Determination of Fried's parameter R0 prediction for the observed r.m.s. contrast in solar granulation

Details Determination of Fried's parameter R0 prediction for the observed r.m.s. contrast in solar granulation Determination of Fried's parameter R0 prediction for the observed r.m.s. contrast in solar granulation

Feb 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981soph...69..223r&link_type=abstract

Solar Physics, vol. 69, Feb. 1981, p. 223-231.

Computer Science

Performance

13

Atmospheric Turbulence, Performance Prediction, Solar Granulation, Telescopes, Interferometry, Photosphere, Solar Atmosphere, Solar Magnetic Field, Speckle Patterns

Scientific paper

Fried's seeing parameter is computed from the observed rms contrast of solar granulation on the basis of results obtained from solar speckle interferometry. The effect of telescope diameter on solar observations is shown, and predictions of observed contrast in solar granulation are made as a function of wavelength. Attention is given to the optimum telescope size to be used for given turbulence conditions, and to the importance of seeing conditions.

Affiliated with

Also associated with

No associations

Rating

Determination of Fried's parameter R0 prediction for the observed r.m.s. contrast in solar granulation 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 Determination of Fried's parameter R0 prediction for the observed r.m.s. contrast in solar granulation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Determination of Fried's parameter R0 prediction for the observed r.m.s. contrast in solar granulation will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1408992