This National Science Foundation (NSF) Geosciences Program (CFDA 47.050) Project Grant award of $578,828 to Predictive Science Incorporated, doing business as Predictive Science Inc., will support research to better understand the dynamic connection between the solar corona and the inner heliosphere. The project, titled "SHINE: How Does Surface Flux Evolution Determine the Structure and Dynamics of the Solar Corona and Inner Heliosphere?", aims to study how the continuous evolution...
This Project Grant award from the National Science Foundation's Geosciences Program (CFDA 47.050) will support a $582,399 research project by the Southwest Research Institute (SwRI) to investigate the origins of "active longitudes" on the Sun's surface and their connection to the solar dynamo and coronal mass ejections. The 3-year project will utilize 3D magnetohydrodynamic simulations and 17 years of observational data from the National Solar Observatory's Global Oscillation Network...
This $385,959 Project Grant award from the National Science Foundation's Geosciences Program (CFDA 47.050) supports a collaborative research effort to improve understanding of the Sun's corona, the outermost layer of the solar atmosphere. The project aims to analyze data from five total solar eclipses spanning 2015-2024 and compare this observational data to advanced magnetohydrodynamic simulations. Key activities include measuring coronal electron temperature, density, and magnetic field...
This Project Grant from the National Science Foundation Division of Atmospheric and Geospace Sciences, under the Geosciences federal grant program (CFDA 47.050), provides $107,634 to the Planetary Science Institute for research entitled "Collaborative Research: SHINE--Using Photospheric Imprints of Coronal Currents to Understand Coronal Magnetic Structure." The research aims to advance understanding of coronal currents and magnetic structure through modeling and analysis of coronal...
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 Project Grant award from the National Science Foundation's Geosciences Program (CFDA 47.050) provides $182,730.00 to Predictive Science Incorporated to analyze data from five total solar eclipses between 2015 and 2024 and compare it to advanced magnetohydrodynamic simulations. The goal is to improve understanding of the Sun's corona, the hot outer layer of the solar atmosphere, including tracking changes over the solar cycle and refining models of the Sun's atmosphere. This research will...
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...
This National Science Foundation (NSF) Geosciences Program (CFDA 47.050) grant award provides $593,864 to the New Jersey Institute of Technology (NJIT) from September 2024 to August 2027. The project will develop an AI-driven framework called SolarDM to generate high-resolution, high-cadence vector magnetograms of the solar chromosphere and photosphere. These AI-generated products will provide valuable data on the Sun's magnetic field to significantly advance the understanding and prediction...
This National Science Foundation Project Grant of $388,769 awarded under the Geosciences program (CFDA 47.050) supports multi-wavelength spectroscopic and spectropolarimetric diagnostics of the solar atmosphere from April 2021 through March 2024. The University Corporation will utilize observations from the Dunn Solar Telescope and SDO/HMI to develop new non-force-free magnetic field extrapolation codes. These codes will estimate magnetic field line heights and strengths surrounding sunspots....
This $568,185 Project Grant awarded by the National Science Foundation's Geosciences Program (CFDA 47.050) will support research to study the origin and evolution of jets emanating from coronal holes on the Sun. The project, titled "SHINE: Statistical Birth Conditions of Coronal Hole Jets Using the Legacy Dunn Solar Telescope," will use measurements from the Dunn Solar Telescope in New Mexico and other observatories to trace the properties of these jets across different atmospheric...