Comparison of BBFs observed by single and multi satellites

留言板

尊敬的读者、作者、审稿人, 关于本刊的投稿、审稿、编辑和出版的任何问题, 您可以本页添加留言。我们将尽快给您答复。谢谢您的支持!

姓名

邮箱

手机号码

标题

留言内容

验证码

1.
School of Astronautics, Beihang University, Beijing, 100191, China
2.
State Key Laboratory of Space Weather, Center for Space Science and Applied Research, Chinese Academy of Sciences, Beijing, China
3.
Graduate University of Chinese Academy of Sciences, Beijing, China

1.
School of Astronautics, Beihang University, Beijing, 100191, China
2.
State Key Laboratory of Space Weather, Center for Space Science and Applied Research, Chinese Academy of Sciences, Beijing, China
3.
Graduate University of Chinese Academy of Sciences, Beijing, China

摘要: This paper, using the data of three Cluster satellites, compares the observations of Bursty Bulk Flow (BBF) by single satellite with those by multi satellites. The results indicate that there exists remarkable difference between observations of BBF by single satellite and multi satellites. The observations of BBF by a single satellite depend on its position relative to the flow channel. The difference is caused by the localization characteristics of fast flows in the plasma sheet, and can lead to diverging views about substorm and causal relations among substorm phenomena.
- Bursty Bulk Flow (BBF) /
- Plasma sheet /
- Substorm Bursty Bulk Flow
Abstract: This paper, using the data of three Cluster satellites, compares the observations of Bursty Bulk Flow (BBF) by single satellite with those by multi satellites. The results indicate that there exists remarkable difference between observations of BBF by single satellite and multi satellites. The observations of BBF by a single satellite depend on its position relative to the flow channel. The difference is caused by the localization characteristics of fast flows in the plasma sheet, and can lead to diverging views about substorm and causal relations among substorm phenomena.
- Bursty Bulk Flow (BBF) /
- Plasma sheet /
- Substorm Bursty Bulk Flow