Identification of CrH and CrD Molecular Lines in the Sunspot Umbral Spectrum
High-resolution Fourier transform spectrometer sunspot umbral spectra obtained at the National Solar Observatory/Kitt Peak were used to identify molecular rotational lines arising from the infrared band systems of CrH and CrD molecules. Measurement of the equivalent width used the Gaussian-profile a...
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Veröffentlicht in: | Solar physics 2009-07, Vol.257 (2), p.261-269 |
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creator | Viswanathan, B. Shanmugavel, R. Bagare, S. P. Rajamanickam, N. Sriramachandran, P. |
description | High-resolution Fourier transform spectrometer sunspot umbral spectra obtained at the National Solar Observatory/Kitt Peak were used to identify molecular rotational lines arising from the infrared band systems of CrH and CrD molecules. Measurement of the equivalent width used the Gaussian-profile approximation method, which is suitable especially for faint lines. Equivalent widths are measured for an adequate number of best lines of the A – X (0,0) band of CrH and the A – X (0,0;1,0) bands of CrD and, thereby, the effective rotational temperatures are estimated. |
doi_str_mv | 10.1007/s11207-009-9374-1 |
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Equivalent widths are measured for an adequate number of best lines of the A – X (0,0) band of CrH and the A – X (0,0;1,0) bands of CrD and, thereby, the effective rotational temperatures are estimated.</description><identifier>ISSN: 0038-0938</identifier><identifier>EISSN: 1573-093X</identifier><identifier>DOI: 10.1007/s11207-009-9374-1</identifier><language>eng</language><publisher>Dordrecht: Springer Netherlands</publisher><subject>Approximation method ; Astrophysics ; Astrophysics and Astroparticles ; Atmospheric Sciences ; Fourier transforms ; Physics ; Physics and Astronomy ; Solar physics ; Space Exploration and Astronautics ; Space Sciences (including Extraterrestrial Physics ; Sunspots ; Temperature</subject><ispartof>Solar physics, 2009-07, Vol.257 (2), p.261-269</ispartof><rights>Springer Science+Business Media B.V. 2009</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c245t-5a43e591c1231e9ede0740f3b5daa96c6ebb730cc3be0d7628e392dd06b817f73</citedby><cites>FETCH-LOGICAL-c245t-5a43e591c1231e9ede0740f3b5daa96c6ebb730cc3be0d7628e392dd06b817f73</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/s11207-009-9374-1$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1007/s11207-009-9374-1$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>314,780,784,27923,27924,41487,42556,51318</link.rule.ids></links><search><creatorcontrib>Viswanathan, B.</creatorcontrib><creatorcontrib>Shanmugavel, R.</creatorcontrib><creatorcontrib>Bagare, S. 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P.</au><au>Rajamanickam, N.</au><au>Sriramachandran, P.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Identification of CrH and CrD Molecular Lines in the Sunspot Umbral Spectrum</atitle><jtitle>Solar physics</jtitle><stitle>Sol Phys</stitle><date>2009-07-01</date><risdate>2009</risdate><volume>257</volume><issue>2</issue><spage>261</spage><epage>269</epage><pages>261-269</pages><issn>0038-0938</issn><eissn>1573-093X</eissn><abstract>High-resolution Fourier transform spectrometer sunspot umbral spectra obtained at the National Solar Observatory/Kitt Peak were used to identify molecular rotational lines arising from the infrared band systems of CrH and CrD molecules. Measurement of the equivalent width used the Gaussian-profile approximation method, which is suitable especially for faint lines. Equivalent widths are measured for an adequate number of best lines of the A – X (0,0) band of CrH and the A – X (0,0;1,0) bands of CrD and, thereby, the effective rotational temperatures are estimated.</abstract><cop>Dordrecht</cop><pub>Springer Netherlands</pub><doi>10.1007/s11207-009-9374-1</doi><tpages>9</tpages></addata></record> |
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subjects | Approximation method Astrophysics Astrophysics and Astroparticles Atmospheric Sciences Fourier transforms Physics Physics and Astronomy Solar physics Space Exploration and Astronautics Space Sciences (including Extraterrestrial Physics Sunspots Temperature |
title | Identification of CrH and CrD Molecular Lines in the Sunspot Umbral Spectrum |
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