic parameters (MHD-types); combinations of proton speed, density, temperature, and magnetic field strength, in addition to the classical solar wind separation into high-
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c4058e93c29353e97f3c446c21e96d50
https://doi.org/10.1134/s0010952519010088
https://doi.org/10.1134/s0010952519010088
Publikováno v:
Cosmic Research. 55:20-29
We have considered the possible causes of discrepancies between the predicted and observed at 1 AU parameters of the recurrent solar wind (SW) streams in the maximum of the 24th solar cycle. These discrepancies have been observed in both the SW veloc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7c3d3e59733516409becd5eb08daacad
https://doi.org/10.1134/s0010952517010087
https://doi.org/10.1134/s0010952517010087
Autor:
A. A. Kochanov, Farid Goryaev, A. M. Uralov, Vladimir Slemzin, I. I. Myshyakov, Denis Rodkin, Victor V. Grechnev, V. I. Kiselev
Publikováno v:
Solar Physics. 294
We study the development of a coronal mass ejection (CME) caused by a prominence eruption on 24 February 2011 and properties of a related interplanetary CME (ICME). The prominence destabilized, accelerated, and produced an M3.5 flare, a fast CME, and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::eb05dd26f0f41dc8b8068f84d0fe1860
https://doi.org/10.1007/s11207-019-1529-0
https://doi.org/10.1007/s11207-019-1529-0
Publikováno v:
The Astrophysical Journal. 905:L17
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a9f51f009ee7b4c3238a21a7cdc335ee
https://doi.org/10.3847/2041-8213/abcc76
https://doi.org/10.3847/2041-8213/abcc76
Publikováno v:
Bulletin of the Lebedev Physics Institute. 43:287-290
The interaction of the interplanetary coronal mass ejection (ICME) and the high-speed solar wind flux (HSSWF) associated with the coronal hole (CH) is considered. By the examples of two events at the maximum of solar cycle 24 from June 4 to June 16 a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1ba08901b29c7d172db6e0b378044ca9
https://doi.org/10.3103/s1068335616090062
https://doi.org/10.3103/s1068335616090062