This grant is for the purpose of supporting fundamental and applied research into the complex processes of energy generation, transport, and ultimate deposition from the Sun into the terrestrial environment. Key areas of investigation include understanding space weather impacts, solar internal dynamics such as helioseismology and the solar dynamo, and the solar activity cycle. It also covers magnetic flux emergence, solar flares, eruptive activity like coronal mass ejections, and the heating mechanisms of the solar wind. Furthermore, the grant supports studies on solar energetic particles, their interactions with cosmic rays, and critical boundary problems at the solar wind/magnetosphere interface, aiming to advance our comprehension of the Sun-Earth system.
Opportunity ID: 359307
General Information
| Document Type: | Grants Notice |
| Funding Opportunity Number: | PD-98-1523 |
| Funding Opportunity Title: | Solar Terrestrial |
| Opportunity Category: | Discretionary |
| Opportunity Category Explanation: | – |
| Funding Instrument Type: | Grant |
| Category of Funding Activity: | Science and Technology and other Research and Development |
| Category Explanation: | – |
| Expected Number of Awards: | – |
| Assistance Listings: | 47.050 — Geosciences |
| Cost Sharing or Matching Requirement: | No |
| Version: | Synopsis 1 |
| Posted Date: | Jun 06, 2025 |
| Last Updated Date: | Jun 06, 2025 |
| Original Closing Date for Applications: | – Proposals accepted anytime |
| Current Closing Date for Applications: | – Proposals accepted anytime |
| Archive Date: | Jun 07, 2025 |
| Estimated Total Program Funding: | – |
| Award Ceiling: | – |
| Award Floor: | – |
Eligibility
| Eligible Applicants: | Unrestricted (i.e., open to any type of entity above), subject to any clarification in text field entitled “Additional Information on Eligibility” |
| Additional Information on Eligibility: | – |
Additional Information
| Agency Name: | U.S. National Science Foundation |
| Description: | Supports research on the processes by which energy in diverse forms is generated by the Sun, transported to the Earth, and ultimately deposited in the terrestrial environment. Major topics include space weather impacts, helioseismology, the solar dynamo, the solar activity cycle, magnetic flux emergence, solar flares and eruptive activity, coronal mass ejections, solar wind heating, solar energetic particles, interactions with cosmic rays, and solar wind/magnetosphere boundary problems. |
| Link to Additional Information: | NSF Program Desccription PD-98-1523 |
| Grantor Contact Information: | If you have difficulty accessing the full announcement electronically, please contact:
NSF grants.gov support
grantsgovsupport@nsf.gov Email:grantsgovsupport@nsf.gov |
Version History
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