Abstract

Astronomical applications suggest wave-front control algorithms that maximize the fractional area of the pupil over which the wave-front distortion is smaller than an eighth of a wave.

© 1992 Optical Society of America

Full Article  |  PDF Article
OSA Recommended Articles
Wave-front correction from point spread function data

Naoshi Baba, Tsutomu Ogura, and Noriaki Miura
Appl. Opt. 32(26) 4979-4983 (1993)

Method for a quantitative investigation of the frozen flow hypothesis

Matthias Schöck and Earl J. Spillar
J. Opt. Soc. Am. A 17(9) 1650-1658 (2000)

References

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
Login to access OSA Member Subscription

Cited By

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
Login to access OSA Member Subscription

Figures (2)

You do not have subscription access to this journal. Figure files 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
Login to access OSA Member Subscription

Metrics

You do not have subscription access to this journal. Article level metrics 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
Login to access OSA Member Subscription