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The Expanded Owens Valley Solar Array Reveals New Insights into Solar Flares’ Explosive Energy Releases

Four of the radio antenna dishes that make up part of the Extended Owen's Valley Solar Array

EOVSA radio intensity spectrogram of the 2017 September 10 solar flare, with frequency (vertical scale) and time (horizontal scale)

Fig. 2: Left panel shows extreme ultraviolet emission from the hot corona measured with the Atmospheric Imaging Assembly (AIA) instrument on the Solar Dynamics Observatory spacecraft at 15:54 universal time, in reverse gray scale (bright emission appears black, and dark areas are lighter gray). At this time, a cavity outlined by dotted lines is rising rapidly in the direction of the arrow labeled "Motion", surrounded by a much larger loop that is also expanding rapidly for form a coronal mass ejection (CME

24 May 2018

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2018The Expanded Owens Valley Solar Array Reveals New Insights into Solar Flares’ Explosive Energy Releases

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