Final Technical Report on Contract Nonr(G)001-60
Abstract
The authors have proceeded to a more detailed analysis of the solar spectra in order to examine the characteristics of certain lines as a function of time. The plates, as well as the corresponding calibration data, have been converted by means of the microphotometer so as to give a geometrical representation of the relative brightness of any given part of the spectrum. Having reduced the spectra to the form intensity vs wavelength, the authors have proceeded to the analysis of individual line profiles, which we have determined as a function, in wavelength, of the line intensity related to the continuum intensity.
Document Details
- Document Type
- Technical Report
- Publication Date
- Jan 01, 1972
- Accession Number
- AD0740884
Entities
People
- B. Folkart
- J. C. Pecker
- J. Rountree-lesh
- S. R. Pottasch
Organizations
- Paris Observatory, PSL University