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LEADER 00000cam  2200685Ki 4500 
001    832286146 
003    OCoLC 
005    20181130031636.1 
006    m     o  d         
007    cr cnu---unuuu 
008    130326s2013    nyua    ob    001 0 eng d 
019    889214735|a1058086979|a1066657329 
020    9781461463849|q(electronic bk.) 
020    146146384X|q(electronic bk.) 
020    |z9781461463832 
020    |z1461463831 
024 7  10.1007/978-1-4614-6384-9|2doi 
035    (OCoLC)832286146|z(OCoLC)889214735|z(OCoLC)1058086979
040    GW5XE|beng|epn|erda|cGW5XE|dYDXCP|dZMC|dCOO|dOCLCO|dSNK
049    MAIN 
050  4 QC459.5|b.C76 2013 
072  7 SCI005000|2bisacsh 
072  7 NAT|x033000|2bisacsh 
072  7 TTDS|2bicssc 
082 04 522.68|223 
245 00 Cross-calibration of far UV spectra of solar system 
       objects and the heliosphere /|cedited by Eric Quemerais, 
       Martin Snow, Roger-Maurice Bonnet. 
264  1 New York :|bSpringer,|c2013. 
300    1 online resource :|billustrations. 
336    text|btxt|2rdacontent 
337    computer|bc|2rdamedia 
338    online resource|bcr|2rdacarrier 
340    |gpolychrome|2rdacc|0
347    text file|2rdaft|0
490 1  ISSI scientific report series ;|vv. 13 
500    Includes index. 
504    Includes bibliographical references and index. 
505 0  |6880-01|aDistribution of interstellar H atoms in the 
       heliosphere and backscattered solar Lyman-₀ -- 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 Ly₀ 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    This 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. 
546    English. 
588 0  Print version record. 
650  0 Far ultraviolet detectors.|0
650  0 Stars|xSpectra.|0
650  0 Astronomical instruments|0
650 14 Physics. 
650 24 Extraterrestrial Physics, Space Sciences. 
650 24 Spectroscopy and Microscopy. 
650 24 Astronomy, Observations and Techniques. 
655  4 Electronic books. 
700 1  Quémerais, Eric.|0
700 1  Snow, Martin.|0
700 1  Bonnet, R.-M.|q(Roger-M.),|0
776 08 |iPrint version:|tCross-calibration of far UV spectra of 
       solar system objects and the heliosphere|z9781461463832
830  0 ISSI scientific report series ;|0
       authorities/names/no2013045021|vv. 13. 
880 00 |6505-01/(S|tInterstellar Hydrogen and the Sun --
       |tDistribution of Interstellar Hydrogen Atoms in the 
       Heliosphere and Backscattered Solar Lyman-α /|rVladislav 
       V. Izmodenov, Olga A. Katushkina, Eric Quemerais, Maciej 
       Bzowski --|tSolar Parameters for Modeling the 
       Interplanetary Background /|rMaciej Bzowski, Justyna M. 
       Soko, Munetoshi Tokumaru, Kenichi Fujiki, Eric Quemerais -
       -|tInterplanetary Hydrogen --|tThirty Years of 
       Interplanetary Background Data: A Global View /|rEric 
       Quemerais, Bill R. Sandel, Vladislav V. Izmodenov, G. 
       Randall Gladstone --|tLyman-α Models for LRO LAMP from 
       MESSENGER MASCS and SOHO SWAN Data /|rWayne R. Pryor, 
       Gregory M. Holsclaw, William E. McClintock, Martin Snow --
       |tNew Horizons Cruise Observations of Lyman-α Emissions 
       from the Interplanetary Medium /|rG. Randall Gladstone, S.
       Alan Stern, Wayne R. Pryor --|tInstrument Cross-
       Calibration --|tA New Catalog of Ultraviolet Stellar 
       Spectra for Calibration /|rMartin Snow, Aurelie Reberac, 
       Eric Quemerais, John Clarke, W.E. McClintock --|tAbsolute 
       Ultraviolet Irradiance of the Moon from the LASP Lunar 
       Albedo Measurement and Analysis from SOLSTICE (LLAMAS) 
       Project /|rMartin Snow, Gregory M. Holsclaw, William E. 
       McClintock, Tom Woods --|tLyman-α Observations of Comet 
       Holmes from SORCE SOLSTICE and SOHO SWAN /|rWayne R. Pryor,
       Martin Snow, Eric Quemerais, Stephane Ferron. 
990    SpringerLink|bSpringer English/International eBooks 2013 -
       Full Set|c2018-11-30|yMaster record variable field(s) 
       change: 650|5OH1 
990    SpringerLink|bSpringer English/International eBooks 2013 -
       Full Set|c2018-10-31|yNew collection 
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