Abstract
We have calculated the spectrum of eigenmodes of umbral oscillations. The eigenmodes of oscillations with periods from several tens of minutes (g-modes) to several tens of seconds (p-modes) have been found. It is shown that the 3-min umbral oscillations are p-modes modified by the magnetic field.
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APA
Zhukov, V. I. (2002). Oscillations on the Sun in regions with a vertical magnetic field I. Sunspot umbral oscillations. Astronomy and Astrophysics, 386(2), 653–657. https://doi.org/10.1051/0004-6361:20020279
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