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Reconfiguration of the coronal magnetic field by means of reconnection driven by photospheric magnet
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相关项目:太阳风中阿尔芬波的起源
同期刊论文项目
太阳风中阿尔芬波的起源
期刊论文 23
会议论文 4
同项目期刊论文
The Nascent Fast Solar Wind Observed by the EUV Imaging Spectrometer on Board Hinode,
Multi-scale pressure-balanced structures in the solar wind observed by WIND
太阳风中小尺度磁通量管边界重联的统计研究
POSSIBLE EVIDENCE OF ALFVEN-CYCLOTRON WAVES IN THE ANGLE DISTRIBUTION OF MAGNETIC HELICITY OF SOLAR
MAGNETOSEISMOLOGICAL DETERMINATION OF MAGNETIC FIELD AND PLASMA DENSITY HEIGHT VARIATION IN A SOLAR
Identification of prominence ejecta by the proton distribution function and magnetic fine structure
Horizontal supergranule-scale motions inferred from TRACE ultraviolet observations of the chromosphe
Upward propagating high-frequency Alfvén waves as identified from dynamic wave-like spicules observe
Excitation of Kink Waves Due to Small-Scale Magnetic Reconnection in the Chromosphere
Upflows in funnel-like legs of coronal magnetic loops
Hydrogen Ly-α and Ly-β Radiances and Profiles in Polar Coronal Holes
Solar transition region above sunspots
Intermittent outflows at the edge of an active region - a possible source of the solar wind
Magnetic and spectroscopic properties of supergranular-scale coronal jets and erupting loops in a po
日冕亮点的观测特征和供能机制
太阳过渡区的结构与特性
太阳大气中氢原子的赖曼谱线