Searching for the Signature of the Magnetic Fields at the Base of the Solar Convection Zone with Solar Cycle Variations of [CLC][ITAL]p[/ITAL][/CLC]-Mode Travel Time-Reference-Cited by-同舟云学术

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Searching for the Signature of the Magnetic Fields at the Base of the Solar Convection Zone with Solar Cycle Variations of [CLC][ITAL]p[/ITAL][/CLC]-Mode Travel Time

Published:2002-10-20 Issue:2 Volume:578 Page:L157-L160
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:

Author:

Chou Dean-Yi,Serebryanskiy Alexander

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference32 articles.

1. Solar-cycle variation of the sound-speed asphericity from GONG and MDI data 1995-2000

2. The Topology of the Sun's Magnetic Field and the 22-YEAR Cycle.

3. Seismology of the base of the solar convection zone

4. Basu, S. & Antia, H. M. 2001, in Proc. SOHO 10/GONG 2000 Workshop: Helio- and Asteroseismology at the Dawn of the Millennium, ed. A. Wilson (ESA SP-464; Noordwijk: ESA), 297

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1. Axion helioscopes as solar magnetometers;Physical Review D;2020-08-26

2. Solar radius and luminosity variations induced by the internal dynamo magnetic fields;Astronomische Nachrichten;2018-08

3. Prospects and Challenges for Helioseismology;Space Sciences Series of ISSI;2017

4. Seismic Holography of the Solar Interior near the Maximum and Minimum of Solar Activity;Solar Physics;2016-05

5. PROBING MAGNETIC FIELDS AT THE BASE OF THE SOLAR CONVECTION ZONE WITH MERIDIONAL FLOWS;The Astrophysical Journal;2015-08-19

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