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Schrinner, M., Schmitt, D., Jiang, J., Hoyng, P. (2010) An efficient method for computing the eigenfunctions of the dynamo equation. Astronomy and Astrophysics, 519. doi:10.1051/0004-6361/200913702

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Reference TypeJournal (article/letter/editorial)
TitleAn efficient method for computing the eigenfunctions of the dynamo equation
JournalAstronomy and Astrophysics
AuthorsSchrinner, M.Author
Schmitt, D.Author
Jiang, J.Author
Hoyng, P.Author
Year2010 (September)Volume519
PublisherEDP Sciences
DOIdoi:10.1051/0004-6361/200913702Search in ResearchGate
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Mindat Ref. ID13985248Long-form Identifiermindat:1:5:13985248:2
GUID0
Full ReferenceSchrinner, M., Schmitt, D., Jiang, J., Hoyng, P. (2010) An efficient method for computing the eigenfunctions of the dynamo equation. Astronomy and Astrophysics, 519. doi:10.1051/0004-6361/200913702
Plain TextSchrinner, M., Schmitt, D., Jiang, J., Hoyng, P. (2010) An efficient method for computing the eigenfunctions of the dynamo equation. Astronomy and Astrophysics, 519. doi:10.1051/0004-6361/200913702
In(2010) Astronomy and Astrophysics Vol. 519. EDP Sciences

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Schrinner, M. (2011) Global dynamo models from direct numerical simulations and their mean-field counterparts. Astronomy & Astrophysics, 533. doi:10.1051/0004-6361/201116642
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Schüssler, M., Schmitt, D. (2004) Does the butterfly diagram indicate a solar flux-transport dynamo?. Astronomy & Astrophysics, 421 (1). 349-351 doi:10.1051/0004-6361:20041302-1
Jiang, J., Cameron, R. H., Schmitt, D., Schüssler, M. (2011) The solar magnetic field since 1700. Astronomy & Astrophysics, 528. doi:10.1051/0004-6361/201016167
Jiang, J., Cameron, R. H., Schmitt, D., Schüssler, M. (2011) The solar magnetic field since 1700. Astronomy & Astrophysics, 528. doi:10.1051/0004-6361/201016168
Mislis, D., Schmitt, J. H. M. M., Carone, L., Guenther, E. W., Pätzold, M. (2010) An algorithm for correcting CoRoT raw light curves. Astronomy & Astrophysics, 522. doi:10.1051/0004-6361/201014334
Jouve, L., Proctor, M. R. E., Lesur, G. (2010) Buoyancy-induced time delays in Babcock-Leighton flux-transport dynamo models. Astronomy and Astrophysics, 519. doi:10.1051/0004-6361/201014455
 
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