Solar microwave bursts in milliseconds - Observations from Mexico City

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Published: Jan 1, 1992
DOI: https://doi.org/10.22201/igeof.00167169p.1992.31.1.1300
Keywords:
Solar radioastronomy, Radio bursts, Flares, Millisecond spikes

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M. Lanzagorta
Universidad Nacional Autónoma de México, Instituto de Geofísica, Departamento de Física Espacial, Ciudad Universitaria, Alcaldía Coyoacán 04510, México CDMX, México
S. Bravo
Universidad Nacional Autónoma de México, Instituto de Geofísica, Departamento de Física Espacial, Ciudad Universitaria, Alcaldía Coyoacán 04510, México CDMX, México

Abstract

Millisecond scale radio spikes associated with nonthermal coherent emission are closely related to particle acceleration and energy release in flares. In this paper we describe the various characteristics of these phenomena as well as their relation to other solar emissions. We also outline a theoretical framework of the spike emission process and some efforts made in Mexico City to observe solar microwave bursts at 4 cm wavelength with a time resolution of milliseconds.

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How to Cite
Lanzagorta, M., & Bravo, S. (1992). Solar microwave bursts in milliseconds - Observations from Mexico City. Geofisica Internacional, 31(1), 51–57. https://doi.org/10.22201/igeof.00167169p.1992.31.1.1300
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Vol. 31 No. 1 (1992): January 1, 1992
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This work is licensed under a Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International License.

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