FUNDING > Magnetospheric Physics
Division of Atmospheric and Geospace Sciences
JKOZYRA@nsf.gov, (703) 292-8519
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/publications/pub_summ.jsp?ods_key=grantsgovguide)
Important Information for Proposers
A revised version of the NSF Proposal & Award Policies & Procedures Guide (PAPPG) (NSF 16-1), is effective for proposals submitted, or due, on or after January 25, 2016. Please be advised that, depending on the specified due date, the guidelines contained in NSF 16-1 may apply to proposals submitted in response to this funding opportunity.
Full Proposal Accepted Anytime
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.
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.
Atmospheric and Geospace Sciences Postdoctoral Research Fellowships
Geospace Environment Modeling
Research in Support of the National Space Weather Program
Solar, Heliospheric, and INterplanetary Environment
This Program is Part of