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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– 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