Probing Solar Subsurface Magnetic Fields View Full Text


Ontology type: schema:Chapter     


Chapter Info

DATE

2003

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

References to SciGraph publications

Book

TITLE

Advances in Space Environment Research - Volume I

ISBN

978-1-4020-1278-5
978-94-007-1069-6

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/978-94-007-1069-6_4

DOI

http://dx.doi.org/10.1007/978-94-007-1069-6_4

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1032387970


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