A year of operation of Melibea e-Callisto Solar Radio Telescope

24th European Cosmic Ray Symposium

Russu, A.^1,2 ; Gómez-Herrero, R.^1,2 ; Prieto, M.^1,2 ; Monstein, C.^3 ; Ivanov, H.^2 ; Rodríguez-Pacheco, J.^1,2 ; Blanco, J.J.^1,2

Space Research Group (SRG), University of Alcalá, Alcalá de Henares, Spain^1

Parque Científico y Tecnológico de Guadalajara (PCyT), Guadalajara, Mexico^2

Institute for Astronomy, Swiss Federal Institute of Technology Zurich (ETHZ), Switzerland^3

关键词: Coronal mass ejection;    First year;    Low frequency instrument;    Radio bursts;    Solar energetic particles;    Solar radio bursts;    Space-borne;    Swiss Federal Institute of Technology;   

Others  :  https://iopscience.iop.org/article/10.1088/1742-6596/632/1/012078/pdf
DOI  :  10.1088/1742-6596/632/1/012078

来源: IOP

【 摘 要 】

The e-CALLISTO (Compound Astronomical Low-cost Low-frequency Instrument for Spectroscopy and Transportable Observatory) is a worldwide radio-spectrograph network with 24 hours a day solar radio burst monitoring. The e-CALLISTO network is led by the Swiss Federal Institute of Technology Zurich (ETHZ Zurich), which work up collaborations with local host institutions. In 2013 the University of Alcalá joined the e-CALLISTO network with the installation of two Solar Radio Telescopes (SRT): the EA4RKU-SRT that was located at the University of Alcalá from January 2013 till June 2013 and the Melibea-SRT that is located at Peralejos de las Truchas (Guadalajara) in operation from June 2013. The Spanish e-Callisto SRTs provide routine data to the network. We present examples of type III and type II radio-bursts observed by Melibea during its first year of operation and study their relation with soft X-ray flares observed by GOES and Coronal Mass Ejections (CMEs) and Solar Energetic Particle (SEP) events observed by space-borne instrumentation.