Magnetohydrodynamic Evolution of Solar Flares
This project studies how magnetic fields evolve during solar flares, releasing energy and changing plasma, using simulations, observations, and modeling.
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 (Next deadline)
Funding Amounts: Stipend approximately $99,200 per year plus $3,000 travel allowance; typical fellowship duration 2-3 years.
Summary: Supports postdoctoral research on the magnetohydrodynamic evolution of solar flares, focusing on magnetic reconnection, plasma dynamics, and radiative processes using simulations, observations, and modeling.
Key Information: Open to U.S. citizens and permanent residents; requires Ph.D. earned within last 5 years; relocation and health insurance benefits included.
Description
This fellowship opportunity at the Naval Research Laboratory (NRL) focuses on the fundamental astrophysical process of magnetic reconnection that drives solar flares. Solar flares result from the release of magnetic energy and changes in the topology of magnetic fields, which in turn affect the plasma's magnetohydrodynamic and radiative behavior. The research aims to understand the complex interplay between magnetic field evolution, plasma hydrodynamics, and radiative output during flares.
Key aspects of the research include examining the roles of accelerated particles, magnetohydrodynamic waves, turbulence, and direct plasma heating. The approach combines advanced simulations, observational data, and forward modeling techniques to provide a comprehensive understanding of solar flare dynamics.
This project is ideal for postdoctoral researchers interested in space science, astrophysics, plasma physics, and computational modeling of solar phenomena.
