PROMINENCE SEISMOLOGY USING GROUND- AND SPACE-BASED OBSERVATIONS

被引：0

作者：

Ballester, J. L. ^{[1
]}

Arregui, I. ^{[1
]}

Oliver, R. ^{[1
]}

Terradas, J. ^{[1
]}

Soler, R. ^{[2
]}

Lin, Y. ^{[3
]}

Engvold, O. ^{[3
]}

Langagen, O. ^{[3
]}

van der Voort, L. H. M. Rouppe ^{[3
]}

机构：

[1] Univ Illes Balears, Dept Fis, Mallorca, Spain

[2] KULeuven, Dept Astrophy, Brussels, Belgium

[3] Inst Theoritic Astrophy, Oslo, Norway

来源：

UNDERSTANDING SOLAR ACTIVITY: ADVANCES AND CHALLENGES | 2012年 / 55卷

关键词：

FILAMENT;

D O I：

10.1051/eas/1255023

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Ground- and space-based observations have confirmed the presence of oscillatory motions in prominences and they have been interpreted in terms of magnetohydrodynamic (MHD) waves. This interpretation opens the door to perform prominence seismology, whose main aim is to determine physical parameters in magnetic and plasma structures (prominences) that are difficult to measure by direct means. Here, two prominence seismology applications are presented.

引用

页码：169 / +

页数：2

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