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Paper: XRT and EIS Observations of Reconnection Associated Phenomena
Volume: 369, New Solar Physics with Solar-B Mission
Page: 439
Authors: Shiota, D.; Isobe, H.; Brooks, D.H.; Chen, P.-F.; Shibata, K.
Abstract: Based on the results of numerical simulations, we sythesized EIS and XRT images of reconnection flows associated with an eruptive flare. The results suggest that reconnection inflows can be observed as pairs of blue- and red-shifted components just above the X-ray arcade in the low temperature lines. It is found that the Doppler velocities are larger in the lower temperature line spectra. Reconnection outflows can also be observed as pairs of blue- and redshifted components with an asymmetry in the high temperature line spectra.
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