Abstract
An observation method for astronomical objects is described which improves especially the angular resolving power and in some cases also the limit of detection. A modulator which is far away from a light modulates the light of the wanted object. Proper information handling enables the detector to detector decide between this light and the light of other objects. This method makes it possible to resolve details on the surface of fixed stars nearby the earth. The method can also be used to observe other physical phenomena which propagate like beams.
© 1966 Optical Society of America
Full Article |
PDF Article
OSA Recommended Articles
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 (13)
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