NTE Analysis of Gattini Antarctic Sky Camera Data
ii iii The Gattini project consists of two site testing cameras located at Dome C on the Antarctic plateau, which are designed to measure the background sky brightness and to collect cloud cover statistics. In this thesis I present an analysis of the data produced by the Gattini cameras for the wint...
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ftciteseerx:oai:CiteSeerX.psu:10.1.1.686.1620 2023-05-15T13:54:19+02:00 NTE Analysis of Gattini Antarctic Sky Camera Data Manu E T Me Timothy Blair Leslie Supervisors Prof Michael Ashley Dr. Jon Lawrence The Pennsylvania State University CiteSeerX Archives 2007 application/pdf http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.686.1620 http://www.timl.id.au/wp-content/uploads/2012/06/astro_thesis.pdf en eng http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.686.1620 http://www.timl.id.au/wp-content/uploads/2012/06/astro_thesis.pdf Metadata may be used without restrictions as long as the oai identifier remains attached to it. http://www.timl.id.au/wp-content/uploads/2012/06/astro_thesis.pdf text 2007 ftciteseerx 2016-01-08T18:08:06Z ii iii The Gattini project consists of two site testing cameras located at Dome C on the Antarctic plateau, which are designed to measure the background sky brightness and to collect cloud cover statistics. In this thesis I present an analysis of the data produced by the Gattini cameras for the winter of 2006. Software to analyse the large data sets generated by the cameras is developed and presented along with preliminary estimates of the background sky brightness as well as cloud cover estimates. The background sky brightness is measured to be between 20.5 and 21.0 mag/arcsec2. A lower bound for the amount of time with clear skies is estimated at 79.4 % between May and Text Antarc* Antarctic Unknown Antarctic The Antarctic |
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English |
description |
ii iii The Gattini project consists of two site testing cameras located at Dome C on the Antarctic plateau, which are designed to measure the background sky brightness and to collect cloud cover statistics. In this thesis I present an analysis of the data produced by the Gattini cameras for the winter of 2006. Software to analyse the large data sets generated by the cameras is developed and presented along with preliminary estimates of the background sky brightness as well as cloud cover estimates. The background sky brightness is measured to be between 20.5 and 21.0 mag/arcsec2. A lower bound for the amount of time with clear skies is estimated at 79.4 % between May and |
author2 |
The Pennsylvania State University CiteSeerX Archives |
format |
Text |
author |
Manu E T Me Timothy Blair Leslie Supervisors Prof Michael Ashley Dr. Jon Lawrence |
spellingShingle |
Manu E T Me Timothy Blair Leslie Supervisors Prof Michael Ashley Dr. Jon Lawrence NTE Analysis of Gattini Antarctic Sky Camera Data |
author_facet |
Manu E T Me Timothy Blair Leslie Supervisors Prof Michael Ashley Dr. Jon Lawrence |
author_sort |
Manu E T Me |
title |
NTE Analysis of Gattini Antarctic Sky Camera Data |
title_short |
NTE Analysis of Gattini Antarctic Sky Camera Data |
title_full |
NTE Analysis of Gattini Antarctic Sky Camera Data |
title_fullStr |
NTE Analysis of Gattini Antarctic Sky Camera Data |
title_full_unstemmed |
NTE Analysis of Gattini Antarctic Sky Camera Data |
title_sort |
nte analysis of gattini antarctic sky camera data |
publishDate |
2007 |
url |
http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.686.1620 http://www.timl.id.au/wp-content/uploads/2012/06/astro_thesis.pdf |
geographic |
Antarctic The Antarctic |
geographic_facet |
Antarctic The Antarctic |
genre |
Antarc* Antarctic |
genre_facet |
Antarc* Antarctic |
op_source |
http://www.timl.id.au/wp-content/uploads/2012/06/astro_thesis.pdf |
op_relation |
http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.686.1620 http://www.timl.id.au/wp-content/uploads/2012/06/astro_thesis.pdf |
op_rights |
Metadata may be used without restrictions as long as the oai identifier remains attached to it. |
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1766260022471294976 |