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solar burstsAstronomy & Astrophysics Group | University of Glasgow
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89% Informative
Solar flares and coronal mass ejections (CMEs) can generate shock waves that propagate through the solar corona.
These shock waves accelerate electrons, leading to Langmuir waves that are then converted into radio emission of type II solar bursts.
Study focuses on a newly identified feature called “spectral cleaving”, which differs from band-splitting.
We attribute the spectral cleaving to changes in magnetic field orientation ahead of the propagating shock front.
The region of the most effective electron acceleration (sources of the Type II ( LFB ) emission) shifts along the shock front or even diverges, as shown in the scenario in Figure 3 .
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