Abstract
The effect of random longitudinal motion of an image is discussed. Numerical results are given for
systems with circular and annular pupils. It is shown that, for a given value of the image motion, the time-averaged
Strehl ratio is larger for a larger value of the obscuration ratio of an annular pupil. We also show
that the time-averaged image irradiance distribution near its center and the corresponding encircled power
can be obtained from their aberration-free values by multiplying them by the Strehl ratio.
© 2007 Optical Society of America
Full Article |
PDF Article
More Like This
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 Optica member, or as an authorized user of your institution.
Contact your librarian or system administrator
or
Login to access Optica Member Subscription
Figures (7)
You do not have subscription access to this journal. Figure files are available to subscribers only. You may subscribe either as an Optica member, or as an authorized user of your institution.
Contact your librarian or system administrator
or
Login to access Optica Member Subscription
Tables (2)
You do not have subscription access to this journal. Article tables are available to subscribers only. You may subscribe either as an Optica member, or as an authorized user of your institution.
Contact your librarian or system administrator
or
Login to access Optica Member Subscription
Equations (13)
You do not have subscription access to this journal. Equations are available to subscribers only. You may subscribe either as an Optica member, or as an authorized user of your institution.
Contact your librarian or system administrator
or
Login to access Optica Member Subscription