Temperature gradients in the inner corona

Details Temperature gradients in the inner corona Temperature gradients in the inner corona

Nov 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978soph...60...67m&link_type=abstract

Solar Physics, vol. 60, Nov. 1978, p. 67-82.

Physics

15

Emission Spectra, Far Ultraviolet Radiation, Solar Corona, Solar Temperature, Temperature Gradients, Magnesium, Oxygen Spectra, Plasma Heating, Skylab Program, Solar Spectra

Scientific paper

Emission gradient curves for extreme ultraviolet (EUV) resonance lines of O VI and Mg X have been constructed from spectroheliograms of quiet limb regions observed with the Harvard experiment on Skylab. An analysis of these data suggests that the coronal temperature rises throughout the height range 1.03-1.3 solar radii. This result implies that in quiet regions there is significant coronal heating beyond 1.3 solar radii.

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