View Item 

Show simple item record

Observations of the infrared triplet of singly ionized calcium

dc.contributor.authorLinsky, Jeffrey L.en_US
dc.contributor.authorTeske, Richard G.en_US
dc.contributor.authorWilkinson, Carol W.en_US
dc.date.accessioned2006-09-11T13:43:08Z
dc.date.available2006-09-11T13:43:08Z
dc.date.issued1970-03en_US
dc.identifier.citationLinsky, Jeffrey L.; Teske, Richard G.; Wilkinson, Carol W.; (1970). "Observations of the infrared triplet of singly ionized calcium." Solar Physics 11(3): 374-383. <http://hdl.handle.net/2027.42/43706>en_US
dc.identifier.issn0038-0938en_US
dc.identifier.issn1573-093Xen_US
dc.identifier.urihttps://hdl.handle.net/2027.42/43706
dc.description.abstractObservations are presented of the Ca ii infrared triplet (8498 Å, 8542 Å, and 8662 Å) at three positions on the solar disk to make possible direct analyses of the lines and comparisons with theoretical computations. The source functions for the two strongest lines (8542 Å and 8662 Å) are equal at those heights corresponding to the wings of the lines (¦Δλ¦ > 0.4 Å) but not to those of the cores. We suggest that the apparent source function inequality in the cores is due to limb darkening caused by inhomogeneities in the chromosphere.en_US
dc.format.extent587805 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.otherPhysicsen_US
dc.subject.otherAstrophysicsen_US
dc.titleObservations of the infrared triplet of singly ionized calciumen_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelAtmospheric, Oceanic and Space Sciencesen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumDepartment of Astronomy, University of Michigan, Ann Arbor, Mich., U. S. A.en_US
dc.contributor.affiliationotherJoint Institute for Laboratory Astrophysics, University of Colorado, Boulder, Colo., U. S. A.en_US
dc.contributor.affiliationotherHarvard College Observatory, Cambridge, Mass., U. S. A.en_US
dc.contributor.affiliationumcampusAnn Arboren_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/43706/1/11207_2004_Article_BF00153072.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1007/BF00153072en_US
dc.identifier.sourceSolar Physicsen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


Files in this item

Name:
11207_2004_Article_BF00153072.pdf
Size:
574.0KB
Format:
PDF
View/Open

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.