Geospace Cluster — U.S. National Science Foundation funding opportunity
U.S. National Science Foundation · Federal agency

Geospace Cluster

The Geospace Cluster (GC) in the Division of Atmospheric and Geospace Sciences (AGS) supports fundamental and solutions-oriented research, technology development and education related to the Earth's near-space environmen...

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Deadline Fixed Location Alabama Type grant Level Federal Open posted Sep 26, 2024
✦ AI Summary
  • Who can apply: Federal-level applicants (see eligibility for details).
  • Issued by: U.S. National Science Foundation.
  • About: The Geospace Cluster (GC) in the Division of Atmospheric and Geospace Sciences (AGS) supports fundamental and solutions-oriented research, technology development and education related to the Earth's near-space environment (including the…
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About this opportunity

The Geospace Cluster (GC) in the Division of Atmospheric and Geospace Sciences (AGS) supports fundamental and solutions-oriented research, technology development and education related to the Earth's near-space environment (including the and radiation belts) and the inner heliosphere and solar atmosphere. The GC advances knowledge of the Sun system, including how various parts of the system are coupled through dynamical, electrodynamical and chemical processes. The GC supports research on the societal impacts of these processes including space weather and upper atmosphere climate change, with the aim of increasing resilience to such natural hazards. The GC supports research that uses ground-based or space-based observational facilities and instruments as well as data centers and a broad range of analyses and laboratory activities. General research topics that are supported by the GC include, but are not limited to: Aeronomy, including studies of wave reaction, photo emission and transport of energy and momentum within and between the mesosphere, thermosphere and ionosphere of the Earth; how this global system is coupled to the stratosphere below and magnetosphere above; and the plasma physics of phenomena manifested in the coupled ionosphere-magnetosphere system. Magnetospheric physics, including studies of the magnetosphere, or the cavity carved out of the solar wind by the Earth's magnetic field, its energization by the solar wind and population by solar and ionospheric sources; waves and instabilities in such natural plasmas; the origin of planetary electric fields; the origin of geomagnetic storms and substorms; and the coupling among the radiation and atmosphere. Solar-terrestrial physics, including how energy generation and eruptive processes occur in the solar atmosphere and how energy and momentum are transported within the Sun-Earth system; solar dynamo, solar activity cycle and magnetic flux emergence; eruptive activity including solar flares and coronal mass ejections; solar wind heating, solar energetic particles and interactions with cosmic rays; solar wind/magnetosphere boundary; and helioseismology. Space weather and space climate, including solar or terrestrial drivers of space weather; observations and modeling of the integrative geospace system that could lead to better predictive capabilities of the time-varying space environment; and characterization of space weather impacts on critical infrastructure and technological systems. Proposals to the GC are welcome at any time. However, the following solicitations in support of specific geospace science and community efforts have target dates or deadlines. They also may have PI and/or Institution restrictions. Please refer to the solicitation documents for further details: The Dynamics of Atmospheric Regions (CEDAR) targeted research program aims to understand the behavior of the Earth's atmospheric regions from the middle atmosphere upward through the thermosphere and ionosphere into the exosphere in terms of and dynamics on regional and global scales. The Geospace Environment Modeling (GEM) targeted research program supports investigations of the physics of the Earth's magnetosphere and the coupling of the magnetosphere to the atmosphere and solar wind, including for making accurate predictions of the geospace environment. The Interplanetary Environment (SHINE) targeted research program supports enhanced understanding of and predictive capabilities for the processes by which energy in the form of magnetic fields and particles are produced by the Sun and/or accelerated in interplanetary space and on the mechanisms by which these fields and particles are transported to the Earth through the inner heliosphere.

Funding agency

U.S. National Science Foundation
Federal agency

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Who can apply

Eligibility details aren't on file yet — check the agency source link in the Documents tab for the latest rules.

Geographic eligibility

  • Alabama
  • Alaska
  • Arizona
  • Arkansas
  • California
  • Colorado
  • Connecticut
  • Delaware
  • Florida
  • Georgia
  • Hawaii
  • Idaho
  • Illinois
  • Indiana
  • Iowa
  • Kansas
  • Kentucky
  • Louisiana
  • Maine
  • Maryland
  • Massachusetts
  • Michigan
  • Minnesota
  • Mississippi
  • Missouri
  • Montana
  • Nebraska
  • Nevada
  • New Hampshire
  • New Jersey
  • New Mexico
  • New York
  • North Carolina
  • North Dakota
  • Ohio
  • Oklahoma
  • Oregon
  • Pennsylvania
  • Rhode Island
  • South Carolina
  • South Dakota
  • Tennessee
  • Texas
  • Utah
  • Vermont
  • Virginia
  • Washington
  • West Virginia
  • Wisconsin
  • Wyoming
  • District of Columbia

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Source documents

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Citation details

Source systemgrants.gov
Source ID356536
PostedSep 26, 2024

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