2 papers
astro-ph.SR2025
Structure and dynamics of the internetwork solar chromosphere: results of a small-scale dynamo simulation
D. Przybylski, R. Cameron, S. K. Solanki +3
The heating and structure of the solar chromosphere depends on the underlying magnetic field, among other parameters. The lowest magnetic flux of the solar atmosphere is found in t…
astro-ph.SR2024
Low-latitude magnetic flux emergence on rapidly rotating solar-type stars
Emre IÅık, Sami K. Solanki, Robert H. Cameron +1
Besides a dense coverage of their high latitudes by starspots, rapidly rotating cool stars also display low-latitude spots in Doppler images, although generally with a lower covera…