Analysis of the 23 June 1988 flare using NIXT multilayer X-ray images

Details Analysis of the 23 June 1988 flare using NIXT multilayer X-ray images Analysis of the 23 June 1988 flare using NIXT multilayer X-ray images

Jul 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989spie.1160..629g&link_type=abstract

IN: X-ray/EUV optics for astronomy and microscopy; Proceedings of the Meeting, San Diego, CA, Aug. 7-11, 1989 (A90-46006 21-74).

Computer Science

Sound

15

Imaging Techniques, Solar Flares, Sounding Rockets, X Ray Astrophysics Facility, X Ray Telescopes, Emission Spectra, Laminates, Onboard Equipment, Solar Corona

Scientific paper

Results obtained during the June 23, 1988 flight of the normal incidence X-ray telescope (NIXT) sounding rocket payload are reported. The telescope primary is 25 cm in diameter, in a 750 cm e.f.l. (f/30) Ritchey-Chretien configuration, with multilayer coatings on the optics designed to image the Fe XVI and Mg X coronal emission lines near 63.5 A. Images of the onset phase of a large (M8) Solar flare were recorded during the flight on a modified T-max 400 film manufactured by Kodak. Some of the results obtained by comparison of the NIXT data with ground-based observations of the sun obtained simultaneously to the flight are also reported.

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