NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Collections About News Help Login
Back to Results
Terrestrial Response to Eruptive Solar Flares: Geomagnetic StormsThis paper describes the interplanetary structures that are associated with the large-amplitude and long-duration negative B subscript z fields that are found in the sheath field and/or driver gas regions of the shock and are thought to be the main cause of the intense storms.
Document ID
20060042388
Acquisition Source
Jet Propulsion Laboratory
Document Type
Preprint (Draft being sent to journal)
External Source(s)
hdl:2014/36708
Authors
Gonzalez, W.
Date Acquired
August 23, 2013
Publication Date
January 1, 1992
Subject Category
Geophysics
Distribution Limits
Public
Copyright
Other
Keywords
solar flares geomagnetic storms magnetic field data plasma data

Available Downloads

There are no available downloads for this record.

Related Records

There are no records associated with this record.
No Preview Available