Implications of a weak termination shock
dc.contributor.author | Fisk, Lennard A. | en_US |
dc.date.accessioned | 2006-09-11T13:49:36Z | |
dc.date.available | 2006-09-11T13:49:36Z | |
dc.date.issued | 1996-10 | en_US |
dc.identifier.citation | Fisk, L. A.; (1996). "Implications of a weak termination shock." Space Science Reviews 78 (1-2): 129-136. <http://hdl.handle.net/2027.42/43779> | en_US |
dc.identifier.issn | 0038-6308 | en_US |
dc.identifier.issn | 1572-9672 | en_US |
dc.identifier.uri | https://hdl.handle.net/2027.42/43779 | |
dc.description.abstract | Recent observations from the Voyager spacecraft have suggested that the spectrum of the anomalous cosmic ray component is relatively steep at the termination shock, which is believed to be responsible for accelerating these particles. This conclusion argues that the termination shock must be weak, which in turn requires that the upstream Mach number in the solar wind must be quite low, ∼2.4. It is pointed out that such conditions are unlikely to prevail at all locations along the shock front. However, it is possible for such conditions to exist at the interface between high speed streams at high heliographic latitudes and the region at low latitudes where high and low speed streams have interacted and come into equilibrium. This discussion suggests a preferred location for the injection of the anomalous component into the shock acceleration process. | en_US |
dc.format.extent | 571513 bytes | |
dc.format.extent | 3115 bytes | |
dc.format.mimetype | application/pdf | |
dc.format.mimetype | text/plain | |
dc.language.iso | en_US | |
dc.publisher | Kluwer Academic Publishers; Springer Science+Business Media | en_US |
dc.subject.other | Physics | en_US |
dc.subject.other | Astronomy | en_US |
dc.subject.other | Anomalous Cosmic Rays | en_US |
dc.subject.other | Solar Wind | en_US |
dc.subject.other | Termination Shock | en_US |
dc.title | Implications of a weak termination shock | en_US |
dc.type | Article | en_US |
dc.subject.hlbsecondlevel | Atmospheric, Oceanic and Space Sciences | en_US |
dc.subject.hlbsecondlevel | Aerospace Engineering | en_US |
dc.subject.hlbtoplevel | Engineering | en_US |
dc.subject.hlbtoplevel | Science | en_US |
dc.description.peerreviewed | Peer Reviewed | en_US |
dc.contributor.affiliationum | Department of Atmospheric, Oceanic, and Space Sciences, University of Michigan, 48109-2143, Ann Arbor, Ml, USA | en_US |
dc.contributor.affiliationumcampus | Ann Arbor | en_US |
dc.description.bitstreamurl | http://deepblue.lib.umich.edu/bitstream/2027.42/43779/1/11214_2004_Article_BF00170799.pdf | en_US |
dc.identifier.doi | http://dx.doi.org/10.1007/BF00170799 | en_US |
dc.identifier.source | Space Science Reviews | en_US |
dc.owningcollname | Interdisciplinary and Peer-Reviewed |
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