NSF
AGS-PRF: Ground-Based Radio and Space-Based White-Light Observations to Study the Structure of the Solar Corona
AGS-PRF: Ground-Based Radio and Space-Based White-Light Observations to Study the Structure of the Solar Corona is a funding opportunity from NSF, closing September 30, 2028.
Sep 30, 2028
(793d left)Overview
The solar corona – the Sun’s outermost atmosphere – continuously expands into space as the solar wind. Fundamental questions about the physical conditions and processes in corona and solar wind remain open, including how the corona gets so hot. Resolving this particular question requires understanding the…