The Intensity Distribution in Sunspot Penumbras

Bibcode
1987rfsm.conf..214C
Collados, M.; del Toro Iniesta, J. C.; Vázquez, M.
Referencia bibliográfica

The Role of Fine-Scale Magnetic Fields on the Structure of the Solar Atmosphere, Proceedings of the Inaugural workshop and round table discussion for the D-E-S Telescope installations on the Canary Islands, La Laguna, Tenerife, Spain, 6-12 October 1986. Edited by E.-H. Schröter, M. Vázquez, and A.A. Wyller. Cambridge: Cambridge University Press, 1987., p.214

Fecha de publicación:
0
1987
Número de autores
3
Número de autores del IAC
0
Número de citas
1
Número de citas referidas
0
Descripción
The intensity distribution of the penumbra at different stages of evolution has been analyzed. The results have been different for both evolved and primitive penumbras. While the former present almost symmetrical, single-peaked histograms, the same does not occur for the latter, their distributions being, preferentially, asymmetrical or double-peaked. These results are interpreted in terms of bright and dark elements. Thus, an evolutionary process has been proposed to explain the diverse characteristics found at the different stages.
Tipo
Sin árbitro

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