8 citations · 21 across the 3 of their papers we have counts for
4 papers · 1 filter
The spatial structure of solar magnetoconvection at scales up to ~Mm
D. Przybylski, R. H. Cameron
While convective motions at the scale of granules on the solar surface are well understood, those of mesogranular and supergranulation are not. At still larger scales, the lack of…
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…