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The Origin and Evolution of Deep Plasmaspheric NotchesDeep plasmaspheric notches can extend over more than 2 RE and 3 hours MLT in the magnetic equatorial plane. They can last for days and exhibit varying structure. In this presentation, the low L-shell portion of the recovery-time plasmaspheric convection plume will be explored as the source for these deep evacuations in density. Interactions with the ring current will be explored as the source of features observed in these density depletions.
Document ID
20040034030
Acquisition Source
Marshall Space Flight Center
Document Type
Conference Paper
Authors
Gallagher, D. (NASA Marshall Space Flight Center Huntsville, AL, United States)
Adrian, M. (Alabama Univ. Huntsville, AL, United States)
Liemohn, M. (Maryland Univ.)
Date Acquired
August 21, 2013
Publication Date
January 1, 2004
Subject Category
Astronomy
Meeting Information
Meeting: Inner Magnetosphere Interactions Workshop
Location: Yosemite, CA
Country: United States
Start Date: February 2, 2004
End Date: February 7, 2004
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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