000 03848nam a22005537a 4500
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003 BD-SySUS
005 20160413122304.0
007 cr nn 008mamaa
008 130321s2013 xxu| s |||| 0|eng d
020 _a9781461463849
_9978-1-4614-6384-9
024 7 _a10.1007/978-1-4614-6384-9
_2doi
050 4 _aQB495-500.269
072 7 _aTTDS
_2bicssc
072 7 _aSCI005000
_2bisacsh
082 0 4 _a520
_223
082 0 4 _a500.5
_223
245 1 0 _aCross-Calibration of Far UV Spectra of Solar System Objects and the Heliosphere
_h[electronic resource] /
_cedited by Eric Quémerais, Martin Snow, Roger-Maurice Bonnet.
264 1 _aNew York, NY :
_bSpringer New York :
_bImprint: Springer,
_c2013.
300 _aVII, 275 p. 129 illus., 96 illus. in color.
_bonline resource.
336 _atext
_btxt
_2rdacontent
337 _acomputer
_bc
_2rdamedia
338 _aonline resource
_bcr
_2rdacarrier
347 _atext file
_bPDF
_2rda
490 1 _aISSI Scientific Report Series ;
_v13
505 0 _aDistribution of interstellar H atoms in the heliosphere and backscattered solar Lyman-α -- 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 Lyα 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.
520 _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.
650 0 _aPhysics.
650 0 _aObservations, Astronomical.
650 0 _aAstronomy
_xObservations.
650 0 _aSpace sciences.
650 0 _aSpectroscopy.
650 0 _aMicroscopy.
650 1 4 _aPhysics.
650 2 4 _aExtraterrestrial Physics, Space Sciences.
650 2 4 _aSpectroscopy and Microscopy.
650 2 4 _aAstronomy, Observations and Techniques.
700 1 _aQuémerais, Eric.
_eeditor.
700 1 _aSnow, Martin.
_eeditor.
700 1 _aBonnet, Roger-Maurice.
_eeditor.
710 2 _aSpringerLink (Online service)
773 0 _tSpringer eBooks
776 0 8 _iPrinted edition:
_z9781461463832
830 0 _aISSI Scientific Report Series ;
_v13
856 4 0 _uhttp://dx.doi.org/10.1007/978-1-4614-6384-9
912 _aZDB-2-PHA
942 _2Dewey Decimal Classification
_ceBooks
999 _c44623
_d44623