Extreme-ultraviolet observations of coronal holes - Initial results from SKYLAB

Details Extreme-ultraviolet observations of coronal holes - Initial results from SKYLAB Extreme-ultraviolet observations of coronal holes - Initial results from SKYLAB

Dec 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974apj...194l.115h&link_type=abstract

Astrophysical Journal, vol. 194, Dec. 1, 1974, pt. 2, p. L115-L118.

Astronomy and Astrophysics

Astronomy

89

Far Ultraviolet Radiation, Skylab Program, Solar Corona, Spaceborne Astronomy, Spectroheliographs, Chromosphere, Fine Structure, Histograms, Line Spectra, Solar Limb

Scientific paper

We compare the appearance and physical parameters of the solar chromosphere, transition zone, and corona in areas of coronal holes with that of quiet areas outside the hole. Measurements of the height of emission of various ions in a coronal hole appearing at the polar limb give a quantitative indication of the increased thickness of the transition zone underlying coronal holes.

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