LEADER 04146nam 22006495 450 001 9910438117103321 005 20230810160735.0 010 $a1-4614-6384-X 024 7 $a10.1007/978-1-4614-6384-9 035 $a(CKB)3460000000120297 035 $a(EBL)1205311 035 $a(SSID)ssj0000878696 035 $a(PQKBManifestationID)11514894 035 $a(PQKBTitleCode)TC0000878696 035 $a(PQKBWorkID)10837381 035 $a(PQKB)11120779 035 $a(DE-He213)978-1-4614-6384-9 035 $a(MiAaPQ)EBC1205311 035 $a(PPN)169136175 035 $a(EXLCZ)993460000000120297 100 $a20130321d2013 u| 0 101 0 $aeng 135 $aur|n|---||||| 181 $ctxt 182 $cc 183 $acr 200 10$aCross-Calibration of Far UV Spectra of Solar System Objects and the Heliosphere /$fedited by Eric Quémerais, Martin Snow, Roger-Maurice Bonnet 205 $a1st ed. 2013. 210 1$aNew York, NY :$cSpringer New York :$cImprint: Springer,$d2013. 215 $a1 online resource (275 p.) 225 1 $aISSI Scientific Report Series ;$v13 300 $aDescription based upon print version of record. 311 $a1-4614-6383-1 320 $aIncludes bibliographical references and index. 327 $aDistribution of interstellar H atoms in the heliosphere and backscattered solar Lyman-? -- Solar parameters for modeling interplanetary background -- 30 Years of Interplanetary Background Data: A Global View -- Lyman-alpha Models from Messenger and SOHO data -- New Horizons Cruise Observations of Ly? Emissions from the Interplanetary Medium -- A New Catalog of Ultraviolet Stellar Spectra -- Absolute Ultraviolet Irradiance of the Moon from SORCE SOLSTICE -- Lyman-alpha Observations of Comet Holmes from SORCE SOLSTICE and SOHO SWAN. 330 $aThis book is the result of a working group sponsored by ISSI in Bern, which was initially created to study possible ways to calibrate a Far Ultraviolet (FUV) instrument after launch. In most cases, ultraviolet instruments are well calibrated on the ground, but unfortunately, optics and detectors in the FUV are very sensitive to contaminants and it is very challenging to prevent contamination before and during the test and launch sequences of a space mission. Therefore, ground calibrations need to be confirmed after launch and it is necessary to keep track of the temporal evolution of the sensitivity of the instrument during the mission. The studies presented here cover various fields of FUV spectroscopy with the exclusion of direct solar UV spectroscopy, including a catalog of stellar spectra, data-sets of lunar Irradiance, observations of comets and measurements of the interplanetary background. Detailed modeling of the interplanetary background is presented as well. This work also includes comparisons of older data-sets with current ones. This raises the question of the consistency of the existing data-sets. Previous experiments have been calibrated independently and comparison of the data-sets may lead to inconsistencies. The authors have tried to check that possibility in the data-sets and when relevant, suggest a correction factor for the corresponding data. 410 0$aISSI Scientific Report Series ;$v13 606 $aSolar system 606 $aSpectrum analysis 606 $aAstronomy$xObservations 606 $aSpace Physics 606 $aSpectroscopy 606 $aAstronomy, Observations and Techniques 615 0$aSolar system. 615 0$aSpectrum analysis. 615 0$aAstronomy$xObservations. 615 14$aSpace Physics. 615 24$aSpectroscopy. 615 24$aAstronomy, Observations and Techniques. 676 $a522.68 702 $aQuémerais$b Eric$4edt$4http://id.loc.gov/vocabulary/relators/edt 702 $aSnow$b Martin$4edt$4http://id.loc.gov/vocabulary/relators/edt 702 $aBonnet$b Roger-Maurice$4edt$4http://id.loc.gov/vocabulary/relators/edt 906 $aBOOK 912 $a9910438117103321 996 $aCross-Calibration of Far UV Spectra of Solar System Objects and the Heliosphere$92108086 997 $aUNINA