Heliographic longitude distribution of the flares associated with type III bursts observed at kilometric wavelengths
dc.contributor.author | Alvarez, Hector | en_US |
dc.contributor.author | Potter, William H. | en_US |
dc.contributor.author | Haddock, Fred T. | en_US |
dc.date.accessioned | 2006-09-11T13:45:24Z | |
dc.date.available | 2006-09-11T13:45:24Z | |
dc.date.issued | 1973-08 | en_US |
dc.identifier.citation | Alvarez, Hector; Haddock, Fred T.; Potter, William H.; (1973). "Heliographic longitude distribution of the flares associated with type III bursts observed at kilometric wavelengths." Solar Physics 31(2): 493-500. <http://hdl.handle.net/2027.42/43732> | en_US |
dc.identifier.issn | 0038-0938 | en_US |
dc.identifier.issn | 1573-093X | en_US |
dc.identifier.uri | https://hdl.handle.net/2027.42/43732 | |
dc.description.abstract | We have grouped observed type III solar bursts according to the discrete frequencies of observation in the kilometric wavelength range. For each group we have obtained the bursts' frequency of occurrence as a function of the heliographic longitude of the associated optical flares. We found that flares occurring east of a certain cutoff longitude do not produce bursts observable near the earth below a given frequency. The cutoff on the west is determined by observational limitation for flares beyond the limb. The mean longitude and the extreme eastern end of the longitude distribution both shift to the west as the radio frequency decreases. We interpret these findings in terms of radio wave propagation effects and curved trajectories of the bursts' exciter particles. | en_US |
dc.format.extent | 378807 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 | Heliographic longitude distribution of the flares associated with type III bursts observed at kilometric wavelengths | 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 | Radio Astronomy Observatory, University of Michigan, 48104, Ann Arbor, Mich., U.S.A. | en_US |
dc.contributor.affiliationum | Radio Astronomy Observatory, University of Michigan, 48104, Ann Arbor, Mich., U.S.A. | en_US |
dc.contributor.affiliationum | Radio Astronomy Observatory, University of Michigan, 48104, Ann Arbor, Mich., U.S.A. | en_US |
dc.contributor.affiliationumcampus | Ann Arbor | en_US |
dc.description.bitstreamurl | http://deepblue.lib.umich.edu/bitstream/2027.42/43732/1/11207_2004_Article_BF00152824.pdf | en_US |
dc.identifier.doi | http://dx.doi.org/10.1007/BF00152824 | en_US |
dc.identifier.source | Solar Physics | en_US |
dc.owningcollname | Interdisciplinary and Peer-Reviewed |
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