Abstract
The location of magnetic reconnection in the mid-tail during a substorm was studied in many researches. Here we present multi-point THEMIS observations of a reconnection event in the near-Earth magnetotail during substorm. In this event, THEMIS probes stayed in the near-Earth and mid-tail region aligning along the magnetotail. This allows reconnection evolution to be probed simultaneously from about g-10 to g-23 down tail. The Hall current related electron streams were observed at the same time by two probes far away from the reconnection site. Before near-Earth reconnection involved the tail lobe magnetic field, the reconnection site was restricted in earthward g -23 . When reconnection involved into the tail lobe region, the reconnection site started to retreat gradually.
| Original language | English |
|---|---|
| Pages (from-to) | 143-151 |
| Number of pages | 9 |
| Journal | Annales Geophysicae |
| Volume | 30 |
| Issue number | 1 |
| DOIs | |
| State | Published - 2012 |
| Externally published | Yes |
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