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dc.contributor.authorUgolnikov, O. S.en
dc.contributor.authorPunanova, A. F.en
dc.contributor.authorKrushinsky, V. V.en
dc.date.accessioned2014-11-29T19:47:57Z-
dc.date.available2014-11-29T19:47:57Z-
dc.date.issued2013-
dc.identifier.citationUgolnikov O. S. Trajectory retrieval and component investigations of the southern polar stratosphere based on high-resolution spectroscopy of the totally eclipsed moon surface / O. S. Ugolnikov, A. F. Punanova, V. V. Krushinsky // Journal of Quantitative Spectroscopy and Radiative Transfer. — 2013. — Vol. 116. — P. 67-74.en
dc.identifier.issn0022-4073-
dc.identifier.other1good_DOI
dc.identifier.other4a499914-580f-4a19-9138-2addeeeafbd7pure_uuid
dc.identifier.otherhttp://www.scopus.com/inward/record.url?partnerID=8YFLogxK&scp=84871873296m
dc.identifier.urihttp://elar.urfu.ru/handle/10995/27529-
dc.description.abstractIn this paper we present the high-resolution spectral observations of the fragment of lunar surface during the total lunar eclipse of December 10, 2011. The observations were carried out with the fiber-fed echelle spectrograph at the 1.2-m telescope in Kourovka Astronomical observatory (Ural mountains, central Russia). The observed radiation is transmitted by tangent trajectory through the southern polar stratosphere before the reflection from the Moon and the spectra contain a number of absorption bands of atmospheric gases (O2, O3, O4, NO2, H2O). High-resolution analysis of three O2 bands and O4 absorption effects is used to trace the effective trajectory of solar emission through the stratosphere and to detect the contribution of scattered light. Bands of other gases allow us to measure their abundances along the trajectory. © 2012 Elsevier Ltd.en
dc.format.mimetypeapplication/pdfen
dc.language.isoenen
dc.sourceJournal of Quantitative Spectroscopy and Radiative Transferen
dc.subjectHIGH-RESOLUTION SPECTROSCOPYen
dc.subjectLUNAR ECLIPSEen
dc.subjectOZONEen
dc.subjectSTRATOSPHEREen
dc.subjectWATER VAPORen
dc.subjectABSORPTION EFFECTSen
dc.subjectASTRONOMICAL OBSERVATORIESen
dc.subjectECHELLE SPECTROGRAPHen
dc.subjectHIGH RESOLUTIONen
dc.subjectHIGH RESOLUTION ANALYSISen
dc.subjectHIGH-RESOLUTION SPECTROSCOPYen
dc.subjectLUNAR ECLIPSEen
dc.subjectLUNAR SURFACEen
dc.subjectMOON SURFACEen
dc.subjectPOLAR STRATOSPHEREen
dc.subjectSOLAR EMISSIONen
dc.subjectSPECTRAL OBSERVATIONSen
dc.subjectOZONEen
dc.subjectSPECTROSCOPIC ANALYSISen
dc.subjectTRACE ANALYSISen
dc.subjectTRAJECTORIESen
dc.subjectUPPER ATMOSPHEREen
dc.subjectWATER VAPORen
dc.subjectMOONen
dc.subjectABSORPTIONen
dc.subjectDETECTION METHODen
dc.subjectLIGHT SCATTERINGen
dc.subjectOBSERVATIONAL METHODen
dc.subjectRADIATIVE TRANSFERen
dc.subjectSPECTRAL RESOLUTIONen
dc.subjectSTRATOSPHEREen
dc.titleTrajectory retrieval and component investigations of the southern polar stratosphere based on high-resolution spectroscopy of the totally eclipsed moon surfaceen
dc.typeArticleen
dc.typeinfo:eu-repo/semantics/publishedVersionen
dc.typeinfo:eu-repo/semantics/articleen
dc.identifier.doi10.1016/j.jqsrt.2012.11.013-
dc.identifier.scopus84871873296-
local.affiliationSpace Research Institute, Russian Academy of Sciences, Profsoyuznaya st., 84/32, Moscow, 117997, Russian Federationen
local.affiliationKourovka Astronomical Observatory, Ural Federal University, Lenina st., 51, Ekaterinburg, 620000, Russian Federationen
local.contributor.employeeПунанова Анна Федоровнаru
local.contributor.employeeКрушинский Вадим Владимировичru
local.description.firstpage67-
local.description.lastpage74-
local.volume116-
dc.identifier.wos000314430400007-
local.contributor.departmentИнститут естественных наук и математикиru
local.identifier.pure903641-
local.identifier.eid2-s2.0-84871873296-
local.identifier.wosWOS:000314430400007-
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