Speckle image reconstruction of solar features

Details Speckle image reconstruction of solar features Speckle image reconstruction of solar features

Mar 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977natur.266..149s&link_type=abstract

Nature, vol. 266, Mar. 10, 1977, p. 149-151. NSF-supported research.

Astronomy and Astrophysics

Astronomy

17

Astronomical Photography, Atmospheric Turbulence, Imaging Techniques, Speckle Patterns, Fourier Transformation, High Resolution, Telescopes, Transfer Functions

Scientific paper

The application of speckle imaging to reconstruction of solar surface features with resolution approaching the telescope limit despite severe atmospheric blurring in the original data is described. The imaging process is outlined, and sample reconstructions of solar photographs exhibiting relatively small surface features are presented. It is noted that the ultimate resolution of the process is the diffraction limit of the telescope, independent of seeing conditions.

Affiliated with

Also associated with

No associations

Rating

Speckle image reconstruction of solar features 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 Speckle image reconstruction of solar features, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Speckle image reconstruction of solar features will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1849565