Imaging method for moon-based optical sensor
An optical sensor and imaging method technology, applied in astronomical navigation, navigation through velocity/acceleration measurement, etc., can solve the problem of lack of moon-based optical sensor imaging method research, the lack of clear combination of global change research, and the research on the temporal and spatial characteristics of global change. Less problems, etc., to achieve the effect of a wide range of applications
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Embodiment 1
[0125] Set the sensor, set the input data: imaging time, image resolution.
[0126] We assume that a commonly used optical sensor, a multispectral camera, is placed on the side of the moon facing the earth. The spatial resolution of the sensor is 1° in the WGS84 coordinate system. In this way, the multispectral camera can obtain a 360*180 image. Moon-based observation images in raster format, each raster takes the latitude and longitude of the center.
[0127] We take September 08, 2016 01:00 (UTC) as an example to simulate and obtain a disk observation image. 1 continuous observation image for 24 hours in the whole day of September 08, 2016 (UTC) by scanning simulation observation. Obtain the solar and lunar altitudes for each region of the world through the altitude model.
[0128] The first step is to obtain the positions of the sun's barycenter and the moon's barycenter in the geocentric inertial coordinate system from the ephemeris data.
[0129] We obtain the position...
Embodiment 2
[0167] Set the sensor, set the input data: imaging time, image resolution.
[0168]We assume that a commonly used optical sensor, a multispectral camera, is placed on the side of the moon facing the earth. The spatial resolution of the sensor is 0.5° in the WGS84 coordinate system. In this way, the multispectral camera can obtain a 720*360 image. Moon-based observation images in raster format, each raster takes the latitude and longitude of the center.
[0169] We take July 04, 2016 01:00 (UTC) as an example to simulate and obtain a disk observation image. 1 continuous observation image for 24 hours in the whole day on July 4, 2016 (UTC) by scanning simulation observation.
[0170] Obtain the solar and lunar altitudes for each region of the world through the altitude model
[0171] The first step is to obtain the positions of the sun's barycenter and the moon's barycenter in the geocentric inertial coordinate system from the ephemeris data.
[0172] We obtain the positions ...
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