.png){kind=icon}
返回
Slow Solar Wind: Observations and Modeling
.png){kind=icon}
PRE
AI
DOI：10.1007/s11214-016-0264-1.png)
.png){kind=icon}
原文求助.png){kind=icon}
分享.png){kind=icon}
收藏
摘要
En 中文
While it is certain that the fast solar wind originates from coronal holes, where and how the slow solar wind (SSW) is formed remains an outstanding question in solar physics even in the post-SOHO era. The quest for the SSW origin forms a major objective for the planned future missions such as the Solar Orbiter and Solar Probe Plus. Nonetheless, results from spacecraft data, combined with theoretical modeling, have helped to investigate many aspects of the SSW. Fundamental physical properties of the coronal plasma have been derived from spectroscopic and imaging remote-sensing data and in situ data, and these results have provided crucial insights for a deeper understanding of the origin and acceleration of the SSW. Advanced models of the SSW in coronal streamers and other structures have been developed using 3D MHD and multi-fluid equations. However, the following questions remain open: What are the source regions and their contributions to the SSW? What is the role of the magnetic topology in the corona for the origin, acceleration and energy deposition of the SSW? What are the possible acceleration and heating mechanisms for the SSW? The aim of this review is to present insights on the SSW origin and formation gathered from the discussions at the International Space Science Institute (ISSI) by the Team entitled Slow solar wind sources and acceleration mechanisms in the corona held in Bern (Switzerland) in March 2014 and 2015.
Keyword:
Sun
Corona
Solar wind
Coronal streamers
MHD and kinetic models
AI总结
对已上传原文的论文进行重点信息的提取，主要内容包括：简要概述、研究摘要、背景介绍、关键亮点、图文解析、展望与总结。
期刊
IF:
7.4
论文数:
4.2K
被引数:
1.8W
机构
引用论文
分享收藏分享收藏Co-expression of the voltage-gated potassium channel Kv1.4 with transient receptor potential channels (TRPV1 and TRPV2) and the cannabinoid receptor CB1 in rat dorsal root ganglion neurons电压门控钾通道Kv1.4与瞬时受体电位通道 (TRPV1和TRPV2) 和大麻素受体CB1在大鼠背根神经节神经元中的共表达.png)
Neuroscience
NeuroscienceIF0
PREAI
分享收藏Full-Sun observations for identifying the source of the slow solar windNATURE COMMUNICATIONS
OAAI
NATURE COMMUNICATIONSIF15.7
OAAI分享收藏分享收藏
查看更多内容