Computational Seismic Holography of Transient Seismic Emission from Flares

被引：0

作者：

Lindsey, C. ^{[1
]}

Donea, A. -C. ^{[2
]}

Oliveros, J. C. Martinez ^{[3
]}

机构：

[1] NorthWest Res Associates, 3380 Mitchell Lane, Boulder, CO 80302 USA

[2] Monash Univ, Sch Math Sci, Ctr Stellar & Planetary Astrophys, Melbourne, Vic 3800, Australia

[3] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA

来源：

FIFTY YEARS OF SEISMOLOGY OF THE SUN AND STARS | 2013年 / 478卷

关键词：

MAGNETIC-FIELD CHANGES; SOLAR ATMOSPHERE; VELOCITY FIELDS;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Conceived as an optimal basis for local helioseismology, computational seismic holography applies basic principles of optics to helioseismic signatures of waves that travel through the Sun's interior, including its far hemisphere. Objects of its diagnostic applications include the thermal and magnetic structure of active regions, sources of seismic emission from the quiet Sun, active regions in the Sun's far hemisphere, and transient seismic emission from flares. The monitor of active regions in the Sun's far hemisphere is described by another paper in these proceedings. This paper reviews the application of computational seismic holography as a diagnostic of transient seismic emission from flares.

引用

页码：323 / +

页数：4

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