The Association of a J-burst with a Solar Jet
D. E. Morosan, P. T. Gallagher, R. A. Fallows, H. Reid, G. Mann, M. M., Bisi, J. Magdalenic, H. O. Rucker, B. Thide, C. Vocks, J. Anderson, A., Asgekar, I. M. Avruch, M. E. Bell, M. J. Bentum, P. Best, R. Blaauw, A., Bonafede, F. Breitling, J. W. Broderick, M. Bruggen

TL;DR
This study links a solar jet to a J-burst, revealing how magnetic reconnection triggers energetic events and accelerates particles, with radio imaging clarifying the electrons' paths.
Contribution
It provides the first detailed association between a solar jet and a J-burst using multi-wavelength radio and EUV observations, highlighting the emission mechanism.
Findings
J-burst showed fundamental and harmonic components.
The jet was triggered by magnetic flux emergence.
Radio imaging traced the path of accelerated electrons.
Abstract
Context. The Sun is an active star that produces large-scale energetic events such as solar flares and coronal mass ejections and numerous smaller-scale events such as solar jets. These events are often associated with accelerated particles that can cause emission at radio wavelengths. The reconfiguration of the solar magnetic field in the corona is believed to be the cause of the majority of solar energetic events and accelerated particles. Aims. Here, we investigate a bright J-burst that was associated with a solar jet and the possible emission mechanism causing these two phenomena. Methods. We used data from the Solar Dynamics Observatory (SDO) to observe a solar jet, and radio data from the Low Frequency Array (LOFAR) and the Nan\c{c}ay Radioheliograph (NRH) to observe a J-burst over a broad frequency range (33-173 MHz) on 9 July 2013 at ~11:06 UT. Results. The J-burst showed…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Geophysics and Gravity Measurements · Gamma-ray bursts and supernovae
