Solar physics meeting at IIA, Bangalore
Solar physics meeting at IIA, Bangalore
Solar physics meeting at IIA, Bangalore
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Towards flux transport dynamo<br />
• Induction equ<strong>at</strong>ion:<br />
model<br />
∂ B =∇× ( v × B)<br />
+ η ∇<br />
2<br />
B<br />
∂t<br />
t<br />
Evolution of mean (large scale) field is given by<br />
∂ B = ∇× ( v × B + α<br />
B ) + η<br />
2<br />
T<br />
∇<br />
B<br />
∂t<br />
•Our approach is kinem<strong>at</strong>ics (velocity field is given)
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