Tv Experiment on VEGA Mission: Strategy, Hardware, Software

Details Tv Experiment on VEGA Mission: Strategy, Hardware, Software Tv Experiment on VEGA Mission: Strategy, Hardware, Software

Dec 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986esasp.250b.289s&link_type=abstract

The Exploration of Halley's Comet. Volume 2: Dust and Nucleus Proceedings of the 20th ESLAB Symposium held in Heidelberg, West G

Astronomy and Astrophysics

Astronomy

Scientific paper

The strategy of the TV experiment is described. The television system (TVS) was designed as a two-camera, four channel system with CCD imagers. It permits imaging with angular resolutions of about 35 and 28 arc s in six different spectral bands in the range 400 - 1100 nm. The image formats sent to the Earth are 128×128 and 512×512 pixels. The TVS was placed on a pointing platform. The pointing of the platform during the encounter was also controlled by the TVS's processor after it analysed the images obtained.

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