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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 )

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