Semi-weekly monitoring of the performance and attitude of Kepler using a sparse set of targets
Identifieur interne : 000A66 ( Main/Exploration ); précédent : 000A65; suivant : 000A67Semi-weekly monitoring of the performance and attitude of Kepler using a sparse set of targets
Auteurs : Hema Chandrasekaran [États-Unis] ; Jon M. Jenkins [États-Unis] ; JIE LI [États-Unis] ; Forrest R. Girouard [États-Unis] ; Joseph D. Twicken [États-Unis] ; Douglas A. Caldwell [États-Unis] ; Christopher Allen [États-Unis] ; Stephen T. Bryson [États-Unis] ; Todd C. Klaus [États-Unis] ; Miles T. Cote [États-Unis] ; Brett A. Stroozas [États-Unis] ; Jennifer R. Hall [États-Unis] ; Khadeejah Ibrahim [États-Unis]Source :
- Proceedings of SPIE, the International Society for Optical Engineering [ 0277-786X ] ; 2010.
Descripteurs français
- Pascal (Inist)
- Wicri :
- topic : Satellite.
English descriptors
- KwdEn :
Abstract
The Kepler spacecraft is in a heliocentric Earth-trailing orbit, continuously observing ˜160,000 select stars over ˜115 square degrees of sky using its photometer containing 42 highly sensitive CCDs. The science data from these stars, consisting of ˜6 million pixels at 29.4-minute intervals, is downlinked only every ˜30 days. Additional low-rate X-band communications contacts are conducted with the spacecraft twice a week to downlink a small subset of the science data. This paper describes how we assess and monitor the performance of the photometer and the pointing stability of the spacecraft using such a sparse data set.
Affiliations:
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Le document en format XML
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<term>Measurement</term>
<term>Monitoring</term>
<term>Orbit</term>
<term>Satellite</term>
<term>Sky</term>
<term>Solid dynamic</term>
<term>Spacecraft</term>
<term>Sparse set</term>
<term>Star</term>
<term>Surveillance</term>
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<term>Surveillance</term>
<term>Mesure</term>
<term>Attitude</term>
<term>Spationef</term>
<term>Satellite</term>
<term>Orbite</term>
<term>Dynamique solide</term>
<term>Ensemble épars</term>
<term>Etoile</term>
<term>Ciel</term>
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<front><div type="abstract" xml:lang="en">The Kepler spacecraft is in a heliocentric Earth-trailing orbit, continuously observing ˜160,000 select stars over ˜115 square degrees of sky using its photometer containing 42 highly sensitive CCDs. The science data from these stars, consisting of ˜6 million pixels at 29.4-minute intervals, is downlinked only every ˜30 days. Additional low-rate X-band communications contacts are conducted with the spacecraft twice a week to downlink a small subset of the science data. This paper describes how we assess and monitor the performance of the photometer and the pointing stability of the spacecraft using such a sparse data set.</div>
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<name sortKey="Bryson, Stephen T" sort="Bryson, Stephen T" uniqKey="Bryson S" first="Stephen T." last="Bryson">Stephen T. Bryson</name>
<name sortKey="Caldwell, Douglas A" sort="Caldwell, Douglas A" uniqKey="Caldwell D" first="Douglas A." last="Caldwell">Douglas A. Caldwell</name>
<name sortKey="Chandrasekaran, Hema" sort="Chandrasekaran, Hema" uniqKey="Chandrasekaran H" first="Hema" last="Chandrasekaran">Hema Chandrasekaran</name>
<name sortKey="Cote, Miles T" sort="Cote, Miles T" uniqKey="Cote M" first="Miles T." last="Cote">Miles T. Cote</name>
<name sortKey="Girouard, Forrest R" sort="Girouard, Forrest R" uniqKey="Girouard F" first="Forrest R." last="Girouard">Forrest R. Girouard</name>
<name sortKey="Hall, Jennifer R" sort="Hall, Jennifer R" uniqKey="Hall J" first="Jennifer R." last="Hall">Jennifer R. Hall</name>
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<name sortKey="Jenkins, Jon M" sort="Jenkins, Jon M" uniqKey="Jenkins J" first="Jon M." last="Jenkins">Jon M. Jenkins</name>
<name sortKey="Jie Li" sort="Jie Li" uniqKey="Jie Li" last="Jie Li">JIE LI</name>
<name sortKey="Klaus, Todd C" sort="Klaus, Todd C" uniqKey="Klaus T" first="Todd C." last="Klaus">Todd C. Klaus</name>
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<name sortKey="Twicken, Joseph D" sort="Twicken, Joseph D" uniqKey="Twicken J" first="Joseph D." last="Twicken">Joseph D. Twicken</name>
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