Estudio de la dinámica de una fulguración de clase M.
Abstract
In this work we analize the compact flare of May 9, 2012, at 12:21 UT using data in different wavelenghts, including images obtained with the H-Alpha Solar Telescope for Argentina (HASTA). We identify the brightenings, their location with respect to the photospheric magnetic field, and the presence of a surge after the flare impulsive phase. We interprete the observations and the presence of cold loops after the flare in terms of the location of the energy release site. We estimate the height and length of the loops through which the surge material flows. FULL TEXT IN SPANISH
- Publication:
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Boletin de la Asociacion Argentina de Astronomia La Plata Argentina
- Pub Date:
- 2012
- Bibcode:
- 2012BAAA...55..107L