Solar physics meeting at IIA, Bangalore
Solar physics meeting at IIA, Bangalore
Solar physics meeting at IIA, Bangalore
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Magnetic buoyancy:<br />
y<br />
Inside flux Tube,<br />
P<br />
out<br />
B<br />
2µ<br />
2<br />
= P<br />
in<br />
+ out in<br />
P<br />
≤<br />
P<br />
Usually the inside is under-dense
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