High-resolution spectra of the solar MG II H and K lines from SKYLAB

Details High-resolution spectra of the solar MG II H and K lines from SKYLAB High-resolution spectra of the solar MG II H and K lines from SKYLAB

Dec 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977apjs...35..471d&link_type=abstract

Astrophysical Journal Supplement Series, vol. 35, Dec. 1977, p. 471-482.

Astronomy and Astrophysics

Astronomy

21

H Lines, K Lines, Skylab Program, Solar Spectra, Spaceborne Astronomy, Chromosphere, High Resolution, Line Spectra, Solar Atmosphere, Solar Granulation, Ultraviolet Spectra

Scientific paper

Spectra of the Mg II h and k lines emitted by different regions in the solar atmosphere have been recorded by the NRL slit spectrograph on Skylab. The spectral resolution is 0.12 A, and the spatial resolution is 2 by 60 arcsec. Several examples are presented, including spectra of a chromospheric supergranulation cell boundary and interior and of a quiet-sun region above the limb, as well as selected active-region spectra on the disk and above the limb. Obvious differences among these spectra are noted and qualitatively discussed.

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