AA Abunin, MA Abunina, AV Belov, IM Chertok - Solar Physics, 2020 - Springer
On the approach to minimum of Solar Cycle 24, on 26 August 2018, an unexpectedly strong geomagnetic storm (GMS) suddenly occurred. Its D st D_st index reached− 174 nT -174~nT …
AA Melkumyan, AV Belov, NS Shlyk… - Monthly Notices of …, 2023 - academic.oup.com
In this paper, Forbush decrease (FD) profiles are compared for events associated with (i) coronal mass ejections from active regions accompanied by solar flares (AR CMEs),(ii) …
Interplanetary coronal mass ejections (ICMEs) are known to modify the structure of the solar wind as well as interact with the space environment of planetary systems. Their large …
AA Melkumyan, AV Belov, MA Abunina… - Monthly Notices of …, 2022 - academic.oup.com
In this paper, Forbush decreases (FDs) from 1997 to 2020 associated with coronal mass ejections from active and non-active regions are compared between themselves and to FDs …
Context. Corotating interaction regions (CIRs), formed by the interaction of slow solar wind and fast streams that originate from coronal holes (CHs), produce recurrent Forbush …
High-magnitude (amplitude) Forbush decreases (FDs) are generally employed by researchers investigating the solar-terrestrial connection mechanisms. Although it has been …
We compare the cosmic-ray response to interplanetary coronal mass ejections (ICMEs) and corotating interaction regions (CIRs) during their passage in near-Earth space. We study the …
AA Melkumyan, AV Belov, MA Abunina… - Advances in Space …, 2019 - Elsevier
In this paper, we compare Forbush decreases associated with solar wind disturbances from two types of solar sources: coronal mass ejections (sporadic Forbush decreases) and …
The relationship between coronal mass ejections (CMEs) and Forbush decreases (FDs) has been investigated in the past. But the selection of both solar events are difficult. Researchers …