Hard microflares produce prompt solar energetic electrons with hard spectra, extending the known HXR-electron spectral index correlation to smaller events and demonstrating efficient acceleration without large flare energy.
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High-resolution coronagraph images resolve CME substructures and fast circular wave-trains interpreted as quasi-periodic propagating fast magnetosonic modes.
citing papers explorer
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Solar Orbiter observations of solar energetic electron events associated with hard microflares
Hard microflares produce prompt solar energetic electrons with hard spectra, extending the known HXR-electron spectral index correlation to smaller events and demonstrating efficient acceleration without large flare energy.
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A view of the evolution of a CME and the associated wave-trains at high spatial and temporal resolution
High-resolution coronagraph images resolve CME substructures and fast circular wave-trains interpreted as quasi-periodic propagating fast magnetosonic modes.