Search Results - "Kryshtal, A. N."
-
1
Small-scale Langmuir wave instability in preflare chromosphere of solar active region
Published in Astrophysics and space science (01-02-2014)“…Necessary conditions have been investigated for the appearance of instability of high-frequency electron Langmuir waves in plasma of solar chromosphere near…”
Get full text
Journal Article -
2
One type of three-wave interaction of low-frequency waves in magnetoactive plasma of the solar atmosphere
Published in Kinematics and physics of celestial bodies (01-05-2014)“…We study the process of occurrence of “quasi-mode” decay instability of kinetic Alfven waves (KAW) in the chromosphere of a solar active region before a flare,…”
Get full text
Journal Article -
3
On the possibility of the development of longitudinal wave instabilities on the background of the small-scale Bernstein turbulence in preflare chromosphere of a solar active region
Published in Kinematics and physics of celestial bodies (01-09-2014)“…The process of origination and development of instabilities of the longitudinal waves of two types, namely, low-frequency ion-acoustic and high-frequency…”
Get full text
Journal Article -
4
Low-Frequency Kinetic Waves in Plasmas of Magnetic Loops at the Early Stage of a Flare Process in an Active Region
Published in Kinematics and physics of celestial bodies (01-05-2019)“…The process of the rise and development of low-frequency instability of kinetic Alfven waves (KAW) and kinetic ion-acoustic waves (KIAW) in preflare solar…”
Get full text
Journal Article -
5
Kink mode m = 1 in a thin plasma filament with discontinuous vertical magnetic field
Published in Kinematics and physics of celestial bodies (01-05-2017)“…In this paper, we study the conditions of realization and stability of kink modes with azimuthal wave numbers m = ±1 in a cylindrical plasma filament with a…”
Get full text
Journal Article -
6
Effect of small-scale bernstein turbulence on low-frequency plasma waves in the preflare solar chromosphere
Published in Kinematics and physics of celestial bodies (01-07-2017)“…The studied region is a part of the current circuit of a magnetic loop in a solar active region in the altitude range of 1400–2500 km above the photosphere. At…”
Get full text
Journal Article -
7
“Oblique” Bernstein modes in solar preflare plasma: Generation of second harmonics
Published in Advances in space research (15-02-2012)“…Process of second harmonics generation due to development of corresponding instability has been investigated for pure electron weakly oblique Bernstein mode…”
Get full text
Journal Article -
8
Decay instability of kinetic Alfvén waves in preflare plasmas of the loops in active solar regions
Published in Kinematics and physics of celestial bodies (01-06-2007)“…We examine the physical conditions for the origin of the decay instability of kinetic Alfvén waves in loop plasmas at the early flare stages. The synchronism…”
Get full text
Journal Article -
9
Incompressible MHD modes in the thin magnetically twisted flux tube
Published 03-07-2017“…Context. Observations have shown that twisted magnetic fields naturally occur, and indeed are omnipresent in the Sun's atmosphere. It is therefore of great…”
Get full text
Journal Article -
10
Kinetic Alfvén waves in preflare plasma
Published in Astronomische Nachrichten (01-01-2005)“…Low‐frequency instabilities of plasma waves in the arch structures in solar active regions have been investigated before a flare. In the framework of mechanism…”
Get full text
Journal Article -
11
Kink mode m=1 in magnetic tube with discontinuous magnetic field
Published in Advances in space research (15-01-2018)“…In this paper, we study conditions of realization and stability of kink modes with azimuthal wave numbers m=±1 in cylindrical plasma flex with twisted magnetic…”
Get full text
Journal Article -
12
Ion-acoustic instability caused by large-scale electric field in solar active regions
Published in Solar physics (01-04-1996)“…The ion-acoustic instability caused by large-scale electric fields is considered for plasmas of solar active regions. The dispersion relation has been obtained…”
Get full text
Journal Article -
13