110 citations · 154 across the 3 of their papers we have counts for
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astro-ph2008★ 110 cited
Coupling from the photosphere to the chromosphere and the corona
S. Wedemeyer-Böhm, A. Lagg, Å. Nordlund
The atmosphere of the Sun is characterized by a complex interplay of competing physical processes: convection, radiation, conduction, and magnetic fields. The most obvious imprint…
astro-ph2008★ 36 cited
How to use magnetic field information for coronal loop identification?
T. Wiegelmann, B. Inhester, A. Lagg +1
The structure of the solar corona is dominated by the magnetic field because the magnetic pressure is about four orders of magnitude higher than the plasma pressure. Due to the hig…