EFFECT OF EXCITATION-AUTOIONIZATION PROCESSES ON THE LINE EMISSION OF ZN-I-LIKE AND GA-I-LIKE RARE-EARTH IONS IN HOT CORONAL PLASMAS

被引:19
作者
MANDELBAUM, P
FINKENTHAL, M
MEROZ, E
SCHWOB, JL
OREG, J
GOLDSTEIN, WH
KLAPISCH, M
OSTERHELD, L
SHALOM, AB
LIPPMAN, S
HUANG, LK
MOOS, HW
机构
[1] UNIV CALIF LAWRENCE LIVERMORE NATL LAB, DIV HIGH TEMP PHYS, LIVERMORE, CA 94550 USA
[2] UNIV CALIF BERKELEY, BERKELEY, CA 94720 USA
[3] JOHNS HOPKINS UNIV, DEPT PHYS, BALTIMORE, MD 21218 USA
[4] GEN ATOM CO, SAN DIEGO, CA 92138 USA
来源
PHYSICAL REVIEW A | 1990年 / 42卷 / 07期
关键词
D O I
10.1103/PhysRevA.42.4412
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
A systematic variation in the line-intensity ratios of Gai and Zni-like Pr (Z=59) to Dy (Z=66) ions has been observed in spectra emitted by atoms injected in a low-density high-temperature tokamak plasma. This variation is shown to be correlated with the progressive closing of the autoionizing channels through the excited 3d94s24p4f configuration in the Gai-like ionization state as Z increases. © 1990 The American Physical Society.
引用
收藏
页码:4412 / 4415
页数:4
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