Line formation in a magnetic field

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

Measurements of Magnetic Fields

1971 ◽  
Vol 43 ◽  
pp. 37-43
Author(s):  
M. Semel
Keyword(s):  
Magnetic Field ◽  
Magnetic Fields ◽  
Stokes Parameters ◽  
Line Formation ◽  
On Line ◽  
The Magnetic Field

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.

Quantum theory of line formation in a magnetic field

Solar Physics ◽  
1972 ◽  
Vol 27 (2) ◽  
pp. 319-329 ◽  
Author(s):  
Egidio Landi Degl'innocenti ◽  
Maurizio Landi Degl'innocenti
Keyword(s):  
Magnetic Field ◽  
Quantum Theory ◽  
Line Formation

Field-free line formation in a magnetic field

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

Non-LTE line formation in a magnetic field

Solar Physics ◽  
1973 ◽  
Vol 31 (2) ◽  
pp. 291-298 ◽  
Author(s):  
H. Domke ◽  
J. Staude
Keyword(s):  
Magnetic Field ◽  
Line Formation

Non-LTE line formation in a magnetic field

Solar Physics ◽  
1973 ◽  
Vol 31 (2) ◽  
pp. 279-289 ◽  
Author(s):  
H. Domke ◽  
J. Staude
Keyword(s):  
Magnetic Field ◽  
Line Formation

scholarly journals Atomic Data Relevant to Line Formation in Strongly Magnetized White Dwarf Stars

1987 ◽  
Vol 93 ◽  
pp. 595-599
Author(s):  
G. Wunner ◽  
F. Geyer ◽  
H. Ruder
Keyword(s):  
Magnetic Field ◽  
Quantitative Analysis ◽  
White Dwarf ◽  
Atomic Data ◽  
Line Formation ◽  
Dwarf Stars ◽  
White Dwarf Stars ◽  
Field Strengths

AbstractThe discovery of magnetic field strengths in the range of 500 million Gauss in the objects Grw+70°8247 and PG1031+224 has given enormous impetus to investigations of magnetic white dwarf stars. We have determined intensities of Balmer transitions for B > 108 Gauss as a function of field and find strong oscillations of the transitions strengths, which are of importance to the quantitative analysis of the observed spectra and the interpretation of polarimetric measurements in these objects.

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