Are the umbral dots, penumbral grains, and G band bright points formed by the same type of magnetic flux tubes?

被引：0

作者：

Sattarov, Isroil ^{[1
]}

机构：

[1] Tashkent State Pedag Univ, Tashkent 100070, Uzbekistan

来源：

PHYSICS OF SUN AND STAR SPOTS | 2011年 / 273期

关键词：

Umbral dots; penumbral grains; sunspots; G-band bright points;

D O I：

10.1017/S1743921311015699

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Today's Solar Physics comes across of different type of fine structures in solar atmosphere including umbral dots and penumbral grains in sunspots, and C-band bright points in quiet Sun. In this report, we present evidence that umbral dots, penumbral grains, and, possibly, C band bright points are related to a common type of features in solar atmosphere magnetic flux tubes.

引用

页码：426 / 429

页数：4

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