Relay-assisted deep space optical communication system over coronal fading channels

G Xu, Q Zhang, Z Song, B Ai - IEEE Transactions on Aerospace …, 2023 - ieeexplore.ieee.org
The integration of free-space optical (FSO) communications and relay technology has been
envisioned as a promising and effective solution to achieve substantial performance gains …

Peculiar solar sources and geospace disturbances on 20–26 August 2018

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 …

Statistical comparison of time profiles of Forbush decreases associated with coronal mass ejections and streams from coronal holes in solar cycles 23–24

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) …

The two-step Forbush decrease: a tale of two substructures modulating galactic cosmic rays within coronal mass ejections

M Janvier, P Démoulin, J Guo, S Dasso… - The Astrophysical …, 2021 - iopscience.iop.org
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 …

Forbush decreases associated with coronal mass ejections from active and non-active regions: statistical comparison

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 …

Generic profile of a long-lived corotating interaction region and associated recurrent Forbush decrease

M Dumbović, B Vršnak, M Temmer, B Heber… - Astronomy & …, 2022 - aanda.org
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 …

A preliminary investigation of the empirical relationship between small-amplitude Forbush Decreases and solar wind disturbances

FM Menteso, AE Chukwude, O Okike… - Monthly Notices of the …, 2023 - academic.oup.com
High-magnitude (amplitude) Forbush decreases (FDs) are generally employed by
researchers investigating the solar-terrestrial connection mechanisms. Although it has been …

Study of the cosmic-ray modulation during the passage of ICMEs and CIRs

Badruddin, A Kumar - Solar Physics, 2016 - Springer
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 …

Comparison between statistical properties of Forbush decreases caused by solar wind disturbances from coronal mass ejections and coronal holes

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 …

Testing the impact of coronal mass ejections on cosmic-ray intensity modulation with algorithm selected Forbush decreases

O Okike, OC Nwuzor, FC Odo, EU Iyida… - Monthly Notices of …, 2021 - academic.oup.com
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 …