Isoplanatism, and high spatial resolution solar imaging

Details Isoplanatism, and high spatial resolution solar imaging Isoplanatism, and high spatial resolution solar imaging

Sep 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26a...276..663i&link_type=abstract

Astronomy and Astrophysics, Vol. 276, p. 663 (1993)

Astronomy and Astrophysics

Astrophysics

5

Atmospheric Effects - Methods: Observational Techniques: Image Processing - Sun: General - Sun: Photosphere

Scientific paper

A method is presented allowing one to estimate, in the case of daytime observations, the angle-of-arrival isoplanatic patch size from the measurement of the differential image motion of the solar limb. The experimental results have been obtained using the solar astrolabe of Calern Observatory (CERGA-France). Performing a modelization as proposed by Fried (1977) leads to an explanation of these results by an equivalent atmosphere formed with two impulse turbulent layers corresponding to two different scales for the size of the isoplanatic patch. Finally, the isoplanatism is quantified for speckle interferometry and adaptive optics experiments.

Affiliated with

Also associated with

No associations

Rating

Isoplanatism, and high spatial resolution solar imaging 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 Isoplanatism, and high spatial resolution solar imaging, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Isoplanatism, and high spatial resolution solar imaging will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1558903