A scheme for finding the front boundary of an interplanetary magnetic cloud
We develop a scheme for finding a "refined" front boundary-time (<I>t<sub>B</sub></I>*) of an interplanetary magnetic cloud (MC) based on criteria that depend on the possible existence of any one or more of four specific solar wind features. The features that the...
| Main Authors: | , , |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
Copernicus Publications
2009-03-01
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| Series: | Annales Geophysicae |
| Online Access: | https://www.ann-geophys.net/27/1295/2009/angeo-27-1295-2009.pdf |