Non-thermal O(1D) produced by dissociative recombination of O2+: A theoretical model and observational results
dc.contributor.author | Schmitt, G. A. | en_US |
dc.contributor.author | Abreu, Vincent J. | en_US |
dc.contributor.author | Hays, Paul B. (Paul Byron) | en_US |
dc.date.accessioned | 2006-04-07T18:01:46Z | |
dc.date.available | 2006-04-07T18:01:46Z | |
dc.date.issued | 1981-10 | en_US |
dc.identifier.citation | Schmitt, G. A., Abreu, V. J., Hays, P. B. (1981/10)."Non-thermal O(1D) produced by dissociative recombination of O2+: A theoretical model and observational results." Planetary and Space Science 29(10): 1095-1099. <http://hdl.handle.net/2027.42/24250> | en_US |
dc.identifier.uri | http://www.sciencedirect.com/science/article/B6V6T-46YJGJS-1G/2/4dcf6c54804d74df4b954f952950aded | en_US |
dc.identifier.uri | https://hdl.handle.net/2027.42/24250 | |
dc.description.abstract | Thermal and non-thermal O(1D) number density profiles are calculated. The two populations are assumed to be coupled by a thermalization cross-section which determines the loss and production in the non-thermal and thermal populations, respectively. The sources, sinks and transport of the two populations are used to model volume emission rate profiles at 6300 A. The 6300 A brightness measured by the Visible Airglow Experiment is then used to establish the presence of the non-thermal population and to determine the thermalization cross-section. | en_US |
dc.format.extent | 436319 bytes | |
dc.format.extent | 3118 bytes | |
dc.format.mimetype | application/pdf | |
dc.format.mimetype | text/plain | |
dc.language.iso | en_US | |
dc.publisher | Elsevier | en_US |
dc.title | Non-thermal O(1D) produced by dissociative recombination of O2+: A theoretical model and observational results | en_US |
dc.type | Article | en_US |
dc.rights.robots | IndexNoFollow | en_US |
dc.subject.hlbsecondlevel | Atmospheric, Oceanic and Space Sciences | en_US |
dc.subject.hlbtoplevel | Science | en_US |
dc.description.peerreviewed | Peer Reviewed | en_US |
dc.contributor.affiliationum | Space Physics Research Laboratory, The University of Michigan, Department of Atmospheric and Oceanic Science, Ann Arbor, MI 48109, U.S.A. | en_US |
dc.contributor.affiliationum | Space Physics Research Laboratory, The University of Michigan, Department of Atmospheric and Oceanic Science, Ann Arbor, MI 48109, U.S.A. | en_US |
dc.contributor.affiliationum | Space Physics Research Laboratory, The University of Michigan, Department of Atmospheric and Oceanic Science, Ann Arbor, MI 48109, U.S.A. | en_US |
dc.description.bitstreamurl | http://deepblue.lib.umich.edu/bitstream/2027.42/24250/1/0000513.pdf | en_US |
dc.identifier.doi | http://dx.doi.org/10.1016/0032-0633(81)90008-8 | en_US |
dc.identifier.source | Planetary and Space Science | en_US |
dc.owningcollname | Interdisciplinary and Peer-Reviewed |
Files in this item
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.