| Record ID | ia:collectiondesmm28fragoog |
| Source | Internet Archive |
| Download MARC XML | https://archive.org/download/collectiondesmm28fragoog/collectiondesmm28fragoog_marc.xml |
| Download MARC binary | https://www.archive.org/download/collectiondesmm28fragoog/collectiondesmm28fragoog_meta.mrc |
LEADER: 01811ctm 2200421Ii 4500
001 ocm04124048
003 OCoLC
005 20211108003959.0
008 780809s1975 xx a rbm 000 0 eng d
040 $aIRU$beng$epn$cIRU$dOCL$dOCLCQ$dOCLCF$dOCLCQ$dOCLCO$dOCLCQ$dOCLCO$dOCL
035 $a(OCoLC)4124048
043 $azju----
050 4 $aQB661$b.O78 1975a
100 1 $aOrton, Glenn Scott,$d1948-
245 10 $a1. Spatially resolved absolute spectral reflectivity of Jupiter: 3390-8400 angstroms. :$b2. The Jovian thermal structure from Pioneer 10 infrared radiometer data. 3. Observations and analysis of 8-14 micron thermal emission of Jupiter: a model of thermal structure and cloud properties /$cby Glenn Scott Orton.
246 3 $aThermal structure and cloud properties
246 3 $aSpatially resolved absolute spectral reflectivity of Jupiter : 3390-8400 angstroms
264 0 $c1975.
300 $axvii, 170 leaves :$billustrations
336 $atext$btxt$2rdacontent
337 $aunmediated$bn$2rdamedia
338 $avolume$bnc$2rdacarrier
500 $aOn spine: Thermal structure and cloud properties.
502 $cCalifornia Institute of Technology
504 $aIncludes bibliographical references (leaves 166-170).
500 $aTypescript.
533 $aPrint reproduction.
651 0 $aJupiter (Planet)$xRadiation.
650 0 $aPlanets$xSpectra.
650 0 $aRadiometers.
650 7 $aPlanets$xSpectra.$2fast$0(OCoLC)fst01065168
650 7 $aPlanets$xRadiation.$2fast$0(OCoLC)fst02003734
650 7 $aRadiometers.$2fast$0(OCoLC)fst01088310
651 7 $aJupiter (Planet)$2fast$0(OCoLC)fst01244812
655 7 $aAcademic theses.$2fast$0(OCoLC)fst01726453
655 7 $aAcademic theses.$2lcgft
994 $aZ0$bP4A
948 $hNO HOLDINGS IN P4A - 1 OTHER HOLDINGS