A&A 403, 277-285 (2003)
DOI: 10.1051/0004-6361:20030237
La Palma observations of umbral flashes
L. H. M. Rouppe van der Voort1, R. J. Rutten2, 3, P. Sütterlin2, P. J. Sloover2 and J. M. Krijger21 The Institute for Solar Physics of the Royal Swedish Academy of Sciences, AlbaNova University Center, 10691 Stockholm, Sweden
2 Sterrekundig Instituut, Utrecht University, Postbus 80 000, 3508 TA Utrecht, The Netherlands
e-mail: R.J.Rutten,P.Suetterlin,P.J.Sloover,J.M.Krijger@astro.uu.nl
3 Institute of Theoretical Astrophysics, Oslo University, PO Box 1029 Blindern, 0315 Oslo, Norway
(Received 23 December 2002 / Accepted 13 February 2003)
Abstract
We present high-quality Ca II H & K data showing
chromospheric flashes in sunspot umbrae collected with the Swedish
Vacuum Solar Telescope, the Dutch Open Telescope, and the Swedish
1-m Solar Telescope at the Roque de los Muchachos Observatory on La
Palma. Differential movies, time slices, spectrograms, and Fourier
power maps demonstrate that umbral flashes and running penumbral
waves are closely related oscillatory phenomena, combining upward
shock propagation with coherent wave spreading over the entire
spot. We attribute the flash brightening to large redshift by
post-shock material higher up. We find no obvious relation between
umbral dots and umbral flashes.
Key words: Sun: sunspots -- Sun: oscillations
Offprint request: L. Rouppe van der Voort, rouppe@astro.su.se
© ESO 2003

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