CA-II K2V SPECTRAL FEATURES AND THEIR RELATION TO SMALL-SCALE PHOTOSPHERIC MAGNETIC-FIELDS

被引:69
作者
SIVARAMAN, KR [1 ]
LIVINGSTON, WC [1 ]
机构
[1] KITT PEAK NATL OBSERV,TUCSON,AZ 85726
关键词
D O I
10.1007/BF00147970
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
引用
收藏
页码:227 / 231
页数:5
相关论文
共 7 条
[1]   K EMISSION-LINE WIDTHS AND SOLAR CHROMOSPHERE [J].
BAPPU, MK ;
SIVARAMAN, KR .
SOLAR PHYSICS, 1971, 17 (02) :316-+
[2]  
FRAZIER EN, 1970, SOL PHYS, V14, P89, DOI 10.1007/BF00240163
[3]  
Harvey J., 1977, Highlights of Astronomy, P223
[4]  
LEAN JL, 1981, EOS, V62, P1017
[5]   DIRECT OBSERVATIONAL EVIDENCE FOR PROPAGATION AND DISSIPATION OF ENERGY IN CHROMOSPHERE [J].
LIU, SY .
ASTROPHYSICAL JOURNAL, 1974, 189 (02) :359-366
[6]   TIME BEHAVIOR OF CAII K2NU SPECTRAL FEATURES IN NON-MAGNETIC REGIONS OF SOLAR DISK [J].
LIU, SY ;
SHEELEY, NR ;
SMITH, EVP .
SOLAR PHYSICS, 1972, 23 (02) :289-&
[7]   SOLAR MAGNETOGRAPH EMPLOYING INTEGRATED DIODE ARRAYS [J].
LIVINGSTON, WC ;
HARVEY, J ;
SLAUGHTER, C ;
TRUMBO, D .
APPLIED OPTICS, 1976, 15 (01) :40-52