Manganese and carbon lines as temperature indicators
dc.contributor.author | Elste, G. H. | en_US |
dc.date.accessioned | 2006-09-11T13:43:02Z | |
dc.date.available | 2006-09-11T13:43:02Z | |
dc.date.issued | 1986-03 | en_US |
dc.identifier.citation | Elste, G.; (1986). "Manganese and carbon lines as temperature indicators." Solar Physics 107(1): 47-56. <http://hdl.handle.net/2027.42/43705> | en_US |
dc.identifier.issn | 0038-0938 | en_US |
dc.identifier.issn | 1573-093X | en_US |
dc.identifier.uri | https://hdl.handle.net/2027.42/43705 | |
dc.description.abstract | Selected hyperfine structure broadened lines of various excitations and the carbon line at 5380 Å are tested as temperature diagnostics for photospheric heterogeneities. This is done by comparing the observed center-to-limb variation of the equivalent widths of these lines with predictions by several proposed models of homogeneous type. Model 10 (Elste, 1968), which also explains the limb-darkening of the continuum in the same spectral range, provides a better basis for the analysis of heterogeneities at different photospheric levels than other recent reference models. | en_US |
dc.format.extent | 572126 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; D. Reidel Publishing Company ; Springer Science+Business Media | en_US |
dc.subject.other | Physics | en_US |
dc.subject.other | Astrophysics | en_US |
dc.title | Manganese and carbon lines as temperature indicators | en_US |
dc.type | Article | 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 | Department of Astronomy, University of Michigan, 48109, Ann Arbor, MI, U.S.A. | en_US |
dc.contributor.affiliationumcampus | Ann Arbor | en_US |
dc.description.bitstreamurl | http://deepblue.lib.umich.edu/bitstream/2027.42/43705/1/11207_2004_Article_BF00155340.pdf | en_US |
dc.identifier.doi | http://dx.doi.org/10.1007/BF00155340 | en_US |
dc.identifier.source | Solar Physics | en_US |
dc.owningcollname | Interdisciplinary and Peer-Reviewed |
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