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20232025
most citedExact solution to the problem of slow oscillations in coronal loops and its diagnostic applications

10 citations · 23 across the 6 of their papers we have counts for

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6 papers · 1 filter

astro-ph.SR2025

Detection of kink oscillations in solar coronal loops by a CNN-LSTM neural network

Sergey A. Belov, Yu Zhong, Dmitrii Y. Kolotkov +1

A hybrid machine learning model which combines a shallow convolutional neural network and a long short-term memory network (CNN--LSTM), has been developed to automate the detection…

astro-ph.SR20256 cited

Solar Flare Ion Temperatures

Alexander J. B. Russell, Vanessa Polito, Paola Testa +2

This paper proposes that the ion temperature is several times the local electron temperature in the hot onset phase and at the above-the-loop region of solar flares. The paper cons…

astro-ph.SR2025

Thermodynamic Evolution of Flaring Loops with Non-local Thermal Transport

S. Belov, T. Parmenter, T. Arber +3

Hot solar coronal loops, such as flaring loops, reach temperatures where the thermal transport becomes non-local. This occurs when the mean-free-path of electrons can no longer be…

astro-ph.SR20244 cited

Non-local thermal transport impact on compressive waves in two-temperature coronal loops

S. A. Belov, T. Goffrey, T. D. Arber +1

Context. Observations of slow magnetoacoustic waves in solar coronal loops suggest that, in hot coronal plasma, heat conduction may be suppressed in comparison with the classical t…

astro-ph.SR20233 cited

On collective nature of nonlinear torsional Alfvén waves

S. A. Belov, D. I. Riashchikov, D. Y. Kolotkov +3

Torsional Alfvén waves in coronal plasma loops are usually considered to be non-collective, i.e. consist of cylindrical surfaces evolving independently, which significantly complic…

astro-ph.SR202310 cited

Exact solution to the problem of slow oscillations in coronal loops and its diagnostic applications

Dmitrii I. Zavershinskii, Nonna E. Molevich, Dmitrii S. Riashchikov +1

Magnetoacoustic oscillations are nowadays routinely observed in various regions of the solar corona. This allows them to be used as means of diagnosing plasma parameters and proces…