Emission curve of growth for Fe II in chromospheric limb spectra

Details Emission curve of growth for Fe II in chromospheric limb spectra Emission curve of growth for Fe II in chromospheric limb spectra

Jul 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986soph..106...87h&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 106, July 1986, p. 87-93.

Statistics

Computation

Chromosphere, Emission Spectra, Iron, Line Shape, Solar Limb, Computational Astrophysics, Temperature Dependence

Scientific paper

The 270 chromospheric emission lines of Fe II ranging between 2000 and 3200 Å observed by Skylab at a height of 4arcsec (2900 km) above the limb of the quiet sun are analyzed by the emission curve of growth method, using newly calculated gf-values. It is derived that the excitation temperature is 7.2×103K and that the turbulent velocity is consistent with the previous results that the microturbulent velocity is lower than 10 km s-1 in the cool (<104K) region of the chromosphere.

Affiliated with

Also associated with

No associations

Rating

Emission curve of growth for Fe II in chromospheric limb spectra 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 Emission curve of growth for Fe II in chromospheric limb spectra, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Emission curve of growth for Fe II in chromospheric limb spectra will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1656944