Analysis of the spectra of the coronal condensation at the solar eclipse of June 11, 1983.

Details Analysis of the spectra of the coronal condensation at the solar eclipse of June 11, 1983. Analysis of the spectra of the coronal condensation at the solar eclipse of June 11, 1983.

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993acaps..13..253l&link_type=abstract

Acta Astrophys. Sin., Vol. 13, No. 3, p. 253 - 262

Astronomy and Astrophysics

Astrophysics

Scientific paper

The distributions of the electron density and temperature in a coronal condensation were obtained by analysing the coronal spectrograms taken at the total eclipse of 1983 June 11. The electron density was higher in the centre of the condensation than on the edge. From different line pairs the maximum electron density was found to be between 1.7 - 3.5×109cm-3 while the temperature was found to be basically uniform at 1.7 - 2.7×106K. The turbulence velocity was 15 - 35 km/s and the relative motion velocity between the condensation and the quiet corona was less than 15 km/s.

Affiliated with

Also associated with

No associations

Rating

Analysis of the spectra of the coronal condensation at the solar eclipse of June 11, 1983. does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Analysis of the spectra of the coronal condensation at the solar eclipse of June 11, 1983., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Analysis of the spectra of the coronal condensation at the solar eclipse of June 11, 1983. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1066809