Line Formation Theory for the Multiterm Atom with Hyperfine Structure in a Magnetic Field

2005 ◽  
Vol 624 (2) ◽  
pp. 1025-1037 ◽  
Author(s):  
R. Casini ◽  
R. Manso Sainz
2001 ◽  
Vol 203 ◽  
pp. 303-306 ◽  
Author(s):  
Z. Q. Qu ◽  
Y. C. Jiang ◽  
T. Luan ◽  
Z. Xu

The three-dimensional (3D) image of an Hα flare is reconstructed from its line-center and seriary off-center filtergrams. The reconstruction is based on the principle of the line formation theory that the contribution function (CF) of emergent specific line intensity describes the escape photon distribution from stellar atmospheric layers. Thus the reconstruction depends on the model atmosphere accepted which determines the CF. An Hα flare taking place on April 22, 1992 is utilized to illustrate the process.


1971 ◽  
Vol 43 ◽  
pp. 37-43
Author(s):  
M. Semel

It is demonstrated that certain interrelations between the Stokes parameters are much less dependent on line formation than generally expected. Thus the dependence of these parameters on the magnetic field may be made more explicit and may lead to reliable calibration of polarimetric measurements in terms of magnetic field.


Solar Physics ◽  
1972 ◽  
Vol 27 (2) ◽  
pp. 319-329 ◽  
Author(s):  
Egidio Landi Degl'innocenti ◽  
Maurizio Landi Degl'innocenti

E.p.r. and endor spectra have been measured in ThO 2 containing Tb 4+ . The crystalline electric field is cubic, and the splittings are very large compared with other S state ions. The values of the parameters in the standard cubic spin-Hamiltonian are: g = 2·0146 ±0·0004, 60 B 4 = —2527·53 ±0·10 Mc/s, 1260 B 6 = —24·84 ± 0·04 Mc/s, A = —73·891 ±0·023 Mc/s, B = + 6·194 ± 0·038 Mc/s, μN ( 159 Tb) = + 1·994 ± 0·004 nuclear magnetons. There are also additional small high-order terms. There are very marked differences between these parameters and those for the other S state ions Gd 3+ and Eu 2+ . In addition to the much larger 60 B 4 , the g value is in excess of the free spin value; at the nucleus, the electrons produce a smaller magnetic field (proportional to A / g 1 ) and a larger electric field gradient (proportional to B / Q ) than they do in Gd 3+ and Eu 2+ . These differences are probably due to covalent bonding. The value of the nuclear moment of 159 Tb has been used to obtain a value of <r -3 > = 8·23 a.u. for Tb 3+ from the known hyperfine structure in Tb 3+ .


Solar Physics ◽  
1969 ◽  
Vol 10 (2) ◽  
pp. 268-282 ◽  
Author(s):  
David E. Rees

2009 ◽  
Vol 43 (1) ◽  
pp. 012002 ◽  
Author(s):  
T Knopp ◽  
T F Sattel ◽  
S Biederer ◽  
T M Buzug

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