Combining LOFAR type II radio imaging, STIX hard X-rays, MHD connectivity, and Solar Orbiter in situ electrons shows the electron event on 3 Oct 2023 was dominated by shock acceleration with a smaller far-side flare contribution.
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Determining the acceleration regions of in situ electrons using remote radio and X-ray observations
Combining LOFAR type II radio imaging, STIX hard X-rays, MHD connectivity, and Solar Orbiter in situ electrons shows the electron event on 3 Oct 2023 was dominated by shock acceleration with a smaller far-side flare contribution.