Project Grant 2147399
- Federal Project Grant Award Summary The National Science Foundation's Division of Atmospheric and Geospace Sciences awarded a $509,494 Project Grant to the University of California, Berkeley on February 15, 2026, to advance understanding of solar energetic particle formation and transport through multi-point spacecraft observations. The research will deliver scientific analysis and datasets examining sunward-streaming energetic particles across one complete solar cycle, utilizing existing...
- This three-year Project Grant from the National Science Foundation Division of Atmospheric and Geospace Sciences, under the Geosciences federal grant program (CFDA 47.050), provides $144,535 to the University of Wisconsin System to conduct collaborative research on coronal magnetic structure and solar flares/coronal mass ejections. The research team will employ Gauss's separation method and nonlinear force-free field extrapolations to analyze photospheric vector magnetograms of solar active...
- This Project Grant from the National Science Foundation Division of Atmospheric and Geospace Sciences, totaling $357,172, supports research into small-scale ejections in the sun's photosphere through chromosphere and corona from September 1, 2021 through August 31, 2024. The award is being administered by the New Jersey Institute of Technology under the Geosciences program (CFDA 47.050) to strengthen understanding of the integrated Earth system through basic atmospheric and ocean sciences...
- This $283,079 Project Grant award from the National Science Foundation (NSF) Mathematical and Physical Sciences (CFDA 47.049) program supports observational investigations of ion heating by magnetic reconnection in the Earth's magnetotail. The research project, led by the University of California, Berkeley, aims to study hundreds of reconnection events using in-situ spacecraft observations to determine the factors controlling the degree of plasma heating. The results are expected to enhance...
- This $300,519 National Science Foundation project grant supports research and outreach activities to study the parametric decay instability mechanism's potential role in solar corona heating. Funded under the Geosciences program, which supports basic research to improve understanding of Earth's integrated systems, the two-year award to New Mexico Consortium will analyze observational data and conduct numerical simulations. Postdoctoral researchers and undergraduate students at Columbia...
- The National Science Foundation awarded a $280,817 Project Grant to the University of Colorado Boulder under the Geosciences federal grant program (CFDA 47.050) from May 15, 2023 to April 30, 2026. The grant supports research to advance understanding of coronal heating and solar wind acceleration processes through multi-messenger data analysis and four-dimensional forward modeling simulations. Specifically, the University will construct line-of-sight models of extreme ultraviolet and X-ray...
- This three-year Project Grant from the National Science Foundation's Division of Atmospheric and Geospace Sciences Geosciences program (CFDA 47.050) provides $150,000 to the New Jersey Institute of Technology to advance understanding of coronal heating mechanisms in the Sun. Through a combination of multi-wavelength microwave imaging observations from the Extended Owens Valley Solar Array and 3D numerical simulations, the grantee will examine the coupling of thermal and magnetic structures...
- This $554,951 Project Grant was awarded by the National Science Foundation's (NSF) Division of Atmospheric and Geospace Sciences under the Geosciences program (CFDA 47.050). The grant supports research by the University of Maryland, College Park to investigate energy conversion processes associated with non-equilibrium plasma velocity distribution functions during dayside magnetic reconnection at the Earth's magnetopause. The research aims to understand when, where, and how energy conversion...
- This National Science Foundation Project Grant of $508,504 provides funding from November 1, 2022 to October 31, 2025 under the Geosciences program (CFDA 47.050) to advance understanding of coronal mass ejections (CMEs) from the Sun. Led by underrepresented groups in STEM, the award supports physics-based and statistical studies to quantify the structure and evolution of magnetic flux ropes from the solar photosphere to the inner heliosphere. Researchers will characterize CME flux ropes using...
- This $305,598 Project Grant from the National Science Foundation Division of Astronomical Sciences, under the Mathematical and Physical Sciences program (CFDA 47.049), will fund collaborative research between the New Jersey Institute of Technology and the University of Alabama, Huntsville to study solar flare-producing active regions. The researchers will leverage high-resolution observations from the Daniel K. Inouye Solar Telescope and other ground-based and space-based telescopes, along...
This Project Grant from the National Science Foundation Division of Atmospheric and Geospace Sciences, under the Geosciences federal grant program (CFDA 47.050), provides $620,904 to support numerical modeling of reconnection-generated transients in the solar corona. The Regents of the University of California, doing business as the University of California, Berkeley, will utilize the funding from March 15, 2022 through February 28, 2025 to conduct a comprehensive, multidisciplinary investigation into the multi-scale nature of solar eruptive structures. Specifically, the University will determine how solar and heliospheric magnetic flux rope properties vary across spatial and energy scales, and how coronal source region topologies influence eruption formation mechanisms and resulting magnetic structures. It will also examine similarities and differences between various populations of flux rope transients, and how each interacts with overlying flux systems and the ambient solar wind outflow. The University will address the objectives through state-of-the-art high-performance numerical modeling and analysis of multi-spacecraft observations. Results will be disseminated at scientific meetings and in peer-reviewed publications.
Mod # | Description | ReasonForModification | Federal Obligation | Date |
|---|---|---|---|---|
| Not listed | $620.9k | 3/10/22 |