Probing Solar Subsurface Magnetic Fields View Full Text


Ontology type: schema:ScholarlyArticle     


Article Info

DATE

2003-04

AUTHORS

Dean-Yi Chou, Alexander Serebryanskiy, Ming-Tsung Sun

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. More... »

PAGES

35-42

Journal

TITLE

Space Science Reviews

ISSUE

1-2

VOLUME

107

Identifiers

URI

http://scigraph.springernature.com/pub.10.1023/a:1025594932638

DOI

http://dx.doi.org/10.1023/a:1025594932638

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1022109921


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