INTENSITY VELOCITY AND MAGNETIC STRUCTURE OF A SUNSPOT REGION .3. ON ORIGIN OF APPARENT PI COMPONENT IN SUNSPOT UMBRAE

被引:22
作者
BECKERS, JM
SCHROTER, EH
机构
[1] Sacramento Peak Observatory Air Force Cambridge Research Laboratories, Sunspot, N.M.
[2] Universitäts-Sternwarte, Göttingen
关键词
D O I
10.1007/BF00148400
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
[No abstract available]
引用
收藏
页码:22 / &
相关论文
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  • [3] DEUBNER F, TO BE PUBLISHED
  • [4] DEUBNER FL, 1967, MITT ASTRON GES, V22, P33
  • [5] HENOUX JC, 1968, SOL PHYS, V4, P315
  • [6] Severnyi A. B., 1959, SOV ASTRON, V3, P214
  • [7] SHEELEY NR, 1968, PRIVATE COMMUNICATIO