Non linear inversion for the sound speed in the solar interior using bison and SOI/MDI p-mode frequencies

被引：0

作者：

Marchenkov, KI ^{[1
]}

Roxburgh, IW ^{[1
]}

Vorontsov, SV ^{[1
]}

Chaplin, WJ ^{[1
]}

Elsworth, Y ^{[1
]}

Isaak, GR ^{[1
]}

New, R ^{[1
]}

机构：

[1] Univ Birmingham, Sch Phys & Astron, Birmingham B15 2TT, W Midlands, England

来源：

PROCEEDINGS OF THE SOHO 10/GONG 2000 WORKSHOP ON HELIO- AND ASTEROSEISMOLOGY AT THE DAWN OF THE MILLENNIUM | 2001年 / 464卷

关键词：

sun : interior; sun : oscillations;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The results of the global sound-speed inversion obtained with solar p-mode frequencies provided by the recent high-quality observational data (BiSON, SOI/MDI) are presented and discussed. The iterative nonlinear inversion technique used here is a generalization (for the case of exact solution of the adiabatic oscillation equations) of the Born quasiasymptotic approximate inversion developed by Marchenkov et al. (2000).

引用

页码：531 / 534

页数：4

共 6 条

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ASTROPHYSICAL JOURNAL, 2003, 591 (01) : 432 - 445
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Chou, DY
ASTROPHYSICAL JOURNAL, 2005, 633 (02) : 1187 - 1190
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New, R
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1998, 300 (04) : 1077 - 1090
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GOUGH, DO
KOSOVICHEV, AG
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1993, 264 (02) : 522 - 528
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Chou, DY
Serebryanskiy, A
ASTROPHYSICAL JOURNAL, 2005, 624 (01) : 420 - 427
[6] Latitudinal variation of solar subsurface rotation inferred from p-mode frequency splittings measured with SOI-MDI and GONG
Birch, AC
Kosovichev, AG
ASTROPHYSICAL JOURNAL, 1998, 503 (02) : L187 - L190

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