Changes in the atmospheric-lens modulation transfer function used for calibration in solar speckle interferometry
JOSA, Vol. 68, Issue 8, pp. 1063-1066 (1978)
http://dx.doi.org/10.1364/JOSA.68.001063
Acrobat PDF (394 KB)
Abstract
A method is described for the calibration of power spectra of nonstellar astronomical objects, by the use of changes in seeing conditions during speckle-interferometric measurements. Results are given for an application of this technique to solar granulation. The correction of 40 analyses, determined with Fried’s parameter r0 ranging between 2.5 and 11.5 cm, provides satisfactory convergence, and thus permits estimation of the solar granulation power spectrum for frequencies up to 2.5 arc sec−1.
© 1978 Optical Society of America
Citation
C. Aime, G. Ricort, C. Roddier, and G. Lago, "Changes in the atmospheric-lens modulation transfer function used for calibration in solar speckle interferometry," J. Opt. Soc. Am. 68, 1063-1066 (1978)
http://www.opticsinfobase.org/josa/abstract.cfm?URI=josa-68-8-1063
You do not have subscription access to this journal. Citation lists with outbound citation links are available to subscribers only. You may subscribe either as an OSA member, or as an authorized user of your institution.
Contact your librarian or system administrator
or
Log in to access OSA Member Subscription
You do not have subscription access to this journal. Cited by links are available to subscribers only. You may subscribe either as an OSA member, or as an authorized user of your institution.
Contact your librarian or system administrator
or
Log in to access OSA Member Subscription
« Previous Article | Next Article »
OSA is a member of 