Solar physics meeting at IIA, Bangalore
Solar physics meeting at IIA, Bangalore
Solar physics meeting at IIA, Bangalore
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Dynamo growth r<strong>at</strong>e is<br />
determined by the<br />
dynamo number,<br />
N<br />
D<br />
∝<br />
η<br />
α<br />
2<br />
P<br />
If the dur<strong>at</strong>ion of the M.M.<br />
is really an indic<strong>at</strong>or of the<br />
dynamo growth time, then<br />
it puts constraints on the<br />
parameters of the model.<br />
Choudhuri & Karak (2009)
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