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An explanation for strongly underwound magnetic field in co‐rotating rarefaction regions and its relationship to footpoint motion on the the sun

dc.contributor.authorSchwadron, N. A.en_US
dc.date.accessioned2013-01-03T19:38:36Z
dc.date.available2013-01-03T19:38:36Z
dc.date.issued2002-07en_US
dc.identifier.citationSchwadron, N. A. (2002). "An explanation for strongly underwound magnetic field in co‐rotating rarefaction regions and its relationship to footpoint motion on the the sun." Geophysical Research Letters 29(14): 8-1-8-4. <http://hdl.handle.net/2027.42/94855>en_US
dc.identifier.issn0094-8276en_US
dc.identifier.issn1944-8007en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/94855
dc.publisherWiley Periodicals, Inc.en_US
dc.titleAn explanation for strongly underwound magnetic field in co‐rotating rarefaction regions and its relationship to footpoint motion on the the sunen_US
dc.typeArticleen_US
dc.rights.robotsIndexNoFollowen_US
dc.subject.hlbsecondlevelGeological Sciencesen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumAlso at Department of Atmospheric, Oceanic and Space Science, The University of Michigan, Ann Arbor, USA.en_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/94855/1/grl15835.pdf
dc.identifier.doi10.1029/2002GL015028en_US
dc.identifier.sourceGeophysical Research Lettersen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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