Exploring the Physical Basis of Solar Cycle Predictions: Flux Transport Dynamics and Persistence of Memory in Advection‐ versus Diffusion‐dominated Solar Convection Zones

Anthony R. Yeates; Dibyendu Nandy; Duncan H. Mackay

doi:10.1086/524352

journal article Jan 20, 2008

Exploring the Physical Basis of Solar Cycle Predictions: Flux Transport Dynamics and Persistence of Memory in Advection‐ versus Diffusion‐dominated Solar Convection Zones

Anthony R. Yeates Dibyendu Nandy

Duncan H. Mackay

The Astrophysical Journal Vol. 673 No. 1 pp. 544-556 · American Astronomical Society

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Details

Published: Jan 20, 2008
Vol/Issue: 673(1)
Pages: 544-556

Authors

Department of Physical Sciences Indian Institute of Science Education and Research Kolkata Mohanpur India; Center of Excellence in Space Sciences India, Indian Institute of Science Education and Research Kolkata Mohanpur India

D

Duncan H. Mackay

Cite This Article

Anthony R. Yeates, Dibyendu Nandy, Duncan H. Mackay (2008). Exploring the Physical Basis of Solar Cycle Predictions: Flux Transport Dynamics and Persistence of Memory in Advection‐ versus Diffusion‐dominated Solar Convection Zones. The Astrophysical Journal, 673(1), 544-556. https://doi.org/10.1086/524352

Exploring the Physical Basis of Solar Cycle Predictions: Flux Transport Dynamics and Persistence of Memory in Advection‐ versus Diffusion‐dominated Solar Convection Zones

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