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Bekki, Yuto, Cameron, Robert H. (2023) Three-dimensional non-kinematic simulation of the post-emergence evolution of bipolar magnetic regions and the Babcock-Leighton dynamo of the Sun. Astronomy & Astrophysics, 670. doi:10.1051/0004-6361/202244990

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Reference TypeJournal (article/letter/editorial)
TitleThree-dimensional non-kinematic simulation of the post-emergence evolution of bipolar magnetic regions and the Babcock-Leighton dynamo of the Sun
JournalAstronomy & Astrophysics
AuthorsBekki, YutoAuthor
Cameron, Robert H.Author
Year2023 (February)Volume670
PublisherEDP Sciences
DOIdoi:10.1051/0004-6361/202244990Search in ResearchGate
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Mindat Ref. ID15698000Long-form Identifiermindat:1:5:15698000:7
GUID0
Full ReferenceBekki, Yuto, Cameron, Robert H. (2023) Three-dimensional non-kinematic simulation of the post-emergence evolution of bipolar magnetic regions and the Babcock-Leighton dynamo of the Sun. Astronomy & Astrophysics, 670. doi:10.1051/0004-6361/202244990
Plain TextBekki, Yuto, Cameron, Robert H. (2023) Three-dimensional non-kinematic simulation of the post-emergence evolution of bipolar magnetic regions and the Babcock-Leighton dynamo of the Sun. Astronomy & Astrophysics, 670. doi:10.1051/0004-6361/202244990
In(2023) Astronomy and Astrophysics Vol. 670. EDP Sciences

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Cloutier, S., Cameron, R. H., Gizon, L. (2023) A Babcock-Leighton dynamo model of the Sun incorporating toroidal flux loss and the helioseismically inferred meridional flow. Astronomy & Astrophysics, 680. doi:10.1051/0004-6361/202347022
Cameron, R. H., Schüssler, M. (2020) Loss of toroidal magnetic flux by emergence of bipolar magnetic regions. Astronomy & Astrophysics, 636. doi:10.1051/0004-6361/201937281
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Bekki, Yuto, Cameron, Robert H., Gizon, Laurent (2022) Theory of solar oscillations in the inertial frequency range: Linear modes of the convection zone. Astronomy & Astrophysics, 662. doi:10.1051/0004-6361/202243164
Kumar, Rohit, Jouve, Laurène, Nandy, Dibyendu (2019) A 3D kinematic Babcock Leighton solar dynamo model sustained by dynamic magnetic buoyancy and flux transport processes. Astronomy & Astrophysics, 623. doi:10.1051/0004-6361/201834705
Toriumi, S., Yokoyama, T. (2013) Three-dimensional magnetohydrodynamic simulation of the solar magnetic flux emergence. Astronomy & Astrophysics, 553. doi:10.1051/0004-6361/201321098
Pierens, Arnaud, Nelson, Richard P. (2023) Three-dimensional evolution of radiative circumbinary discs: The size and shape of the inner cavity. Astronomy & Astrophysics, 670. doi:10.1051/0004-6361/202244828
Cloutier, S., Cameron, R. H., Gizon, L. (2025) The rush to the poles and the role of magnetic buoyancy in the solar dynamo. Astronomy & Astrophysics, 693. doi:10.1051/0004-6361/202450968
Bekki, Yuto (2024) Numerical study of non-toroidal inertial modes with l = m + 1 radial vorticity in the Sun’s convection zone. Astronomy & Astrophysics, 682. doi:10.1051/0004-6361/202348380
Hofer, B., Krivova, N. A., Cameron, R., Solanki, S. K., Jiang, J. (2024) The influence of small bipolar magnetic regions on basic solar quantities. Astronomy & Astrophysics, 683. doi:10.1051/0004-6361/202245635
Guerrero, G., de Gouveia Dal Pino, E. M. (2008) Turbulent magnetic pumping in a Babcock-Leighton solar dynamo model. Astronomy & Astrophysics, 485 (1). 267-273 doi:10.1051/0004-6361:200809351
 
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