T. S. T. Young
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Corrigendum: Numerical Simulations of Large-scale Solar Magnetic Fields Open
On p.1000, both the fourth and fifth terms on the left-hand side of equation (1) should be preceded by minus signs. Line 22 on the same page should read: ' ... obtained by integrating equation (1) for S = 0, ...
Numerical Simulations of Large-scale Solar Magnetic Fields Open
We have solved numerically a transport equation which describes the evolution of the large-scale magnetic field of the Sun. Data derived from solar magnetic observations are used to initialize the computations and to account for the emerge…