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- W1990495965 abstract "High-performance baffles are required in the operation of space sensors mounted aboard a satellite to track stars for attitude control or to identify the sky region aimed by a paralleled X-ray telescope. For example, on a typical X-ray observation mission, the star sensor shall identify stars in a 8 deg by 8 deg field of view down to the 6th magnitude, even when very bright sources (as the sun or the earth horizon) are only 10-15 degrees off the field of view. This corresponds to attenuate stray light down to approximately 10-9, what calls for a very sophisticated design of the optical baffle and also is an unusual requirement for the measurement of attenuation in the test-laboratory to validate the baffle before launch.1,2." @default.
- W1990495965 created "2016-06-24" @default.
- W1990495965 creator A5029389811 @default.
- W1990495965 date "1990-01-02" @default.
- W1990495965 modified "2023-09-23" @default.
- W1990495965 title "Measurement Of Light-Baffle Attenuation By A Gating Technique" @default.
- W1990495965 doi "https://doi.org/10.1117/12.962848" @default.
- W1990495965 hasPublicationYear "1990" @default.
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