A Brief Introduction to Space Plasma Physics.pdf - Institute of ...
A Brief Introduction to Space Plasma Physics.pdf - Institute of ...
A Brief Introduction to Space Plasma Physics.pdf - Institute of ...
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– On time scales much shorter than<br />
r<br />
∂B<br />
∂t<br />
r r<br />
= ∇× ( u × B)<br />
– The electric field vanishes in the frame moving with the fluid.<br />
– Consider the rate <strong>of</strong> change <strong>of</strong> magnetic flux<br />
dΦ<br />
dt<br />
=<br />
d<br />
dt<br />
r<br />
∂B<br />
∂t<br />
∫ B ⋅ndA<br />
= ∫ ⋅ ndA + ∫ B ⋅(<br />
u ×<br />
A<br />
r<br />
ˆ<br />
– The first term on the right is caused by the temporal changes<br />
in B<br />
– The second term is caused by motion <strong>of</strong> the boundary<br />
– The term is the area swept out per unit time<br />
A<br />
r r<br />
u × dl<br />
0<br />
– Use S<strong>to</strong>ke’s theorem<br />
Φ r<br />
d ⎛ ∂<br />
⎞<br />
= ∫ B r r<br />
⎜ ( ) ⎟<br />
− ∇× u × B<br />
⋅ nˆ<br />
=<br />
dt ⎝ ∂<br />
dA<br />
A<br />
t<br />
⎠<br />
– If the fluid is initially on surface s as it moves through the<br />
system the flux through the surface will remain constant<br />
even though the location and shape <strong>of</strong> the surface change.<br />
ˆ<br />
τ D<br />
C<br />
r<br />
r<br />
r<br />
dl )