The green coronal line above an active region at the solar limb on 5 Aug. of 1989.

Details The green coronal line above an active region at the solar limb on 5 Aug. of 1989. The green coronal line above an active region at the solar limb on 5 Aug. of 1989.

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991chjss..11..286d&link_type=abstract

Chin. J. Space Sci., Vol. 11, No. 4, p. 286 - 290

Physics

Solar Corona: Spectral Lines, Sunspot Groups: Continuum Radiation

Scientific paper

The green coronal line above the sunspot group No. 5629 of 5 Aug. of 1989 with excited continuum and bright knots is observed. According to the intensities of the continuum, the following parameters are estimated: the electron densities are 3·109 - 1011/cm, half width is up to 1.2 Å, temperature is 4 - 5·106K without considering turbulent velocity, and the sizes of strong radiation regions along the direction of line of sight are 0.5·109cm.

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