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Multi-spectral characterization of solar gamma ray events radio emission. Study case July 14, 2000.

Published online by Cambridge University Press:  14 March 2005

R.E. Rodriguez Taboada  and
A.L. Mendez Berhondo
R.E. Rodriguez Taboada
Affiliation:
Institute of Geophysics and Astronomy, Calle 212 No 2906, La Coronela, C. Habana, Cuba CP 11600 e-mail: ramone@infomed.sld.cu
A.L. Mendez Berhondo
Affiliation:
Institute of Geophysics and Astronomy, Calle 212 No 2906, La Coronela, C. Habana, Cuba CP 11600 e-mail: ramone@infomed.sld.cu
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Abstract

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Solar sporadic radio emission takes place in a wide range of time scales; from milliseconds to days. Researches have been conduced mainly to explain the behavior of radio emission in specific time scales and lately to millisecond spikes research has been devoted a lot of papers.

In this work we pay attention to the characteristics of millisecond spikes in relation to the general activity in which they are included, processes with very different time scales.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS223 , June 2004 , pp. 663 - 664
Copyright
© 2004 International Astronomical Union