Opportunity Information: Apply for PD 04 4202

  • The National Science Foundation in the science and technology and other research and development sector is offering a public funding opportunity titled "Geospace Facilities" and is now available to receive applicants.
  • Interested and eligible applicants and submit their applications by referencing the CFDA number(s): 47.050 Geosciences.
  • This funding opportunity was created on Mar 13, 2015 and posted on Mar 13, 2015.
  • Applicants must submit their applications by Proposals accepted anytime. (Agency may still review applications by suitable applicants for the remaining/unused allocated funding in 2026.)
  • Eligible applicants include: Unrestricted (i.e., open to any type of entity above), subject to any clarification in text field entitled Additional Information on Eligibility.
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Opportunity Summary:

The National Science Foundation (NSF) Geospace Facilities (GF) grant opportunity (Funding Opportunity Number PD 04 4202) supports research that uses NSF-funded radar and related observational infrastructure to study the Earth s upper atmosphere. The central aim of the program is to advance basic science on the structure, behavior, and dynamics of the geospace environment, particularly the ionosphere and upper atmospheric regions that are strongly influenced by energy and particle inputs from the Sun and by coupling to the magnetosphere. Projects funded under GF typically rely on observations made with major community facilities rather than building new large instruments, and they are expected to produce fundamental understanding of upper-atmospheric processes rather than primarily applied or operational outcomes.

A key part of the opportunity is access to four large incoherent scatter radar (ISR) facilities supported by NSF. These radars are arranged along a longitudinal chain extending from Greenland to Peru, which is scientifically valuable because it enables coordinated measurements across a wide range of latitudes and geophysical conditions, from high-latitude auroral regions through mid-latitudes and into equatorial ionospheric regimes. Incoherent scatter radars are powerful tools for directly measuring ionospheric parameters such as electron density, ion and electron temperatures, plasma drifts, and related quantities that describe how the upper atmosphere responds to solar forcing, geomagnetic activity, and lower-atmosphere influences. Each of these ISR facilities is also equipped with strong optical diagnostic instruments, which can include systems that observe airglow and auroral emissions. Those optical measurements complement radar data by providing additional information about composition, energy deposition, and spatial structure, and they often make it possible to interpret radar-derived plasma parameters in a broader physical context.

The opportunity also highlights NSF support for the Super Dual Auroral Radar Network (SuperDARN), a distributed system of coherent scatter high-frequency (HF) radars located across both the northern and southern hemispheres. SuperDARN radars are particularly useful for mapping large-scale plasma convection and electric fields in the high-latitude ionosphere over broad geographic areas. Because it is a network rather than a single site, SuperDARN enables synoptic views of geospace dynamics, supporting studies of magnetosphere ionosphere coupling, storm and substorm evolution, and the global response of the ionosphere to solar wind driving. Research that combines SuperDARN observations with incoherent scatter radar and optical data is often especially compelling because it can connect detailed local measurements to global-scale dynamics.

NSF positions Geospace Facilities research as strongly linked to the Aeronomy Program and the Magnetospheric Physics Program. In practice, that means proposals commonly address questions at the intersection of upper-atmosphere chemistry and dynamics (aeronomy) and the physics of the near-Earth space environment shaped by the magnetic field and solar wind (magnetospheric physics). Typical science themes can include energy and momentum transfer between the magnetosphere and ionosphere, ionospheric electrodynamics and plasma instabilities, auroral processes, thermosphere ionosphere coupling, and the ways in which geomagnetic storms reshape density, temperature, and circulation patterns in the upper atmosphere. The program emphasis is on basic research, so proposals are generally expected to articulate clear hypotheses or research questions, a plan for using facility data effectively, and how the results will advance fundamental understanding.

Administratively, this is a discretionary NSF grant opportunity in the science and technology and other research and development category, listed under CFDA 47.050 (Geosciences). There is no cost sharing or matching requirement. The opportunity is open to an unrestricted pool of applicants, meaning it is broadly available to eligible entities, subject to any specific eligibility clarifications that may appear in the full program description. Proposals are accepted at any time, which indicates an ongoing solicitation rather than a single annual deadline, though applicants still need to follow NSF proposal preparation and submission rules and should pay attention to any internal review cycles or target dates described in the linked NSF program description.

For applicant support, the announcement indicates that technical issues accessing the full announcement through Grants.gov should be directed to NSF Grants.gov support at grantsgovsupport@nsf.gov. The opportunity also references an additional information link to the NSF program description for PD 04 4202, which is typically where details such as proposal types, review considerations, facility access expectations, and any special submission instructions are provided.

Frequently Asked Questions (FAQs): NSF Geospace Facilities (GF) - PD 04 4202

What is the NSF Geospace Facilities (GF) grant opportunity (PD 04 4202)?

The NSF Geospace Facilities (GF) grant opportunity (Funding Opportunity Number PD 04 4202) supports research that uses NSF-funded radar and related observational infrastructure to study the Earths upper atmosphere. The program aims to advance basic science on the structure, behavior, and dynamics of the geospace environment, with particular focus on the ionosphere and upper atmospheric regions influenced by energy and particle inputs from the Sun and by coupling to the magnetosphere.

What is the central scientific aim of this opportunity?

The central aim is to produce fundamental understanding of upper-atmospheric processes, especially how the ionosphere and nearby regions respond to solar forcing, geomagnetic activity, and coupling processes involving the magnetosphere. The emphasis is on basic research rather than primarily applied or operational outcomes.

What kinds of research does the program typically fund?

Projects funded under GF typically rely on observations made with major community facilities supported by NSF. Rather than building new large instruments, proposals are expected to use existing radar and related observational infrastructure to address clear hypotheses or research questions and advance fundamental knowledge of geospace and upper-atmospheric physics.

Does this program focus on building new instruments or using existing facilities?

The program is described as typically supporting research that uses major community facilities rather than building new large instruments. The expectation is that the work will leverage NSF-supported observational capabilities to generate new scientific insight.

Which major radar facilities are highlighted for this opportunity?

The opportunity highlights access to four large incoherent scatter radar (ISR) facilities supported by NSF. These radars form a longitudinal chain extending from Greenland to Peru, enabling coordinated measurements across a wide range of latitudes and geophysical conditions.

Why is the Greenland-to-Peru longitudinal radar chain scientifically valuable?

Because it spans from high-latitude auroral regions through mid-latitudes and into equatorial ionospheric regimes, the chain enables coordinated measurements across diverse geophysical environments. This makes it possible to study how processes vary with latitude and how different regions of the ionosphere respond under different conditions.

What is an incoherent scatter radar (ISR) used for in geospace research?

Incoherent scatter radars are used to directly measure ionospheric parameters. The opportunity notes that ISRs can measure electron density, ion and electron temperatures, plasma drifts, and related quantities that describe how the upper atmosphere responds to solar forcing, geomagnetic activity, and influences from the lower atmosphere.

What types of measurements can ISR facilities provide?

Based on the opportunity description, ISR measurements can include electron density, ion temperature, electron temperature, plasma drifts, and other related parameters used to characterize the state and dynamics of the ionosphere.

Are optical instruments part of the supported facilities?

Yes. Each ISR facility is described as being equipped with strong optical diagnostic instruments. These may include systems that observe airglow and auroral emissions, and they are used to complement radar observations.

How do optical observations complement radar data in this program?

Optical measurements provide additional information about composition, energy deposition, and spatial structure. The opportunity notes that these measurements often help interpret radar-derived plasma parameters in a broader physical context.

What is SuperDARN and how does it relate to this opportunity?

SuperDARN (the Super Dual Auroral Radar Network) is a distributed system of coherent scatter high-frequency (HF) radars located across both the northern and southern hemispheres, supported by NSF. It is highlighted as part of the observational infrastructure relevant to Geospace Facilities research.

What kinds of science can SuperDARN enable?

SuperDARN radars are described as useful for mapping large-scale plasma convection and electric fields in the high-latitude ionosphere over broad geographic areas. Because it is a network, it enables synoptic views of geospace dynamics and supports studies of magnetosphere-ionosphere coupling, storm and substorm evolution, and the global response of the ionosphere to solar wind driving.

Is combining SuperDARN with ISR and optical data encouraged?

The opportunity indicates that research combining SuperDARN observations with incoherent scatter radar and optical data is often especially compelling because it can connect detailed local measurements to global-scale dynamics.

How is Geospace Facilities research positioned within NSF programs?

NSF positions Geospace Facilities research as strongly linked to the Aeronomy Program and the Magnetospheric Physics Program. This reflects the common overlap between upper-atmosphere chemistry and dynamics (aeronomy) and the physics of the near-Earth space environment shaped by the magnetic field and solar wind (magnetospheric physics).

What are examples of typical science themes for GF proposals?

The opportunity lists example themes including energy and momentum transfer between the magnetosphere and ionosphere, ionospheric electrodynamics and plasma instabilities, auroral processes, thermosphere-ionosphere coupling, and how geomagnetic storms reshape density, temperature, and circulation patterns in the upper atmosphere.

Is this opportunity mainly for basic research or applied/operational work?

The program emphasis is on basic research. The opportunity states that projects are expected to produce fundamental understanding of upper-atmospheric processes rather than primarily applied or operational outcomes.

What does the program expect a strong proposal to include?

The opportunity indicates that proposals are generally expected to articulate clear hypotheses or research questions, describe a plan for using facility data effectively, and explain how the results will advance fundamental understanding.

What is the funding mechanism and category for this opportunity?

Administratively, the opportunity is described as a discretionary NSF grant opportunity in the science and technology and other research and development category.

What CFDA number is associated with this NSF opportunity?

The opportunity is listed under CFDA 47.050 (Geosciences).

Is cost sharing or matching required?

No. The announcement states there is no cost sharing or matching requirement.

Who is eligible to apply?

The opportunity is described as open to an unrestricted pool of applicants, meaning it is broadly available to eligible entities. The announcement also notes that applicants should review the full program description for any specific eligibility clarifications.

When are proposals due?

Proposals are accepted at any time, indicating an ongoing solicitation rather than a single annual deadline. Applicants are still expected to follow NSF proposal preparation and submission rules and to pay attention to any internal review cycles or target dates described in the NSF program description.

Where can applicants find additional submission details or special instructions?

The opportunity references an additional information link to the NSF program description for PD 04 4202. That program description is indicated as the place where details such as proposal types, review considerations, facility access expectations, and any special submission instructions are typically provided.

What should applicants do if they have technical issues accessing the opportunity on Grants.gov?

The announcement directs technical issues accessing the full announcement through Grants.gov to NSF Grants.gov support at grantsgovsupport@nsf.gov.

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