Observations of Large-Scale Dynamic Bubbles in Prominences

被引：0

作者：

de Toma, G. ^{[1
]}

Casini, R. ^{[1
]}

Berger, T. E. ^{[2
]}

Low, B. C. ^{[1
]}

de Wijn, A. G. ^{[1
]}

Burkepile, J. T. ^{[1
]}

Balasubramaniam, K. S. ^{[3
]}

机构：

[1] Natl Ctr Atmospher Res, High Altitude Observ, POB 3000, Boulder, CO 80307 USA

[2] Lockheed Martin Solar & astrophys Lab, Palo Alto, CA 94304 USA

[3] Natl Solar Observ, Air Force Res Lab, Sunspot, NM USA

来源：

SECOND HINODE SCIENCE MEETING: BEYOND DISCOVERY-TOWARD UNDERSTANDING | 2009年 / 415卷

基金：

美国国家科学基金会;

关键词：

QUIESCENT PROMINENCE;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Solar prominences are very dynamic objects, showing continuous motions down to their smallest resolvable spatial and temporal scales. However, as macroscopic magnetic structures, they are remarkably stable during their quiescent phase. We present recent ground-based and Hinode observations of large-scale bubble-like, dynamic sub-structures that form within and rise through quiescent prominences without disrupting them. We investigate the similarities and differences of the Hinode and ground-based observations and discuss their implications for models of prominences.

引用

页码：163 / +

页数：2

共 4 条

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