Show simple item record

Stable mid-latitude red arcs: Observations and theory

dc.contributor.authorRoble, Raymond Geralden_US
dc.contributor.authorNagy, Andrew F.en_US
dc.contributor.authorHays, Paul B. (Paul Byron)en_US
dc.date.accessioned2006-09-11T13:48:05Z
dc.date.available2006-09-11T13:48:05Z
dc.date.issued1970-12en_US
dc.identifier.citationNagy, A. F.; Roble, R. G.; Hays, P. B.; (1970). "Stable mid-latitude red arcs: Observations and theory." Space Science Reviews 11(5): 709-727. <http://hdl.handle.net/2027.42/43762>en_US
dc.identifier.issn0038-6308en_US
dc.identifier.issn1572-9672en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/43762
dc.description.abstractThe observational features of the arc are fairly well established. At present, the thermal conduction model appears to explain the red arc features most consistently, but it must be noted that a soft electron flux would give very similar results. Ion temperature measurements in the vicinity of an arc, which should be forthcoming in the very near future, can establish conclusively whether transverse electric fields play any important role in the formation of the arcs. Accepting the assumption that the arcs are the result of energy flowing down from the plasmasphere, the major remaining question is: where does the energy come from and how does it get into the plasmasphere? The various proposed mechanisms discussed in the previous chapter appear feasible, but much work needs to be done before this problem is completely resolved.en_US
dc.format.extent1104844 bytes
dc.format.extent3115 bytes
dc.format.mimetypeapplication/pdf
dc.format.mimetypetext/plain
dc.language.isoen_US
dc.publisherKluwer Academic Publishers; D. Reidel Publishing Company ; Springer Science+Business Mediaen_US
dc.subject.otherAstronomyen_US
dc.subject.otherPhysicsen_US
dc.titleStable mid-latitude red arcs: Observations and theoryen_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelAtmospheric, Oceanic and Space Sciencesen_US
dc.subject.hlbsecondlevelAerospace Engineeringen_US
dc.subject.hlbtoplevelScienceen_US
dc.subject.hlbtoplevelEngineeringen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumDept. of Aerospace Engineering, The University of Michigan, Ann Arbor, Mich., USAen_US
dc.contributor.affiliationotherDept. of Applied Physics and Information Science, The University of California at San Diego, La Jolla, Calif., USAen_US
dc.contributor.affiliationotherNational Center for Atmospheric Research, Boulder, Colo., USAen_US
dc.contributor.affiliationumcampusAnn Arboren_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/43762/1/11214_2004_Article_BF00177029.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1007/BF00177029en_US
dc.identifier.sourceSpace Science Reviewsen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


Files in this item

Show simple item record

Remediation of Harmful Language

The University of Michigan Library aims to describe library materials in a way that respects the people and communities who create, use, and are represented in our collections. Report harmful or offensive language in catalog records, finding aids, or elsewhere in our collections anonymously through our metadata feedback form. More information at Remediation of Harmful Language.

Accessibility

If you are unable to use this file in its current format, please select the Contact Us link and we can modify it to make it more accessible to you.