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A Brief Introduction to Space Plasma Physics.pdf - Institute of ...

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– Momentum equation<br />

r<br />

∂us<br />

r r r<br />

r r r<br />

ρ<br />

s<br />

( + us<br />

⋅∇us<br />

) + msus<br />

( Ss<br />

− Ls<br />

) = −∇ps<br />

+ ρqsE<br />

+ J<br />

s<br />

× B + ρsF<br />

∂t<br />

ρ<br />

= q<br />

n<br />

r<br />

J =<br />

where qs s s is the charge density, s s s s is the<br />

current density, and the last term is the density <strong>of</strong> nonelectromagnetic<br />

forces<br />

∂ r<br />

– The opera<strong>to</strong>r ( + u s<br />

⋅∇)<br />

is called the convective derivative<br />

∂t<br />

and gives the <strong>to</strong>tal time derivative resulting from intrinsic<br />

time changes and spatial motion.<br />

– If the fluid is not moving (u s =0) the left side gives the net<br />

change in the momentum density <strong>of</strong> the fluid element.<br />

– The right side is the density <strong>of</strong> forces<br />

• If there is a pressure gradient then the fluid moves <strong>to</strong>ward lower<br />

pressure.<br />

• The second and third terms are the electric and magnetic<br />

forces.<br />

q<br />

n<br />

r<br />

u<br />

g<br />

m<br />

s

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