Stark broadening of neutral germanium spectral lines
نویسندگان
چکیده
منابع مشابه
QUADRATIC STARK CONSTANTS OF NEUTRAL COPPER SPECTRAL LINES IN THE COULOMB APPROXIMATION
Quadratic Stark constants of neutral copper spectral lines for all s,p, and d levels are calculated using the Coulomb approximation. These results are compared with existing data and, generally, good agreement is observed
متن کاملStark broadening of impurity absorption lines by inhomogeneous electric fields in highly compensated germanium.
Stark broadening of Zeeman absorption lines caused by inhomogeneous electric fields in highly compensated Ge has been studied by means of far-infrared magneto-optical absorption spectroscopy measurements. A number of transmutation-doped Ge single crystals with a systematically varying compensation ratio were employed. The broadening of the full width at half maximum ~FWHM! of an absorption line...
متن کاملquadratic stark constants of neutral copper spectral lines in the coulomb approximation
quadratic stark constants of neutral copper spectral lines for all s,p, and d levels are calculated using the coulomb approximation. these results are compared with existing data and, generally, good agreement is observed
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A t low t e m p e r a t u r e s t h e effect of back reac t ion of t h e neu t ra l emi t t e r on a pe r tu rb ing electron m a y become not iceable a n d consequent ly deviat ions of t h e electron mot ion f r o m the un i form one should be t a k e n into account . I n th is no te we discuss some consequences of a n inclusion of the curvi l inear t ra jec tor ies on the i m p a c t S t a r k...
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Plasma spectral line broadening is an important tool for plasma diagnostic in both laboratory and astrophysical field. The neutral helium lines are used e.g., in industrial applications and to determine the properties of stellar atmospheres of hot stars. In local thermal equilibrium, the spectral line profile is related to the dipole autocorrelation function which is related to the two-particle...
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ژورنال
عنوان ژورنال: Astronomy & Astrophysics
سال: 2003
ISSN: 0004-6361,1432-0746
DOI: 10.1051/0004-6361:20031176