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

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2<br />

– bˆ<br />

B ⋅∇B<br />

ˆ ˆ∇B<br />

cancels the parallel component<br />

2<br />

− ∇B 2µ<br />

0<br />

component <strong>of</strong> the magnetic pressure exerts a force on the<br />

<strong>of</strong> the term. Thus only the perpendicular<br />

plasma.<br />

= bb<br />

µ<br />

0<br />

2<br />

µ<br />

0<br />

2<br />

2<br />

ˆ<br />

– ( B ˆ ˆ nB<br />

) b ⋅∇b<br />

= −(<br />

) is the magnetic tension<br />

µ<br />

0 µ<br />

0R C<br />

and is directed antiparallel <strong>to</strong> the radius <strong>of</strong><br />

curvature (R C ) <strong>of</strong> the field line. Note that nˆ is<br />

directed outward.

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