Recent Developments in Helioseismic Analysis Methods and Solar Data Assimilation

被引：4

作者：

Schad, A. ^{[1
]}

Jouve, L. ^{[2
]}

Duvall, T. L., Jr. ^{[3
]}

Roth, M. ^{[1
]}

Vorontsov, S. ^{[4
,5
]}

机构：

[1] Kiepenheuer Inst Sonnenphys, D-79104 Freiburg, Germany

[2] Univ Toulouse, UPS OMP, Inst Rech Astrophys & Planetol, F-31028 Toulouse 4, France

[3] Max Planck Inst Sonnensyst Forsch, D-37077 Gottingen, Germany

[4] Queen Mary Univ London, Astron Unit, Sch Phys & Astron, London E1 4NS, England

[5] Inst Phys Earth, Moscow 123810, Russia

来源：

SPACE SCIENCE REVIEWS | 2015年 / 196卷 / 1-4期

基金：

欧洲研究理事会;

关键词：

Sun; Helioseismology; Data analysis; FLUX-TRANSPORT DYNAMO; EMERGING SUNSPOT REGIONS; MERIDIONAL FLOW; MAGNETIC-FIELD; POWER SPECTRA; MODEL; CONVECTION; CIRCULATION; PREDICTABILITY; FREQUENCIES;

D O I：

10.1007/s11214-015-0199-y

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We review recent advances and results in enhancing and developing helioseismic analysis methods and in solar data assimilation. In the first part of this paper we will focus on selected developments in time-distance and global helioseismology. In the second part, we review the application of data assimilation methods on solar data. Relating solar surface observations as well as helioseismic proxies with solar dynamo models by means of the techniques from data assimilation is a promising new approach to explore and to predict the magnetic activity cycle of the Sun.

引用

页码：221 / 249

页数：29

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