Azimuthal velocity shear within an Earthward fast flow – further evidence for magnetotail untwisting?
It is well known that nonzero interplanetary magnetic field <i>B<sub>y</sub></i> conditions lead to a twisted magnetotail configuration. The plasma sheet is rotated around its axis and tail magnetic field lines are twisted, which causes an azimuthal displacement of their ionospheric footprints. A...
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| Hoofdauteurs: | , , , , , , , |
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| Formaat: | Artigo |
| Taal: | Inglês |
| Gepubliceerd in: |
Copernicus Publications
2015-03-01
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| Reeks: | Annales Geophysicae |
| Online toegang: | https://www.ann-geophys.net/33/245/2015/angeo-33-245-2015.pdf |
| Tags: |
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