Stark broadening of solar Mg I lines

被引：20

作者：

Dimitrijevic, MS ^{[1
]}

SahalBrechot, S ^{[1
]}

机构：

[1] OBSERV PARIS,UA CNRS 812,DEPT ATOMES & MOLEC ASTROPHYS,LAB ASTROPHYS ATOMES & MOLEC,F-92190 MEUDON,FRANCE

来源：

ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES | 1996年 / 117卷 / 01期

关键词：

lines; profile-atomic and molecular data; Sun; photosphere; chromosphere;

D O I：

10.1051/aas:1996135

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Using a semiclassical approach, we have calculated electron-, proton-, Mg II-, Si II-, Fe II-, and Ar II- impact line widths and shifts for 267 Mg I multiplets, in order to provide the needed Stark broadening parameters for all important perturbers for investigation of Solar and laboratory plasma. An analysis of Solar Rydberg lines in the far infrared spectrum has been performed as well.

引用

页码：127 / 129

页数：3

共 34 条

[1]

BASHKIN S, 1975, ATOMIC ENERGY LEVELS, V1

[2] THE CALCULATION OF THE ABSOLUTE STRENGTHS OF SPECTRAL LINES [J].