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|Title: ||Terrestrial Response to Eruptive Solar Flares: Geomagnetic Storms|
|Authors: ||Gonzalez, W.|
|Issue Date: ||1992 |
|Abstract: ||This 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.|
|Appears in Collections:||JPL TRS 1992+|
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