2014年2月25日爆发的近翼X4.9太阳耀斑的磁场动力学和光球发射源的高节奏观测:脉冲阶段两阶段磁重联的证据

IF 0.6 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS
I. N. Sharykin, I. V. Zimovets, A. V. Radivon
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引用次数: 0

摘要

本文的勘误表已发表:https://doi.org/10.1134/S0010952523330031
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Erratum to: High-Cadence Observations of Magnetic Field Dynamics and Photospheric Emission Sources in the Eruptive Near-the-Limb X4.9 Solar Flare on 25 February, 2014: Evidences for Two-Stage Magnetic Reconnection during the Impulsive Phase

An Erratum to this paper has been published: https://doi.org/10.1134/S0010952523330031

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来源期刊
Cosmic Research
Cosmic Research 地学天文-工程:宇航
CiteScore
1.10
自引率
33.30%
发文量
41
审稿时长
6-12 weeks
期刊介绍: Cosmic Research publishes scientific papers covering all subjects of space science and technology, including the following: ballistics, flight dynamics of the Earth’s artificial satellites and automatic interplanetary stations; problems of transatmospheric descent; design and structure of spacecraft and scientific research instrumentation; life support systems and radiation safety of manned spacecrafts; exploration of the Earth from Space; exploration of near space; exploration of the Sun, planets, secondary planets, and interplanetary medium; exploration of stars, nebulae, interstellar medium, galaxies, and quasars from spacecraft; and various astrophysical problems related to space exploration. A chronicle of scientific events and other notices concerning the main topics of the journal are also presented.
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