Connecting Chromospheric Condensation Signatures to Reconnection Driven Heating Rates in an Observed Flare
William H. Ashfield,
Dana W. Longcope,
Chunming Zhu
et al.
Abstract:Observations of solar flare reconnection at very high spatial and temporal resolution can be made indirectly at the footpoints of reconnected loops into which flare energy is deposited. The response of the lower atmosphere to this energy input includes a downward-propagating shock called chromospheric condensation, which can be observed in the UV and visible. In order to characterize reconnection using high-resolution observations of this response, one must develop a quantitative relationship between the two. … Show more
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