High-resolution studies of the structure of the solar atmosphere using a new imaging algorithm

Details High-resolution studies of the structure of the solar atmosphere using a new imaging algorithm High-resolution studies of the structure of the solar atmosphere using a new imaging algorithm

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...371..402k&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 371, April 10, 1991, p. 402-407.

Astronomy and Astrophysics

Astrophysics

9

Image Processing, Solar Atmosphere, Solar Spectra, Solar Temperature, Ultraviolet Spectra, Algorithms, Extreme Ultraviolet Explorer Satellite, High Resolution, Skylab Program

Scientific paper

The results of the application of a new image restoration algorithm developed by Ayers and Dainty (1988) to the multiwavelength EUV/Skylab observations of the solar atmosphere are presented. The application of the algorithm makes it possible to reach a resolution better than 5 arcsec, and thus study the structure of the quiet sun on that spatial scale. The results show evidence for discrete looplike structures in the network boundary, 5-10 arcsec in size, at temperatures of 100,000 K.

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