FURTHER EVIDENCE FOR DOWNFLOW IN SOLAR ATMOSPHERE

被引:0
作者
GREVE, A
机构
[1] Max Planck Institut für Radioastronomie, Bonn
关键词
D O I
10.1007/BF00157273
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Downflow velocities of the higher atmospheric layers of the Sun are derived from wavelength measurements of the Mg ii core absorption. © 1978 D. Reidel Publishing Company.
引用
收藏
页码:287 / 289
页数:3
相关论文
共 5 条
[1]  
Athay R. G., 1976, SOLAR CHROMOSPHERE C
[2]   HIGH-RESOLUTION SPECTRA OF SOLAR MG-II H AND K-LINES FROM SKYLAB [J].
DOSCHEK, GA ;
FELDMAN, U .
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 1977, 35 (04) :471-&
[3]   DOPPLER WAVELENGTH SHIFTS OF TRANSITION ZONE LINES MEASURED IN SKYLAB SOLAR SPECTRA [J].
DOSCHEK, GA ;
FELDMAN, U ;
BOHLIN, JD .
ASTROPHYSICAL JOURNAL, 1976, 205 (03) :L177-L180
[4]  
GOUTTEBROZE P, 1977, ASTRON ASTROPHYS, V54, P203
[5]   ULTRAVIOLET SOLAR SPECTRUM 2756A-2831A [J].
GREVE, A ;
MCKEITH, CD .
SOLAR PHYSICS, 1974, 37 (01) :3-30