High Resolution Spectra of the Sun

Details High Resolution Spectra of the Sun High Resolution Spectra of the Sun

Apr 1969

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1969rspta.264..171d&link_type=abstract

Philosophical Transactions for the Royal Society of London. Series A, Mathematical and Physical Sciences, Volume 264, Issue 1150

Physics

4

Scientific paper

The University of Liege has operated, since 1958, a laboratory of solar spectroscopy at the International Scientific Station of the Jungfraujoch (Switzerland). During recent years, much effort has been devoted in two main directions: (a) techniques of correction for the effects of the instrumental function to obtain the best possible knowledge of central intensities and profiles of photospheric lines; (b) increase of the signal to noise ratio in the records in order to detect and measure very faint absorption features. In addition, a balloon-borne equipment is now under construction in Liege to observe, with maximum resolution, the near infrared solar spectrum from an altitude of about 80 000 ft.

Affiliated with

Also associated with

No associations

Rating

High Resolution Spectra of the Sun 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 High Resolution Spectra of the Sun, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and High Resolution Spectra of the Sun will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1814879