7 citations · 7 across the 1 of their papers we have counts for
3 papers
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…
Low-latitude magnetic flux emergence on rapidly rotating solar-type stars
Emre Işık, 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…
Small-scale Dynamo in Cool Stars III. Changes in the photospheres of F3V to M0V stars
Tanayveer S. Bhatia, Robert H. Cameron, Hardi Peter +1
Some of the quiet solar magnetic flux could be attributed to a small-scale dynamo (SSD) operating in the convection zone. An SSD operating in cool main-sequence stars is expected t…