activity
20162023
most citedPlasma heating in solar microflares: statistics and analysis

36 citations · 107 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2023★ 4 cited

Observations of the Current Sheet Heating in X-ray during a Solar Flare

Anton Reva, Sergey Bogachev, Ivan Loboda +2

In the solar corona, magnetic reconnection occurs due to the finite resistivity of the plasma. At the same time, resistivity leads to ohmic heating. Therefore, the reconnecting cur…

astro-ph.IM2019★ 6 cited

The soft X-ray spectrometer polarimeter SolpeX

J. Sylwester, M. Stęślicki, J. Bąkała +15

We present a novel X-ray assembly of functionally related instrument blocks intended to measure solar flare and active region (AR) spectra from within the Russian instrument comple…

astro-ph.SR2018★ 15 cited

Estimate of the Upper Limit on Hot Plasma Differential Emission Measure (DEM) in Non-Flaring Active Regions and Nanoflare Frequency Based on the Mg XII Spectroheliograph Data from CORONAS-F/SPIRIT

Anton Reva, Artem Ulyanov, Alexey Kirichenko +2

The nanoflare-heating theory predicts steady hot plasma emission in the non-flaring active regions. It is hard to find this emission with conventional non-monochromatic imagers (su…

astro-ph.SR2017★ 30 cited

The Relation between Magnetic Fields and X-ray Emission for Solar Microflares and Active Regions

A. S. Kirichenko, S. A. Bogachev

We present the result of comparison between magnetic field parameters and the intensity of X-ray emission for solar microflares with Geosynchronous Operational Environmental Satell…

astro-ph.SR2017★ 36 cited

Plasma heating in solar microflares: statistics and analysis

A. S. Kirichenko, S. A. Bogachev

In this paper, we present the results of an analysis of 481 weak solar flares, from A0.01 to the B \textit{GOES} class, that were observed during the period of extremely low solar…

astro-ph.SR2016★ 16 cited

Plasma dynamics in solar macrospicules from high-cadence EUV observations

I. P. Loboda, S. A. Bogachev

Macrospicules are relatively large spicule-like formations found mainly over the polar coronal holes when observing in the transition region spectral lines. In this study, we took…