Can the SOI/MDI Detect White Light Flares?

Details Can the SOI/MDI Detect White Light Flares? Can the SOI/MDI Detect White Light Flares?

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001agufmsh42a0765g&link_type=abstract

American Geophysical Union, Fall Meeting 2001, abstract #SH42A-0765

Physics

7524 Magnetic Fields, 7529 Photosphere, 7594 Instruments And Techniques

Scientific paper

We examine flares observed jointly with high spatial resolution by the SOHO instrument the Solar Oscillation Investigation/Michelson Doppler Imager (SOI/MDI) and the Transition Region and Coronal Explorer (TRACE). These include a GOES X1.1 class flare on 6 June 2000 and an X5.7 flare on 14 July 2000. The June flare data provide a unique set of line profiles across the flare site which help us better understand potential instrumental effects in the SOI/MDI response to flares. We locate the photospheric footpoints of the flares in both the SOI/MDI and TRACE intensity images and examine their relationship with the magnetograms. We also show that some flare kernels show emission in both the line and the continuum in SOI/MDI data.

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