Zobrazeno 1 - 10
of 71
pro vyhledávání: '"Yuri Yermolaev"'
Autor:
Liudmila Rakhmanova, Alexander Khokhlachev, Maria Riazantseva, Yuri Yermolaev, Georgy Zastenker
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 11 (2024)
Turbulent solar wind is known to be a main driver of the processes inside the magnetosphere, including geomagnetic storms and substorms. Experimental studies of the last decade demonstrate additional ways of interplanetary plasma transport to the mag
Externí odkaz:
https://doaj.org/article/8340f4149bde42129bf1b8182cde1098
Autor:
Liudmila Rakhmanova, Alexander Khokhlachev, Maria Riazantseva, Yuri Yermolaev, Georgy Zastenker
Publikováno v:
Universe, Vol 10, Iss 5, p 194 (2024)
Solar wind is known to have different properties depending on its origin at the Sun. In addition to the differences in plasma and magnetic field parameters, these streams differ due to the properties of turbulent fluctuations involved in the flow. Th
Externí odkaz:
https://doaj.org/article/d91817a2d9174ac7a2550c4f3eb74936
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 10 (2023)
Varying solar wind plays a crucial role in the processes inside the magnetosphere. Statistical studies generally reveal the geoeffectiveness of solar wind streams of different origins and types, characterized by various parameters such as dynamic pre
Externí odkaz:
https://doaj.org/article/930b9f3d782f4d10af87e9889bf70f68
Publikováno v:
Solar-Terrestrial Physics, Vol 7, Iss 4, Pp 10-17 (2021)
Studying the direction of the solar wind flow is a topical problem of space weather forecasting. As a rule, the quiet and uniform solar wind propagates radially, but significant changes in the solar wind flow direction can be observed, for example, i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::143f6919b6e2485f1db0eef34dfe354d
https://naukaru.ru/en/nauka/article/46428/view
https://naukaru.ru/en/nauka/article/46428/view
Autor:
Irina Lodkina, Georgy Zastenker, Yuri Yermolaev, Tatiana Podladchikova, Viktor Yu. Popov, L. S. Chesalin, Vladislav Izmodenov, Aleksandr A. Vinogradov, E. V. Maiewski, Liudmila Rakhmanova, Olga Katushkina, Maria Riazantseva, Anatoli Petrukovich, Helmi Malova
Publikováno v:
Physics-Uspekhi. 63:801-811
Solar wind — a plasma stream flowing out of the solar corona — is interesting both as a carrier of solar activity and as an example of a collisionless plasma. We present the main results of Russian studies in recent years. The original MHD model
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6d3d56d8b1e5563b1416e053f1f6ed8c
https://doi.org/10.3367/ufne.2019.06.038677
https://doi.org/10.3367/ufne.2019.06.038677
The interplanetary manifestations of coronal mass ejections (ICME) typically characterized by an increased relative abundance of doubly ionized helium, which can be several time higher comparative to the slow solar wind streams and exceed 10%. At the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::cbd7a19f7e2d22047bdfa31dfa98bbcd
https://doi.org/10.5194/egusphere-egu22-11326
https://doi.org/10.5194/egusphere-egu22-11326
In our study we analyzing fluctuations of the solar wind ion flux associated with the Earth bow shock using data obtained by the BMSW experiment, installed onboard the SPEKTR-R satellite. The high time resolution of the spectrometer (0.031 s for the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0084c1ff4bd782d507a0fc342317d1f8
https://doi.org/10.5194/egusphere-egu22-5222
https://doi.org/10.5194/egusphere-egu22-5222
Publikováno v:
Universe, Vol 7, Iss 138, p 138 (2021)
Universe
Volume 7
Issue 5
Universe
Volume 7
Issue 5
One of the most promising methods of research in solar–terrestrial physics is the comparison of the responses of the magnetosphere–ionosphere–atmosphere system to various types of interplanetary disturbances (so-called “interplanetary drivers
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::eb39bdb267d93aad490c951b76670a96
https://www.mdpi.com/2218-1997/7/5/138
https://www.mdpi.com/2218-1997/7/5/138
The structure of quasiperpendicular interplanetary (IP) shock fronts was studied based on the data from the BMSW plasma spectrometer, installed onboard the SPEKTR-R spacecraft, supplemented by magnetic field measurements on the WIND. Special attentio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ec3d7e468e0749e43575755e4ab6875b
https://doi.org/10.5194/egusphere-egu21-10163
https://doi.org/10.5194/egusphere-egu21-10163
The efficiency of the solar wind interaction with the Earth's magnetosphere is determined not only by the values of solar wind parameters, but also by the direction of its flow. As a rule, the slow quiet and uniform solar wind extends radially, but a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d486a7443d84ff0a09a02d990488855c
https://doi.org/10.5194/egusphere-egu21-13829
https://doi.org/10.5194/egusphere-egu21-13829