Solar flare forcing on ionization of upper atmosphere. comparative study of several major X-class events of 23rd and 24th solar cycles

被引：0

作者：

V. E. Kunitsyn

M. O. Nazarenko

I. A. Nesterova

A. M. Padokhin

机构：

[1] Moscow State University,Schmidt Institute of Physics of the Earth

[2] Russian Academy of Sciences,undefined

来源：

Moscow University Physics Bulletin | 2015年 / 70卷

关键词：

Solar Flares; Ionosphere; Total Electron Content; GNSS; Radio Tomography; X-Ray and EUV radiation;

D O I：

暂无

中图分类号：

学科分类号：

摘要：

By analyzing the GNSS (Global Navigational Satellite Systems) signals recorded at the IGS (International GNSS Service) network, we compare the effects of ionization of the upper atmosphere by a series of intense X-class solar flares during the 23rd and 24th solar cycles. We develop the methods for estimating the geo-effectiveness of solar flares from the GNSS data and suggest using the rate of change of the ionospheric total electron content averaged over all the receiving stations located on the sunlit side of the Earth reduced to the solar zenith angle during the flare as the characteristic of the flare’s geo-effectiveness.

引用

页码：312 / 318

页数：6

共 21 条

[1] Solar flare forcing on ionization of upper atmosphere. comparative study of several major X-class events of 23rd and 24th solar cycles
Kunitsyn, V. E.
Nazarenko, M. O.
Nesterov, I. A.
Padokhin, A. M.
MOSCOW UNIVERSITY PHYSICS BULLETIN, 2015, 70 (04) : 312 - 318
[2] Global Electron Content in the 23rd and 24th Solar Cycles
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[3] Solar Activity Indices for Ionospheric Parameters in the 23rd and 24th Cycles
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[4] Solar Activity Indices for Ionospheric Parameters in the 23rd and 24th Cycles
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Geomagnetism and Aeronomy, 2020, 60 : 1 - 6
[5] Forecasting the 23rd and 24th solar cycles on the basis of MGM spectrum
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I. A. Danilchenko
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R. Carbone
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[9] Features of cosmic ray variation at the phase of the minimum between the 23rd and 24th solar cycles
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Bulletin of the Russian Academy of Sciences: Physics, 2011, 75 (6) : 782 - 785
[10] Suprathermal ions in quiescent periods at 1 AU in the 23rd and 24th solar-activity cycles
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