Transition probabilities in highly ionized p2 and p4 configurations
dc.contributor.author | Malville, J. Mc Kim | en_US |
dc.contributor.author | Berger, Richard A. | en_US |
dc.date.accessioned | 2006-04-13T14:40:25Z | |
dc.date.available | 2006-04-13T14:40:25Z | |
dc.date.issued | 1965-11 | en_US |
dc.identifier.citation | Malville, J. McKim, Berger, Richard A. (1965/11)."Transition probabilities in highly ionized p2 and p4 configurations." Planetary and Space Science 13(11): 1131-1136. <http://hdl.handle.net/2027.42/31969> | en_US |
dc.identifier.uri | http://www.sciencedirect.com/science/article/B6V6T-471XB0G-Y/2/2baa79e3df4cef9debf6acd6a67dd794 | en_US |
dc.identifier.uri | https://hdl.handle.net/2027.42/31969 | |
dc.description.abstract | Line strengths of magnetic dipole and electric quadrupole transitions in the configurations 2p2, 2p4, 3p2 and 3p4 are calculated using interpolated values of spin-orbit interaction parameters and unperturbed energies of the levels. Probabilities of the important ground state transitions are tabulated in the four isoelectronic sequences through the following net charges: 17(2p2), 13(2p4), 15(3p2), 13(3p4). | en_US |
dc.format.extent | 289026 bytes | |
dc.format.extent | 3118 bytes | |
dc.format.mimetype | application/pdf | |
dc.format.mimetype | text/plain | |
dc.language.iso | en_US | |
dc.publisher | Elsevier | en_US |
dc.title | Transition probabilities in highly ionized p2 and p4 configurations | en_US |
dc.type | Article | en_US |
dc.rights.robots | IndexNoFollow | 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 of The University of Michigan, Ann Arbor, Michigan, USA | en_US |
dc.contributor.affiliationum | Department of Astronomy of The University of Michigan, Ann Arbor, Michigan, USA | en_US |
dc.description.bitstreamurl | http://deepblue.lib.umich.edu/bitstream/2027.42/31969/1/0000011.pdf | en_US |
dc.identifier.doi | http://dx.doi.org/10.1016/0032-0633(65)90143-1 | en_US |
dc.identifier.source | Planetary and Space Science | en_US |
dc.owningcollname | Interdisciplinary and Peer-Reviewed |
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