Constraining solar emission radius at 42 MHz during the 2024 total solar eclipse using a student-commissioned radio telescope

Olivia R. Young, Timothy E. Dolch, Joseph F. Helmboldt +20

Low-frequency solar radio emission is sourced in the solar corona, with sub-100 MHz radio emission largely originating from the $\sim$10${}^5$\,$\mathrm{K}$ plasma around 2 optical…