First Solar Radio Burst Observations by the Mexican Array Radio Telescope (MEXART) at 140 MHz
E. Huipe-Domratcheva, V. De la Luz, G. A. Casillas-Perez, J. C., Mejia-Ambriz, E. Perez-Leon, J. A. Gonzalez-Esparza, C. Monstein, W. Reeve

TL;DR
This study demonstrates MEXART's capability to detect solar radio bursts at 140 MHz, identifying 75 events and analyzing their characteristics, with implications for space weather monitoring in Mexico.
Contribution
It is the first to show MEXART's effectiveness in solar radio burst detection and characterizes Type III burst evolution using wavelet analysis.
Findings
75 solar radio bursts identified, including 5 Type II and 70 Type III.
Three phases of Type III bursts characterized: pre-phase, main peak, decay, and post-event.
Wavelet analysis revealed a pine tree structure preceding Type III bursts.
Abstract
The National Laboratory of Space Weather in Mexico (Laboratorio Nacional de ClimaEspacial: LANCE) coordinates instrumentation for monitoring the space-weatherimpact over Mexico. Two of these instruments are the Mexican Array Radio Telescope(MEXART) and Compound Astronomical Low frequency Low cost Instrument for Spectroscopy and Transportable Observatory(CALLISTO) station from the e-CALLISTO network (CALLMEX). Both instruments are located at the same facility(Coeneo Michoacan, Mexico) and share a spectral band centered at 140 MHz. In this work we show the capabilities of the e-CALLISTO network as support to identify a solar radio burst in the signal of the MEXART radiotelescope. We identify 75 solarradio bursts in the MEXART signal: five events of Type II and 70 of Type III between September 2015 and May 2019. The analysis of solar radio bursts in the MEXART signal provide us valuable…
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