Duty cycle of Doppler ground-based asteroseismic observations

We report the observations of the clear sky fraction at the Concordia station during winter 2006, and derive from it the duty cycle for astronomical observations. Performance in duty cycle and observation duration promotes Dome C for efficient asteroseismic observations. This performance is analyzed...

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Main Authors: Benoit, M, Eric, A
Language:English
Published: 2006
Subjects:
Online Access:http://cds.cern.ch/record/1006297
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spelling ftcern:oai:cds.cern.ch:1006297 2023-05-15T13:58:28+02:00 Duty cycle of Doppler ground-based asteroseismic observations Benoit, M Eric, A 2006-12-18 http://cds.cern.ch/record/1006297 eng eng http://cds.cern.ch/record/1006297 astro-ph/0612506 oai:cds.cern.ch:1006297 Astrophysics and Astronomy 2006 ftcern 2018-07-28T08:41:24Z We report the observations of the clear sky fraction at the Concordia station during winter 2006, and derive from it the duty cycle for astronomical observations. Performance in duty cycle and observation duration promotes Dome C for efficient asteroseismic observations. This performance is analyzed and compared to network observation. For network observations, simulations were run considering the helioseismic network GONG as a reference. Observations with 1 site in Antarctica provide performance similar or better than with a 6-site network, since the duty cycle limited by meteorology is as high as 92%. On bright targets, a 100-day long time series with a duty cycle about 87% can be observed, what network observation cannot. Other/Unknown Material Antarc* Antarctica CERN Document Server (CDS) Concordia Station ENVELOPE(123.333,123.333,-75.100,-75.100)
institution Open Polar
collection CERN Document Server (CDS)
op_collection_id ftcern
language English
topic Astrophysics and Astronomy
spellingShingle Astrophysics and Astronomy
Benoit, M
Eric, A
Duty cycle of Doppler ground-based asteroseismic observations
topic_facet Astrophysics and Astronomy
description We report the observations of the clear sky fraction at the Concordia station during winter 2006, and derive from it the duty cycle for astronomical observations. Performance in duty cycle and observation duration promotes Dome C for efficient asteroseismic observations. This performance is analyzed and compared to network observation. For network observations, simulations were run considering the helioseismic network GONG as a reference. Observations with 1 site in Antarctica provide performance similar or better than with a 6-site network, since the duty cycle limited by meteorology is as high as 92%. On bright targets, a 100-day long time series with a duty cycle about 87% can be observed, what network observation cannot.
author Benoit, M
Eric, A
author_facet Benoit, M
Eric, A
author_sort Benoit, M
title Duty cycle of Doppler ground-based asteroseismic observations
title_short Duty cycle of Doppler ground-based asteroseismic observations
title_full Duty cycle of Doppler ground-based asteroseismic observations
title_fullStr Duty cycle of Doppler ground-based asteroseismic observations
title_full_unstemmed Duty cycle of Doppler ground-based asteroseismic observations
title_sort duty cycle of doppler ground-based asteroseismic observations
publishDate 2006
url http://cds.cern.ch/record/1006297
long_lat ENVELOPE(123.333,123.333,-75.100,-75.100)
geographic Concordia Station
geographic_facet Concordia Station
genre Antarc*
Antarctica
genre_facet Antarc*
Antarctica
op_relation http://cds.cern.ch/record/1006297
astro-ph/0612506
oai:cds.cern.ch:1006297
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