A Laser Frequency Comb System for Absolute Calibration of the VTT Echelle Spectrograph
A wavelength calibration system based on a laser frequency comb (LFC) was developed in a co-operation between the Kiepenheuer-Institut für Sonnenphysik, Freiburg, Germany and the Max-Planck-Institut für Quantenoptik, Garching, Germany for permanent installation at the German Vacuum Tower Telescope (...
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Veröffentlicht in: | Solar physics 2012-10, Vol.280 (2), p.663-670 |
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creator | Doerr, H.-P. Steinmetz, T. Holzwarth, R. Kentischer, T. Schmidt, W. |
description | A wavelength calibration system based on a laser frequency comb (LFC) was developed in a co-operation between the Kiepenheuer-Institut für Sonnenphysik, Freiburg, Germany and the Max-Planck-Institut für Quantenoptik, Garching, Germany for permanent installation at the German
Vacuum Tower Telescope
(VTT) on Tenerife, Canary Islands. The system was installed successfully in October 2011. By simultaneously recording the spectra from the Sun and the LFC, for each exposure a calibration curve can be derived from the known frequencies of the comb modes that is suitable for absolute calibration at the meters per second level. We briefly summarize some topics in solar physics that benefit from absolute spectroscopy and point out the advantages of LFC compared to traditional calibration techniques. We also sketch the basic setup of the VTT calibration system and its integration with the existing echelle spectrograph. |
doi_str_mv | 10.1007/s11207-012-9960-5 |
format | Article |
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Vacuum Tower Telescope
(VTT) on Tenerife, Canary Islands. The system was installed successfully in October 2011. By simultaneously recording the spectra from the Sun and the LFC, for each exposure a calibration curve can be derived from the known frequencies of the comb modes that is suitable for absolute calibration at the meters per second level. We briefly summarize some topics in solar physics that benefit from absolute spectroscopy and point out the advantages of LFC compared to traditional calibration techniques. We also sketch the basic setup of the VTT calibration system and its integration with the existing echelle spectrograph.</description><identifier>ISSN: 0038-0938</identifier><identifier>EISSN: 1573-093X</identifier><identifier>DOI: 10.1007/s11207-012-9960-5</identifier><language>eng</language><publisher>Dordrecht: Springer Netherlands</publisher><subject>Advances in European Solar Physics ; Astrophysics and Astroparticles ; Atmospheric Sciences ; Calibration ; Lasers ; Measuring instruments ; Physics ; Physics and Astronomy ; Recording ; Solar physics ; Space Exploration and Astronautics ; Space Sciences (including Extraterrestrial Physics ; Space telescopes ; Spectra ; Spectroscopy ; Spectrum analysis ; Telescopes</subject><ispartof>Solar physics, 2012-10, Vol.280 (2), p.663-670</ispartof><rights>Springer Science+Business Media B.V. 2012</rights><rights>Springer Science+Business Media Dordrecht 2012</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c382t-41d5cdeeac548c70d5e945ddbae752d4a6d9e8582c2c0d06b5961ebc470b46993</citedby><cites>FETCH-LOGICAL-c382t-41d5cdeeac548c70d5e945ddbae752d4a6d9e8582c2c0d06b5961ebc470b46993</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1007/s11207-012-9960-5$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1007/s11207-012-9960-5$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>314,780,784,27924,27925,41488,42557,51319</link.rule.ids></links><search><creatorcontrib>Doerr, H.-P.</creatorcontrib><creatorcontrib>Steinmetz, T.</creatorcontrib><creatorcontrib>Holzwarth, R.</creatorcontrib><creatorcontrib>Kentischer, T.</creatorcontrib><creatorcontrib>Schmidt, W.</creatorcontrib><title>A Laser Frequency Comb System for Absolute Calibration of the VTT Echelle Spectrograph</title><title>Solar physics</title><addtitle>Sol Phys</addtitle><description>A wavelength calibration system based on a laser frequency comb (LFC) was developed in a co-operation between the Kiepenheuer-Institut für Sonnenphysik, Freiburg, Germany and the Max-Planck-Institut für Quantenoptik, Garching, Germany for permanent installation at the German
Vacuum Tower Telescope
(VTT) on Tenerife, Canary Islands. The system was installed successfully in October 2011. By simultaneously recording the spectra from the Sun and the LFC, for each exposure a calibration curve can be derived from the known frequencies of the comb modes that is suitable for absolute calibration at the meters per second level. We briefly summarize some topics in solar physics that benefit from absolute spectroscopy and point out the advantages of LFC compared to traditional calibration techniques. 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Vacuum Tower Telescope
(VTT) on Tenerife, Canary Islands. The system was installed successfully in October 2011. By simultaneously recording the spectra from the Sun and the LFC, for each exposure a calibration curve can be derived from the known frequencies of the comb modes that is suitable for absolute calibration at the meters per second level. We briefly summarize some topics in solar physics that benefit from absolute spectroscopy and point out the advantages of LFC compared to traditional calibration techniques. We also sketch the basic setup of the VTT calibration system and its integration with the existing echelle spectrograph.</abstract><cop>Dordrecht</cop><pub>Springer Netherlands</pub><doi>10.1007/s11207-012-9960-5</doi><tpages>8</tpages></addata></record> |
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subjects | Advances in European Solar Physics Astrophysics and Astroparticles Atmospheric Sciences Calibration Lasers Measuring instruments Physics Physics and Astronomy Recording Solar physics Space Exploration and Astronautics Space Sciences (including Extraterrestrial Physics Space telescopes Spectra Spectroscopy Spectrum analysis Telescopes |
title | A Laser Frequency Comb System for Absolute Calibration of the VTT Echelle Spectrograph |
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