Precision spectrophotometry of the sun as a star

Details Precision spectrophotometry of the sun as a star Precision spectrophotometry of the sun as a star

Oct 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990kfnt....6...67g&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 6, Sept.-Oct. 1990, p. 67-74. In Russian.

Physics

Image Processing, Signal Reception, Solar Spectrometers, Stellar Spectrophotometry, Scanning, Spectrophotometers, Spectrum Analysis

Scientific paper

The main deficiencies of existing techniques for the spectrophotometry of the sun as a star are examined. A new observational method based on the cyclic scanning of the solar image and on the time integration of the received signal is proposed. The optimal utilization of this method is considered. The implementation of the proposed method on double-diffraction monochromators is discussed along with the role of the aperture diaphragm.

Affiliated with

Also associated with

No associations

Rating

Precision spectrophotometry of the sun as a star 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 Precision spectrophotometry of the sun as a star, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Precision spectrophotometry of the sun as a star will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1304643