Division of Atmospheric Sciences
Magnetospheric Physics
CONTACTS
PROGRAM GUIDELINES
Apply to PD 98-5750 as follows:
For full proposals submitted via FastLane:
standard Grant Proposal Guidelines apply.
For full proposals submitted via Grants.gov:
NSF Grants.gov Application Guide; A Guide for the Preparation and Submission of NSF Applications via Grants.gov Guidelines apply
(Note: The NSF Grants.gov Application Guide is available on the Grants.gov website and on the NSF website at:
http://www.nsf.gov/bfa/dias/policy/docs/grantsgovguide.pdf)
DUE DATES
Full Proposal Accepted Anytime
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There are no deadlines or target dates for proposals sent in to any of the UARS base programs. However, we recommend that PIs try to send in proposals early in the fiscal year.
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SYNOPSIS
Supports research on the magnetized plasma envelope of the outer atmosphere, including energization by the solar wind; the origin of geomagnetic storms and substorms; the population by solar and ionospheric sources; the origin of electric fields; the coupling among the magnetosphere, ionosphere, and atmosphere; and waves and instabilities in the natural plasma. Also supported are ground-based observational programs at high latitudes and laboratory experiments applicable to the geospace environment. Theoretical research programs may include numerical simulations using a variety of MHD, hybrid and particle codes. The analysis of data from all sources, whether ground-based or from spacecraft, is also supported.
RELATED PROGRAMS
CEDAR, GEM, and SHINE Postdoctoral Research
Geospace Environment Modeling
Research in Support of the National Space Weather Program
Solar, Heliospheric, and INterplanetary Environment
THIS PROGRAM IS PART OF
Upper Atmosphere Research Section
Abstracts of Recent Awards Made Through This Program
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