
NSF Org: |
AGS Division of Atmospheric and Geospace Sciences |
Recipient: |
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Initial Amendment Date: | September 14, 2009 |
Latest Amendment Date: | September 14, 2009 |
Award Number: | 0921979 |
Award Instrument: | Standard Grant |
Program Manager: |
Rachel Walker-Kulzick
AGS Division of Atmospheric and Geospace Sciences GEO Directorate for Geosciences |
Start Date: | September 15, 2009 |
End Date: | August 31, 2013 (Estimated) |
Total Intended Award Amount: | $127,432.00 |
Total Awarded Amount to Date: | $127,432.00 |
Funds Obligated to Date: |
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ARRA Amount: | $127,432.00 |
History of Investigator: |
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Recipient Sponsored Research Office: |
7 LEBANON ST HANOVER NH US 03755-2170 (603)646-3007 |
Sponsor Congressional District: |
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Primary Place of Performance: |
7 LEBANON ST HANOVER NH US 03755-2170 |
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): | MAGNETOSPHERIC PHYSICS |
Primary Program Source: |
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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 award is funded under the American Recovery and Reinvestment Act of 2009 (Public Law 111-5).
This project will improve our ability to predict the access of solar energetic protons to Earth's magnetosphere and ionosphere. Solar energetic particle (SEP) events have strong space weather impacts and can change the radiation environment in the radiation belts and can modify the ionosphere. The project will make use of state-of-the-art empirical models of Earth's magnetic field as well as physics-based models of the coupled ionosphere and magnetosphere. The project will compare the different models with ground-based observations to determine the errors incurred by the various assumptions made by the different models. The project will involve research done by undergraduate students.
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