View Item 

Show simple item record

Solar soft X-rays and solar activity
dc.contributor.authorTeske, Richard G.en_US
dc.contributor.authorThomas, Roger Jerryen_US
dc.date.accessioned2006-09-11T13:47:21Z
dc.date.available2006-09-11T13:47:21Z
dc.date.issued1969-08en_US
dc.identifier.citationTeske, Richard G.; Thomas, Roger J.; (1969). "Solar soft X-rays and solar activity." Solar Physics 8(2): 348-368. <http://hdl.handle.net/2027.42/43754>en_US
dc.identifier.issn0038-0938en_US
dc.identifier.issn1573-093Xen_US
dc.identifier.urihttps://hdl.handle.net/2027.42/43754
dc.description.abstractSoft solar X-rays (8 ⩽ gl ⩽ 12 Å) were observed from OSO-III. An analysis of the X-ray enhancements associated with 165 solar flares revealed that there is a tendency for a weak soft X-ray enhancement to precede the cm- λ burst and H α flare. The peak soft X-ray flux follows the cm- λ peak by about 4 min, on the average. Additionally, it was found that flare-rich active centers tend to produce flares which are stronger X-ray and cm- λ emitters than are flares which take place in flare-poor active centers.en_US
dc.format.extent1111899 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.titleSolar soft X-rays and solar activityen_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelAtmospheric, Oceanic and Space Sciencesen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumDept. of Astronomy and the McMath-Hulbert Observatory, The University of Michigan, Ann Arbor, Mich., U.S.A.en_US
dc.contributor.affiliationumDept. of Astronomy and the McMath-Hulbert Observatory, The University of Michigan, Ann Arbor, Mich., U.S.A.en_US
dc.contributor.affiliationumcampusAnn Arboren_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/43754/1/11207_2004_Article_BF00155382.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1007/BF00155382en_US
dc.identifier.sourceSolar Physicsen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


Files in this item

Name:
11207_2004_Article_BF00155382.pdf
Size:
1.060MB
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.