Implications of modern observations on solar flare theory
We present, in general, the solar flare phenomenon going through several aspects: a brief historical survey of solar flare observations, a general description of its observed characteristics and, finally, an account of the basic requirements set on solar flare models by the observational data. As a...
Guardado en:
| Autores principales: | , |
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| Formato: | Articulo Comunicacion |
| Lenguaje: | Español |
| Publicado: |
1989
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/147142 |
| Aporte de: |
| Sumario: | We present, in general, the solar flare phenomenon going through several aspects: a brief historical survey of solar flare observations, a general description of its observed characteristics and, finally, an account of the basic requirements set on solar flare models by the observational data. As a second step, we summarize some of our recent results on the observed character of energy release in a vast energetic and spatial range of events: flares, microflares and large scale brightening. The base of our analysis is the unique set of data provided by the Hard X-ray Imaging Spectrometer, that flew aboard Solar Maximum Mission satellite, and ground-based vector magnetograms from the Marshall Space Flight Center. |
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