This three-year project grant from the National Science Foundation's Division of Atmospheric and Geospace Sciences, under the Geosciences program (CFDA 47.050), provides $134,443 to support collaborative research titled "SHINE: Where are Particles Accelerated in Coronal Jets?". The research aims to enhance understanding of how energy is produced by the Sun and accelerated in interplanetary space by investigating where electrons are accelerated in coronal jets originating near solar active regions. The grantee, New Jersey Institute of Technology, will analyze observations of coronal jet events from multiple space- and ground-based observatories, including the Expanded Owens Valley Solar Array. Numerical simulations will then be conducted using the analyzed data to reveal where electron energization occurs within jets, how particle spectra evolve, and how energetic particles escape. Graduate and undergraduate researchers will also be supported. The results are intended to provide insight into the source regions of impulsive solar energetic particles and their escape into the heliosphere, supporting space weather forecasting efforts.
Mod # | Description | Reason For Modification | Federal Obligation (Click to sort descending) | Date (Click to sort ascending) |
|---|---|---|---|---|
| Not listed | $134.4k | 7/26/22 |