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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.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
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