Zobrazeno 1 - 10
of 12
pro vyhledávání: '"Alexander Khokhlachev"'
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:
Cosmic Research. 59:415-426
Publikováno v:
Cosmic Research. 58:492-500
One perturbed type of solar wind and magnetospheric disturbance drivers is the compression region in front of fast ICMEs—the Sheath region. In front of this region, an interplanetary shock is observed in approximately half of cases. However, the pa
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
Publikováno v:
Cosmic Research. 58:338-356
This paper is a continuation of our works [1, 2], in which we discussed some incorrect approaches to identifying large-scale types of solar wind and related incorrect conclusions drawn when analyzing the solar-terrestrial physics data. In this paper,
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
Helium is the second most abundant ion component of the solar wind. The relative abundance of helium can differ significantly in various large-scale structures of the solar wind generated by the nonstationarity and inhomogeneity of the solar corona.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8a9706662f57d36ab69253ca7c4a2210
https://doi.org/10.5194/egusphere-egu21-11947
https://doi.org/10.5194/egusphere-egu21-11947
Autor:
Liudmila Rakhmanova, Natalia Borodkova, O. V. Sapunova, Yuri Yermolaev, Michael Yermolaev, Irina Lodkina, Alexander Khokhlachev, Maria Riazantseva
We study the behavior of solar wind (SW) parameters over 21-24 solar cycles (SCs). We take into account that these variation can depend on three reasons: (1) type of SW, (2) phase of SC, and (3) SC...
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::befd773f53839987db304d7a5d30394a
https://doi.org/10.1002/essoar.10504870.1
https://doi.org/10.1002/essoar.10504870.1
Autor:
Maria Riazantseva, Liudmila Rakhmanova, Yuri Yermolaev, Alexander Khokhlachev, Irina Lodkina, Georgy Zastenker
The boundaries between large-scale solar wind streams are often accompanied by sharp changes in helium abundance. Wherein the high value of relative helium abundance is known as a sign of some large-scale solar wind structures ( for example magnetic
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b247b098938efcd04ae20d8666e57e39
https://doi.org/10.5194/egusphere-egu2020-9348
https://doi.org/10.5194/egusphere-egu2020-9348