Interior and Exterior Clues of Solar Activity

Bibcode
2010mcia.conf..368T
DOI
10.1007/978-3-642-02859-5_33
Turck-Chièze, S.; Brun, A. S.; Duez, V.; García, R. A.; Mathis, S.; Piau, L.; Salabert, D.; Pallé, P. L.; Jiménez-Reyes, S. J.; Mathur, S.; Simoniello, R.; Robillot, J. M.
Bibliographical reference

Magnetic Coupling between the Interior and Atmosphere of the Sun, edited by S.S. Hasan and R.J. Rutten; Astrophysics and Space Science Proceedings. ISSN 1570-6591 (Print) 1570-6605 (Online) Published by Springer Berlin Heidelberg; ISBN 978-3-642-02858-8 (Print) 978-3-642-02859-5 (Online), pp.368-373

Advertised on:
2010
Number of authors
12
IAC number of authors
3
Citations
0
Refereed citations
0
Description
Two research paths are described to obtain better understanding of the origin of global solar activity. First, observations with a multichannel resonant spectrometer may reveal the dynamics of the solar core, the tachocline, and the temporal evolution of activity between the photosphere and chromosphere. Such new observations will deliver constraints for 3D simulations of solar activity. Second, we examine the ab-initio introduction of a non-force-free field expressed in spherical harmonics into the solar structure equations and estimate its impact on the inner and subsurface layers, its time evolution, and its role in angular momentum transport.
Type
Non-refereed

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