Probing solar subsurface magnetic fields

Dean Yi Chou; Alexander Serebryanskiy; Ming Tsung Sun

doi:10.1023/A:1025594932638

Probing solar subsurface magnetic fields

Dean Yi Chou^*, Alexander Serebryanskiy, Ming Tsung Sun

^*Corresponding author for this work

Department of Mechanical Engineering

National Tsing Hua University

Research output: Contribution to journal › Journal Article › peer-review

1 Scopus citations

Abstract

Helioseismology uses solar p-mode oscillations to probe the structure of the solar interior. The modifications of p-mode properties due to the presence of solar magnetic fields provide information on the magnetic fields in the solar interior. Here we review some of results in helioseismology on the magnetic fields in the solar convection zone. We will also discuss a recent result on the magnetic fields at the base of the convection zone.

Original language	English
Pages (from-to)	35-42
Number of pages	8
Journal	Space Science Reviews
Volume	107
Issue number	1-2
DOIs	https://doi.org/10.1023/A:1025594932638
State	Published - 2003

Keywords

Helioseismology
Solar interior
Solar magnetic fields

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10.1023/A:1025594932638

Cite this

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title = "Probing solar subsurface magnetic fields",

abstract = "Helioseismology uses solar p-mode oscillations to probe the structure of the solar interior. The modifications of p-mode properties due to the presence of solar magnetic fields provide information on the magnetic fields in the solar interior. Here we review some of results in helioseismology on the magnetic fields in the solar convection zone. We will also discuss a recent result on the magnetic fields at the base of the convection zone.",

keywords = "Helioseismology, Solar interior, Solar magnetic fields",

author = "Chou, {Dean Yi} and Alexander Serebryanskiy and Sun, {Ming Tsung}",

year = "2003",

doi = "10.1023/A:1025594932638",

language = "英语",

volume = "107",

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journal = "Space Science Reviews",

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AU - Serebryanskiy, Alexander

AU - Sun, Ming Tsung

PY - 2003

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N2 - Helioseismology uses solar p-mode oscillations to probe the structure of the solar interior. The modifications of p-mode properties due to the presence of solar magnetic fields provide information on the magnetic fields in the solar interior. Here we review some of results in helioseismology on the magnetic fields in the solar convection zone. We will also discuss a recent result on the magnetic fields at the base of the convection zone.

AB - Helioseismology uses solar p-mode oscillations to probe the structure of the solar interior. The modifications of p-mode properties due to the presence of solar magnetic fields provide information on the magnetic fields in the solar interior. Here we review some of results in helioseismology on the magnetic fields in the solar convection zone. We will also discuss a recent result on the magnetic fields at the base of the convection zone.

KW - Helioseismology

KW - Solar interior

KW - Solar magnetic fields

UR - http://www.scopus.com/inward/record.url?scp=0142059592&partnerID=8YFLogxK

U2 - 10.1023/A:1025594932638

DO - 10.1023/A:1025594932638

M3 - 文章

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SN - 0038-6308

VL - 107

SP - 35

EP - 42

JO - Space Science Reviews

JF - Space Science Reviews

IS - 1-2

ER -

Probing solar subsurface magnetic fields

Abstract

Keywords

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