NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Magnetic Merging Locations Deduced from: Slow-Mode Shock Orientation Determinations, Boundary Layer Wave Intensities and Energetic Ion Velocity Dispersion in the Distant Geomagnetic TailSeveral techniques will be used to determine the location of the magnetic reconnection in the distant geomagnetic tail using the ISEE-3. Techniques to be used are calculated wave-particle scattering time, plasmoid source location (if a plasmoid is found), analysis of the magnetic field geometry and slow-mode shock orientation, and examination of the magnetic field Bz components and plasma bulk speeds.
Document ID
20060037017
Acquisition Source
Jet Propulsion Laboratory
Document Type
Preprint (Draft being sent to journal)
External Source(s)
Authors
Ho, C. M.
Tsurutani, B. T.
Smith, E. J.
Murphy, N.
Date Acquired
August 23, 2013
Publication Date
July 1, 1995
Subject Category
Geophysics
Distribution Limits
Public
Copyright
Other
Keywords
geomagnetic tail ISEE-3 magnetic fields

Available Downloads

There are no available downloads for this record.
No Preview Available