
NSF Org: |
AGS Division of Atmospheric and Geospace Sciences |
Recipient: |
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Initial Amendment Date: | July 17, 2006 |
Latest Amendment Date: | June 10, 2008 |
Award Number: | 0613886 |
Award Instrument: | Continuing Grant |
Program Manager: |
Paul Bellaire
AGS Division of Atmospheric and Geospace Sciences GEO Directorate for Geosciences |
Start Date: | August 1, 2006 |
End Date: | January 31, 2011 (Estimated) |
Total Intended Award Amount: | $404,932.00 |
Total Awarded Amount to Date: | $404,932.00 |
Funds Obligated to Date: |
FY 2007 = $135,000.00 FY 2008 = $135,000.00 |
History of Investigator: |
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Recipient Sponsored Research Office: |
1608 4TH ST STE 201 BERKELEY CA US 94710-1749 (510)643-3891 |
Sponsor Congressional District: |
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Primary Place of Performance: |
1608 4TH ST STE 201 BERKELEY CA US 94710-1749 |
Primary Place of
Performance Congressional District: |
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Unique Entity Identifier (UEI): |
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Parent UEI: |
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NSF Program(s): |
SOLAR-TERRESTRIAL, MAGNETOSPHERIC PHYSICS |
Primary Program Source: |
app-0107 01000809DB NSF RESEARCH & RELATED ACTIVIT |
Program Reference Code(s): |
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Program Element Code(s): |
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Award Agency Code: | 4900 |
Fund Agency Code: | 4900 |
Assistance Listing Number(s): | 47.050 |
ABSTRACT
This research addresses outstanding questions in reconnection physics by using observations of the heliospheric current sheet. The Principal Investigator will use solar wind data from the Wind, Cluster, and Advanced Composition Explorer (ACE) spacecraft to study reconnection events in situ. In addition to exploring basic plasma physics, the proposal objectives are to determine the dependence of reconnection on the magnitude of the guide field (the magnetic shear across the current sheet), whether such reconnection is steady or intermittent, and which parameters are important for controlling the reconnection rate.
PUBLICATIONS PRODUCED AS A RESULT OF THIS RESEARCH
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