Abstract
We have searched for nonthermal radio signatures in the form of metric type III bursts in conjunction with two-sided-loop-type X-ray jets observed by the Yohkoh/SXT experiment. We have found no evidence of type III bursts in association with this particular type of X-ray jets in contrast to the positive evidence of type III's in association with anemone-type X-ray jets. This result is consistent with the simulation results of Yokoyama and Shibata (1995), which show that anemone-type jets are produced by vertical/oblique plasma flow whereas the two-sided-loop-type jets are produced by horizontal plasma flow.
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Kundu, M.R., Raulin, JP., Nitta, N. et al. Two-Sided-Loop-Type X-ray Jets and Metric Radio Bursts. Solar Physics 178, 173–178 (1998). https://doi.org/10.1023/A:1005018109815
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DOI: https://doi.org/10.1023/A:1005018109815