Soft solar X-rays and solar activity
dc.contributor.author | Teske, Richard G. | en_US |
dc.date.accessioned | 2006-09-11T13:44:18Z | |
dc.date.available | 2006-09-11T13:44:18Z | |
dc.date.issued | 1971-12 | en_US |
dc.identifier.citation | Teske, Richard G.; (1971). "Soft solar X-rays and solar activity." Solar Physics 21(1): 146-156. <http://hdl.handle.net/2027.42/43719> | en_US |
dc.identifier.issn | 1573-093X | en_US |
dc.identifier.issn | 0038-0938 | en_US |
dc.identifier.uri | https://hdl.handle.net/2027.42/43719 | |
dc.description.abstract | Minor Hα activity, consisting of small brightenings and small, surgelike spikes, was observed to take place above an active center at the solar limb in good time-association with small fluctuations in the soft X-ray background flux, suggesting that even small dynamical events seen optically are associated with coronal heating. The ratio of Hα flux to soft X-ray flux in some of the surges was approximately the same as the ratio already established for flares. The total energy dissipated by the events in a 24-hour period is estimated; it is approximately equivalent to that released by one flare of imp 1 per day. | en_US |
dc.format.extent | 1113833 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 | Soft solar X-rays and solar activity | 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 and the McMath-Hulbert Observatory, The University of Michigan, Ann Arbor, Mich., U.S.A. | en_US |
dc.contributor.affiliationumcampus | Ann Arbor | en_US |
dc.description.bitstreamurl | http://deepblue.lib.umich.edu/bitstream/2027.42/43719/1/11207_2004_Article_BF00155785.pdf | en_US |
dc.identifier.doi | http://dx.doi.org/10.1007/BF00155785 | en_US |
dc.identifier.source | Solar Physics | en_US |
dc.owningcollname | Interdisciplinary and Peer-Reviewed |
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