2 papers
astro-ph.SR2025
Quantifying how Surface Complexity Influences Properties of the Solar Corona and Solar Wind
Caroline L. Evans, Cooper Downs, Donald Schmit
The Sun's magnetic field is a key driver in coronal heating and consequently solar wind acceleration. Remote measurement of the photosphere provides the magnetic surface boundary c…
astro-ph.SR2024
Identifying Spicules in Mg II: Statistics and Comparisons with Hα
Vicki L. Herde, Souvik Bose, Phillip C. Chamberlin +4
The Sun's chromosphere is a critical region to understand when considering energy and mass deposition into the transition region and corona, but many of the smaller, faster events…