Titlebook: 5th International Symposium of Space Optical Instruments and Applications; Beijing, China, Sept H. Paul Urbach,Qifeng Yu Conference proceed

兇猛

?konomie der Geschlechterdifferenzentation (EWO) algorithm, where pitch/yaw/roll angle errors were well considered in the orientation error aspect. The result showed that by adding two 0.5″ star cameras and optimal layout design, the pitching angle error was minimized to 0.4″, which was satisfied to the high-precision stereo mapping

incisive

現(xiàn)暈光

50plus in Deutschland und Europaysis by the finite element model (FEM), we can get that six degrees of freedom displacement of the optical element. Using the six degrees of freedom displacement data with optical sensitivity matrix, we can get a camera LOS of the short-term and long-term changes in value. The results show that the

lattice

https://doi.org/10.1007/978-3-531-91455-8h richer information for the research on space science exploration. The application of hyperspectral imaging in deep space exploration is discussed. The spectrometers using filters, grating spectrometers, and Fourier transform spectrometers applied in previous deep space exploration missions are con

irreparable

立即

Ronald Wipplinger,Rudolf Winter-Ebmerpping spectrometer (IMS) are all typical examples. In IFS-M, the two-dimensional field of interest is optically divided into small samples that are re-imaged at the entrance plane of the spectrograph. It has the characteristics of low spatial resolution. IFS-F uses a reformatter fiber optics to map

誘騙

太空

Influence of Micro-Vibration Caused by Momentum Wheel on the Imaging Quality of Space Camera,978-3-8349-7120-3

Mets552

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