Abstract
The distribution of average intensity scattered by a plane mirror placed behind a turbulent phase screen is experimentally investigated for a point source of light. It was found that the average intensity distribution in the source plane coincides with the correlation function of intensity fluctuations of a virtual source located at the mirror and observed from the real source plane. Nonmonotonic dependence between the enhancement factor and the diameter of the mirror is observed in experiments. Experimental results are in good agreement with theoretical predictions.
© 1991 Optical Society of America
Full Article |
PDF Article
More Like This
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
Equations (25)
You do not have subscription access to this journal. Equations 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