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.
29 January 2007Study CCD image motion for remote sensing detection
For remote sensing to measure upper atmospheric wind field by optical passive method on-load satellite, the emission
source is used of crepuscular aurora of OH 732.0nm. The time of exposure is need about 9sec by remodel Sagnac
interferometer, so there is a larger image motion on CCD and the measurement precision is limited. This paper has been
calculated the CCD image motion quantity based on remodel pushbroom model by Sagnac interferometer. The MTF
curve is demonstrated the image motion can be compensated. Then the techniques of TDICCD, the whole frame transfer,
swing mirror and photon memorizer to use compensate the image motion quantity.
The alert did not successfully save. Please try again later.
Peng Lv, Yuanhe Tang, Kai Liu, Binglong Zhang, Shijia Wang, Yufei Du, "Study CCD image motion for remote sensing detection," Proc. SPIE 6279, 27th International Congress on High-Speed Photography and Photonics, 62795S (29 January 2007); https://doi.org/10.1117/12.725458