
NSF Org: |
AGS Division of Atmospheric and Geospace Sciences |
Recipient: |
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Initial Amendment Date: | January 4, 2021 |
Latest Amendment Date: | May 21, 2021 |
Award Number: | 2053689 |
Award Instrument: | Standard Grant |
Program Manager: |
Chia-Lin Huang
chihuang@nsf.gov (703)292-7544 AGS Division of Atmospheric and Geospace Sciences GEO Directorate for Geosciences |
Start Date: | January 15, 2021 |
End Date: | January 31, 2024 (Estimated) |
Total Intended Award Amount: | $225,521.00 |
Total Awarded Amount to Date: | $225,521.00 |
Funds Obligated to Date: |
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History of Investigator: |
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Recipient Sponsored Research Office: |
503 S BROAD ST CLINTON SC US 29325-2998 (864)833-8489 |
Sponsor Congressional District: |
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Primary Place of Performance: |
503 S. Broad St. Clinton SC US 29325-2998 |
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
Society relies upon technologies such as power distribution systems and constellations of communications satellites for daily functioning. These technologies are susceptible to the effects of magnetic storms and other severe space weather. This project will study what factors lead to space weather in an effort to better predict impacts. Additionally, the work will involve undergraduate students from under-represented groups in STEM in research at a primarily undergraduate institution. Additionally, an Artist in Residence program will be developed to increase general science literacy and to make links between space science and art.
The science objective is to determine nonlinear metrics that specify the dynamical state of the magnetosphere prior to the onset of, and during, extreme space weather. The research will investigate and statistically characterize, model, and forecast the spatiotemporal fluctuations of the ground magnetic field using advanced mathematical techniques. The central hypothesis is that space weather associated spatiotemporal fluctuations of the geomagnetic field follow the statistics of intermittency-induced criticality. Data will be used from arrays of ground-based magnetometers from high-to-equatorial latitudes.
This award reflects NSF's statutory mission and has been deemed worthy of support through evaluation using the Foundation's intellectual merit and broader impacts review criteria.
PUBLICATIONS PRODUCED AS A RESULT OF THIS RESEARCH
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