In:
Journal of Geophysical Research: Space Physics, American Geophysical Union (AGU), Vol. 125, No. 3 ( 2020-03)
Abstract:
Coronal mass ejections drive more intense nightside reconnection than high speed streams Under extreme conditions, magnetic reconnection produces a distorted Hall magnetic field pattern in the plasma sheet Continued intense solar wind forcing does not produce substorm magnetic flux loading and unloading of tail lobe instead steady convection
Type of Medium:
Online Resource
ISSN:
2169-9380
,
2169-9402
DOI:
10.1029/2019JA027490
Language:
English
Publisher:
American Geophysical Union (AGU)
Publication Date:
2020
detail.hit.zdb_id:
2033040-6
detail.hit.zdb_id:
161665-1
detail.hit.zdb_id:
3094181-7
SSG:
16,13