You have requested a machine translation of selected content from our databases. This functionality is provided solely for your convenience and is in no way intended to replace human translation. Neither SPIE nor the owners and publishers of the content make, and they explicitly disclaim, any express or implied representations or warranties of any kind, including, without limitation, representations and warranties as to the functionality of the translation feature or the accuracy or completeness of the translations.
Translations are not retained in our system. Your use of this feature and the translations is subject to all use restrictions contained in the Terms and Conditions of Use of the SPIE website.
The development of generic optical designs for supporting wide-field imagery from an array of individual telescopes is presented. These systems will be employed to gather imagery over a total field of 0.5 to 1.0 degree. Various design possibilities are studied assuming the use of a square field, with the option of utilizing a slit field. A general optical design concept that can be transferred to a reasonable number of fairly closely packed arrays is examined, evaluating the promising three- or five-mirror arrangements.
The alert did not successfully save. Please try again later.
Cheng-Hsi Miao, Robert R. Shannon, "Design of wide-field arrays," Proc. SPIE 1236, Advanced Technology Optical Telescopes IV, (1 July 1990); https://doi.org/10.1117/12.19209