activity
20122025
most citedSolar Eruptions, Forbush Decreases and Geomagnetic Disturbances from Outstanding Active Region 12673

36 citations · 134 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.SR2025

On the features of great Forbush effect during May 2024 extreme geomagnetic storm

M. A. Abunina, N. S. Shlyk, A. V. Belov +2

The work investigates the features of galactic cosmic ray density and anisotropy behavior and their relation to solar sources, interplanetary and geomagnetic disturbances from May…

astro-ph.SR2019★ 36 cited

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

A. A. Abunin, M. A. Abunina, A. V. Belov +1

On the approach to minimum of Solar Cycle 24, on 26 August 2018, an unexpectedly strong geomagnetic storm (GMS) suddenly occurred. Its Dst index reached -174 nT, that is the third…

astro-ph.SR2018★ 36 cited

Solar Eruptions, Forbush Decreases and Geomagnetic Disturbances from Outstanding Active Region 12673

I. M. Chertok, A. V. Belov, A. A. Abunin

Based on our tool for the early diagnostics of solar eruption geoeffectiveness (EDSEG tool; Chertok et al., 2013, 2015, 2017), we have analyzed space weather disturbances that occu…

astro-ph.SR2017★ 11 cited

An Early Diagnostics of the Geoeffectiveness of Solar Eruptions from Photospheric Magnetic Flux Observations: The Transition from SOHO to SDO

I. M. Chertok, V. V. Grechnev, A. A. Abunin

In our previous articles (Chertok et al.: 2013, Solar Phys. 282, 175, and 2015, Solar Phys. 290, 627), we presented a preliminary tool for the early diagnostics of the geoeffective…

astro-ph.HE2016★ 3 cited

Forbush Decreases during the DeepMin and MiniMax of Solar Cycle 24

D. Lingri, H. Mavromichalaki, A. Belov +4

After a prolong and deep solar minimum at the end of solar cycle 23, the current cycle 24 is one of the lowest cycles. The two periods of deep minimum and mini-maximum of the cycle…

astro-ph.SR2014★ 13 cited

Relationship between the Magnetic Flux of Solar Eruptions and the Ap Index of Geomagnetic Storms

I. M. Chertok, M. A. Abunina, A. A. Abunin +2

Solar coronal mass ejections (CMEs) are main drivers of the most powerful non-recurrent geomagnetic storms. In the extreme-ultraviolet range, CMEs are accompanied by bright post-er…