The solar O I 7773 A triplet. II - Analysis using line inversion techniques

Details The solar O I 7773 A triplet. II - Analysis using line inversion techniques The solar O I 7773 A triplet. II - Analysis using line inversion techniques

Mar 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985soph...96....1k&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 96, March 1985, p. 1-10. Research supported by the Australian Research Grants Committee.

Physics

4

Continuous Radiation, Infrared Spectra, Line Spectra, Solar Physics, Solar Spectra, Spectral Line Width, Atomic Energy Levels, Doppler Effect, Photosphere, Solar Granulation, Solar Temperature, Spatial Resolution, Turbulence, Velocity Distribution

Scientific paper

Spectral line inversion techniques developed by Hearn and Holt (1973), in which the total source function is represented by piecewise linear segments in the line center optical depth, are presently used to analyze profiles of the O I 7773 triplet having a spatial resolution of about 0.5 arcsec. Microturbulence values are found which are in good agreement with those found by Blackwell and Shallis (1979). The velocity gradients have the same signs in upflows and downflows.

Affiliated with

Also associated with

No associations

Rating

The solar O I 7773 A triplet. II - Analysis using line inversion techniques 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 The solar O I 7773 A triplet. II - Analysis using line inversion techniques, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The solar O I 7773 A triplet. II - Analysis using line inversion techniques will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-928685