Features of the Behavior of Microwave and Ultraviolet Emission of Solar Active Regions in Relation to Eruptive and Confined Flares

被引：1

作者：

Bakunina, I. A. ^{[1
]}

Melnikov, V. F. ^{[2
]}

Abramov-Maximov, V. E. ^{[2
]}

Morgachev, A. S. ^{[3
]}

机构：

[1] Natl Res Univ, Higher Sch Econ, Nizhnii Novgorod, Russia

[2] Russian Acad Sci, Cent Pulkovo Astron Observ, St Petersburg, Russia

[3] Nizhnii Novgorod State Univ, Nizhnii Novgorod, Russia

来源：

GEOMAGNETISM AND AERONOMY | 2021年 / 61卷 / 08期

基金：

俄罗斯基础研究基金会;

关键词：

D O I：

10.1134/S0016793221080028

中图分类号：

P3 [地球物理学]; P59 [地球化学];

学科分类号：

0708 ; 070902 ;

摘要：

In this study, a comparative analysis was carried out on the preflare and flare conditions for six flares accompanied by coronal mass ejections (CMEs) and five events not accompanied by CMEs. All of the events occurred in the period 2011-2014. The features of the spatial dynamics of microwave emission of active regions (data from the Nobeyama Radioheliograph) prior to the selected events and during flares were studied. For the same 11 events, the fine structure of active ultraviolet (UV) sources was examined based on SDO/AIA data. Certain differences were found in the behavior of microwave emission for events with CMEs. The features of the frequency radio spectra from the RATAN-600 data were found for some active regions.

引用

页码：1159 / 1171

页数：13

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