
NSF Org: |
AGS Division of Atmospheric and Geospace Sciences |
Recipient: |
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Initial Amendment Date: | June 2, 2005 |
Latest Amendment Date: | April 28, 2008 |
Award Number: | 0531464 |
Award Instrument: | Continuing Grant |
Program Manager: |
Farzad Kamalabadi
AGS Division of Atmospheric and Geospace Sciences GEO Directorate for Geosciences |
Start Date: | March 1, 2005 |
End Date: | July 31, 2009 (Estimated) |
Total Intended Award Amount: | $462,099.00 |
Total Awarded Amount to Date: | $462,099.00 |
Funds Obligated to Date: |
FY 2005 = $95,988.00 FY 2006 = $99,895.00 FY 2007 = $99,994.00 FY 2008 = $99,547.00 |
History of Investigator: |
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Recipient Sponsored Research Office: |
1100 NE 45TH ST, STE 500 SEATTLE WA US 98105-4696 (206)556-8151 |
Sponsor Congressional District: |
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Primary Place of Performance: |
1100 NE 45TH ST, STE 500 SEATTLE WA US 98105-4696 |
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): | AERONOMY |
Primary Program Source: |
app-0105 app-0106 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
A comprehensive assay of the micrometeor flux using extant and new radar head-echo measurements quantifies the amount and temporal variability of dust deposition into the earth's middle atmosphere. The data are used to construct a meteor input function model that will be useful to studies of ionospheric E-region layering, sporadic-E formation, and to the communications disturbances associated with those phenomena. Additionally, the information concerning meteor trajectories prior to earth-encounter are important for understanding dust in the inner solar system, planetary formation and evolution, and evolution of the asteroid belt.
PUBLICATIONS PRODUCED AS A RESULT OF THIS RESEARCH
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