Large-scale motion of solar filaments

被引：0
|
作者：
Ambroz, P [1 ]
Schroll, A
机构：
[1] Acad Sci Czech Republ, Inst Astron, CZ-25165 Ondrejov, Czech Republic
[2] Graz Univ, Kanzelhoehe Solar Observ, A-9521 Treffen, Austria
来源：
JOURNAL OF ASTROPHYSICS AND ASTRONOMY | 2000年 / 21卷 / 3-4期
关键词：
Sun; filaments; horizontal motions;
D O I：
10.1007/BF02702392
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Precise measurements of heliographic position of solar filaments were used for determination of the proper motion of solar filaments on the time-scale of days. The filaments have a tendency to make a shaking or waving of the external structure and to make a general movement of whole filament body, coinciding with the transport of the magnetic flux in the photosphere. The velocity scatter of individual measured points is about one order higher than the accuracy of measurements.
引用
收藏
页码：205 / 208
页数：4
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