The Solar Origin of Space Weather
A special issue of Universe (ISSN 2218-1997). This special issue belongs to the section "Space Science".
Deadline for manuscript submissions: closed (30 June 2023) | Viewed by 3774
Special Issue Editors
Interests: coronal mass ejection and its relative phenomenon; geomagnetic storms; propagation of CMEs in the heliosphere
Interests: solar physics; space physics; space weather
Special Issue Information
Dear Colleagues,
Geomagnetic storms, which cause a wide range of undesirable consequences, such as satellite system disruption, damage to ground-based electric power grids, and interruptions of high-frequency communications and satellite navigation systems, are primarily caused by the coupling of the southward interplanetary magnetic field and the magnetosphere. Interplanetary coronal mass ejections (ICMEs) and stream interaction regions (SIRs) are the primary carriers of the intense south component of the interplanetary magnetic field and are thought to be the primary source of geomagnetic storms. The prediction of the southern magnetic field carried by ICMEs or SIRs and the magnitude of resulting geomagnetic storms are important topics in the space weather forecast. With this Special Issue, we aim to improve our space weather forecast ability.
The Special Issue is essential to fully comprehend space weather prediction, including CME dynamics, CME magnetic field evolution, and the solar origin of geomagnetic storms. We solicit papers include, but are not limited to, coronal mass ejections, stream interaction regions, the interplanetary southerly magnetic field carried by solar eruption transients, geomagnetic storms, and space weather forecast and modelling.
Dr. Yutian Chi
Prof. Dr. Hongqiang Song
Dr. Wageesh Mishra
Guest Editors
Manuscript Submission Information
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Keywords
- southward magnetic field
- geomagnetic storms
- coronal mass ejections
- corotating interaction regions
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