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Record ID harvard_bibliographic_metadata/ab.bib.13.20150123.full.mrc:942469794:1986
Source harvard_bibliographic_metadata
Download Link /show-records/harvard_bibliographic_metadata/ab.bib.13.20150123.full.mrc:942469794:1986?format=raw

LEADER: 01986nam a22004335a 4500
001 013832972-9
005 20131206194942.0
008 120330s1990 gw | s ||0| 0|eng d
020 $a9783642483752
020 $a9783642483752
020 $a9783642483776
024 7 $a10.1007/978-3-642-48375-2$2doi
035 $a(Springer)9783642483752
040 $aSpringer
050 4 $aQC801-809
072 7 $aPHVG$2bicssc
072 7 $aSCI032000$2bisacsh
082 04 $a550$223
082 04 $a526.1$223
100 1 $aJohnson, Robert E.,$eauthor.
245 10 $aEnergetic Charged-Particle Interactions with Atmospheres and Surfaces /$cby Robert E. Johnson.
264 1 $aBerlin, Heidelberg :$bSpringer Berlin Heidelberg,$c1990.
300 $aX, 232p. 84 illus.$bonline resource.
336 $atext$btxt$2rdacontent
337 $acomputer$bc$2rdamedia
338 $aonline resource$bcr$2rdacarrier
347 $atext file$bPDF$2rda
490 1 $aPhysics and Chemistry in Space Planetology,$x0079-1938 ;$v19
520 $aThe surfaces of interstellar and interplanetary grains, planetary satellites, ring particles, asteroids, Mercury and the Moon, etc. are all directly exposed to radiations. Solar wind, magnetospheric plasmas, cosmic rays, solar energetic particles, and U.V. photons can all produce chemical and physical alterations. These alterations affect the surface reflection properties and can eject species into the gas phase affecting the ambient gas and plasma. The physical processes involved are reviewed and the relevant data discussed. These are then applied to a number of outer solar system problems.
650 10 $aEarth sciences.
650 0 $aGeography.
650 0 $aPhysical geography.
650 0 $aAstrophysics.
650 24 $aGeophysics/Geodesy.
650 24 $aExtraterrestrial Physics, Space Sciences.
776 08 $iPrinted edition:$z9783642483776
830 0 $aPhysics and Chemistry in Space Planetology ;$v19.
988 $a20131114
906 $0VEN