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\begin{document}

\title{sTUDY OF SOLAR rADIO SPIKES PROPERTIES OBSERVED AT FREQUENCIES 0.01-8.4
ghZ}



\author[1]{Gilberto A. Casillas-Perez}%
\author[2]{Solai Jeyakumar}%
\author[3]{Armando Carrillo-Vargas}%
\author[4]{Román Pérez-Enríquez}%
\affil[1]{Instituto de Geofísica, Universidad Nacional autónoma de México}%
\affil[2]{Departamento de Astronomía, Universidad de Guanajuato}%
\affil[3]{Instituto de Geofisica, Unidad Morelia, Universidad Nacional Autonoma de México}%
\affil[4]{Centro de Geociencias, Universidad Nacional Autónoma de México}%


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  \date{May 22, 2024}


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\begin{abstract}
Fast transients in the form of spiky radio bursts have been observed in
solar flares events, emitting at different ranges in frequency. These
dynamical phenomena show up as high brightness temperature increments
with short durations of the order of milliseconds. In this work, we
present results of the analysis of some properties of radio spike events
observed at frequencies between 0.01 and 8.4 GHz, as reported in
different studies. We analyze the relation of the duration, bandwidth,
emitted flux, polarization and drift rate of the radio spikes with its
observational frequency. Also, we analyze its correlation with other
energetic solar events.%
\end{abstract}%



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