Solar physics meeting at IIA, Bangalore
Solar physics meeting at IIA, Bangalore
Solar physics meeting at IIA, Bangalore
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Dynamo Model:<br />
Parker (1955)<br />
Axisymmetric magnetic field= toroidal+poloidal<br />
B = B ( r, θ<br />
) e φ<br />
+∇×<br />
[ A ( r, θ<br />
) e<br />
φ<br />
]