
NSF Org: |
AGS Division of Atmospheric and Geospace Sciences |
Recipient: |
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Initial Amendment Date: | January 23, 2006 |
Latest Amendment Date: | January 11, 2008 |
Award Number: | 0517641 |
Award Instrument: | Continuing Grant |
Program Manager: |
Cassandra G. Fesen
AGS Division of Atmospheric and Geospace Sciences GEO Directorate for Geosciences |
Start Date: | February 1, 2006 |
End Date: | January 31, 2009 (Estimated) |
Total Intended Award Amount: | $223,538.00 |
Total Awarded Amount to Date: | $223,538.00 |
Funds Obligated to Date: |
FY 2007 = $71,740.00 FY 2008 = $73,502.00 |
History of Investigator: |
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Recipient Sponsored Research Office: |
506 S WRIGHT ST URBANA IL US 61801-3620 (217)333-2187 |
Sponsor Congressional District: |
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Primary Place of Performance: |
506 S WRIGHT ST URBANA IL US 61801-3620 |
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-0106 app-0107 |
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
The propagation of F-region equatorial irregularities along a common magnetic flux tube or along nearly common flux tubes is investigated using instruments deployed at Neiva, Columbia and at Cerro Tololo, Chile. The instruments deployed are all-sky imaging systems using 777.4 nm, 620.0 nm, and 557.7 nm narrow-band filters, and 50-Hz high sampling rate "ScintMon" GPS receivers. These instruments are complemented by the Jicamarca Peru ISR, other GPS receivers in South America, and C/NOFS satellite measurements to determine how local irregularity and scintillation data can be reconciled with physics of plasma transport along an entire magnetic flux tube.
PUBLICATIONS PRODUCED AS A RESULT OF THIS RESEARCH
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