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Photoelectron energy losses to thermal electrons

dc.contributor.authorSchunk, Robert W.en_US
dc.contributor.authorHays, Paul B. (Paul Byron)en_US
dc.date.accessioned2006-04-17T16:30:43Z
dc.date.available2006-04-17T16:30:43Z
dc.date.issued1971-01en_US
dc.identifier.citationSchunk, Robert W., Hays, Paul B. (1971/01)."Photoelectron energy losses to thermal electrons." Planetary and Space Science 19(1): 113-117. <http://hdl.handle.net/2027.42/33734>en_US
dc.identifier.urihttp://www.sciencedirect.com/science/article/B6V6T-46YM42M-WJ/2/9a44d8748ebe77ff229ea54883eabad0en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/33734
dc.description.abstractThe photoelectron energy loss rate to the ambient electrons is discussed. It is shown that the conventional Butler and Buckingham expression has been incorrectly applied in photoelectron calculations. The appropriate energy loss rates are indicated. It is also shown that the geomagnetic field has little influence on the photoelectron energy loss rate.en_US
dc.format.extent363155 bytes
dc.format.extent3118 bytes
dc.format.mimetypeapplication/pdf
dc.format.mimetypetext/plain
dc.language.isoen_US
dc.publisherElsevieren_US
dc.titlePhotoelectron energy losses to thermal electronsen_US
dc.typeArticleen_US
dc.rights.robotsIndexNoFollowen_US
dc.subject.hlbsecondlevelAtmospheric, Oceanic and Space Sciencesen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumUniversity of Michigan, Ann Arbor, Mich. 48105, U.S.A.en_US
dc.contributor.affiliationumUniversity of Michigan, Ann Arbor, Mich. 48105, U.S.A.en_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/33734/1/0000248.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1016/0032-0633(71)90071-7en_US
dc.identifier.sourcePlanetary and Space Scienceen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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