XRT and EIS Observations of Reconnection Associated Phenomena

Details XRT and EIS Observations of Reconnection Associated Phenomena XRT and EIS Observations of Reconnection Associated Phenomena

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..369..439s&link_type=abstract

New Solar Physics with Solar-B Mission ASP Conference Series, Vol. 369, proceedings of the conference held 8-11 November, 2005 a

Physics

Scientific paper

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 red-shifted components with an asymmetry in the high temperature line spectra.

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