Magnetic Flux in the Solar Convective Envelope Inferred from Initial Observations of Sunspots-Reference-Cited by-同舟云学术

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Magnetic Flux in the Solar Convective Envelope Inferred from Initial Observations of Sunspots

Published:2007-09-20 Issue:1 Volume:667 Page:585-590
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Hiremath K. M.,Lovely M. R.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference60 articles.

1. Antia, H. M. 2002, in IAU Colloq. 188, SOLMAG 2002, ed. H. Sawaya-Lacoste (ESA SP-505; Noordwijk: ESA), 71

2. Solar internal rotation rate and the latitudinal variation of the tachocline

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

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1. Reconstruction of Thermal and Magnetic Field Structure of the Solar Subsurface Through Helioseismology;Cartography of the Sun and the Stars;2016

2. Abnormal rotation rates of sunspots and durations of associated flares;Astronomy & Astrophysics;2015-07-22

3. Coronal Hole Oscillations as inferred from SDO/AIA data;Advances in Space Research;2014-07

4. Toroidal magnetic field structure of the solar convective envelope inferred from the initial observations of the sunspots;New Astronomy;2012-05

5. The mysterious Sun: a source and a trap of exotica;Journal of Physics: Conference Series;2011-08-10

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