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Global heat flow: A new look

dc.contributor.authorChapman, David S.en_US
dc.contributor.authorPollack, Henry N.en_US
dc.date.accessioned2006-04-07T16:34:21Z
dc.date.available2006-04-07T16:34:21Z
dc.date.issued1975-11en_US
dc.identifier.citationChapman, David S., Pollack, Henry N. (1975/11)."Global heat flow: A new look." Earth and Planetary Science Letters 28(1): 23-32. <http://hdl.handle.net/2027.42/21952>en_US
dc.identifier.urihttp://www.sciencedirect.com/science/article/B6V61-473FF75-17/2/13afe56db5facbbc00fbd59469318985en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/21952
dc.description.abstractA global heat flow map has been derived from existing observations supplemented in areas without data by an empirical predictor based on tectonic setting and age. In continental areas the predictor is based on the observed correlation of heat flow with age of last tectono-thermal event, and in oceanic regions on the observed relation of heat flow to age of ocean floor. The predictor was used to assign mean heat flow values to 5[deg] x 5[deg] grid areas on the globe, weighted according to the relative area of tectonic provinces represented. A spherical harmonic analysis to degree 12 of the heat flow field yields a mean value of 59 mW m-2, a rms residual of 13 mW m-2, and an amplitude spectrum which decreases gradually and almost monotonically from n = 1. The spherical harmonic representation of the heat flow field is free of the unreal distortions which have characterized earlier analyses based on a geographically sparse data set. Areas with residuals greater than 15 mW m-2 comprise less than 19% of the area of the globe, thus indicating that most heat flow provinces have characteristic dimensions adequately represented in a 12-degree analysis.en_US
dc.format.extent703933 bytes
dc.format.extent3118 bytes
dc.format.mimetypeapplication/pdf
dc.format.mimetypetext/plain
dc.language.isoen_US
dc.publisherElsevieren_US
dc.titleGlobal heat flow: A new looken_US
dc.typeArticleen_US
dc.rights.robotsIndexNoFollowen_US
dc.subject.hlbsecondlevelGeology and Earth Sciencesen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumDepartment of Geology and Mineralogy, The University of Michigan, Ann Arbor, Mich., USAen_US
dc.contributor.affiliationumDepartment of Geology and Mineralogy, The University of Michigan, Ann Arbor, Mich., USAen_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/21952/1/0000361.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1016/0012-821X(75)90069-2en_US
dc.identifier.sourceEarth and Planetary Science Lettersen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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