Magnetic Sources of Solar Activity
This program studies how the Sun's magnetic fields shape the corona and drive solar activity, using observations and models.
This grant is no longer accepting proposals
NRC Research Associateship Programs has archived this opportunity.
Funder: NRC Research Associateship Programs
Due Dates: May 1, 2025 (Naval Research Laboratory opportunity)
Funding Amounts: $99,200 stipend plus $3,000 travel allowance; typical fellowship duration 2-3 years
Summary: Fellowship supporting postdoctoral research on the Sun’s magnetic fields and their influence on solar corona structure and dynamics using observations and numerical models.
Key Information: Open to U.S. citizens and permanent residents; requires Ph.D. earned within 5 years; relocation and health insurance benefits included.
Description
This fellowship opportunity at the Naval Research Laboratory (NRL) focuses on investigating the Sun’s magnetic field and its critical role in solar phenomena such as coronal mass ejections and solar flares. The research aims to explore the connection between solar magnetic fields and the structure and dynamics of the solar corona by combining high-resolution solar observations with numerical modeling. Observational data from space missions including Hinode, Solar Dynamics Observatory (SDO), and STEREO are extensively used.
The program is designed for postdoctoral researchers to conduct self-directed, innovative research that advances understanding of solar magnetic activity and its effects on the solar atmosphere. The outcomes are expected to contribute to the broader field of solar physics, ultraviolet and X-ray astronomy, and numerical analysis of solar phenomena.
