Electron-Ion Collision Studies Using the Caprice 14.0 GHz ECRIS
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Engineering topics
Publications and source records attributed to Hitz, D..
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Experimental and theoretical collisional excitation cross sections are reported for the transitions 3s(exp 2)3p(exp 3)4S(exp o) approaches 3s(exp 2)3p(exp 3) 2D(exp o), 2P(exp o), and 3s3P(exp 4) 4P in S II. The transition wavelengths (energies) are 6716 A (1.85 eV), 4069 A (3.05 eV), and 1256 A (9.87 eV), respectively. In the experiments, use is made of the energy-loss merged-beams method. The metastable fraction of the S II beam was assessed and minimized. The contribution of elastically scattered electrons was reduced by the use of a lowered solenoidal magnetic field and a modulated radio-frequency voltage on the analyzing plates and by retarding grids to reject the elastically scattered electrons with larger Larmor radii. For each transition, comparisons are made among experiments, the new 19 state R-matrix calculation, and three other close-coupling calculations.
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Experimental and theoretical collisional excitation cross sections are reported for the transitions 3s(sup 2)3p(sup 3) (sup 4)s(deg) (leads to)3s(sup 2)3p(sup 3)(sup 2)D(deg), (sup 2)p(deg) and 3s3p(sup 4) (sup 4)p in s//.
In order to provide a better understanding of the energy balance and ion composition in solar, stellar, and planetary atmospheres, and in the interstellar medium, a new research facility for the study of interactions of multiply-charged ions has been developed at the Jet Propulsion Laboratory (JPL).