Standing shocks in the inner slow solar wind

Bo Li*, Yan Jun Chen, Xing Li

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

2 Citations (SciVal)


We examine whether the now tube along the edge of a coronal streamer supports standing shocks in the inner slow wind by solving an isothermal wind model in terms of the Lambert W function. It is shown that solutions with standing shocks do exist and they exist in a broad area in the parameter space characterizing the wind temperature and now tube. In particular, streamers with cusps located at a heliocentric distance ≳ 3.2R can readily support discontinuous slow winds with temperatures barely higher than 1 MK.

Original languageEnglish
Article number059601
JournalChinese Physics Letters
Issue number5
Publication statusPublished - May 2011


Dive into the research topics of 'Standing shocks in the inner slow solar wind'. Together they form a unique fingerprint.

Cite this