Detection and characterization of 613 repeating radio burst pairs in the solar corona at 30-50 MHz, with delayed components interpreted as turbulent echoes of harmonic emission via imaging spectroscopy and propagation simulations.
Jr.: Magnetic Fields and the Structure of the Solar Corona
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Polytropic stellar wind models are extended beyond extreme adiabatic cases to non-adiabatic localized heating, with added energy shown plausible relative to flares and relevant to solar wind observations.
Statistical analysis shows solar energetic electrons rarely cross the heliospheric current sheet unless the source or spacecraft is close to it.
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