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Global Monitoring of the Terrestrial Ring Current - ESA Space ...

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[Ebihara and Ejiri, JGR,105, 15843, 2000]<br />

In <strong>the</strong> equatorial plane <strong>the</strong> state <strong>of</strong> a particle is<br />

characterized by 4 variables: R, φ (MLT), W, α ο.<br />

The elementary volume in this 4-dimensional phase<br />

space is: δV=δxδp<br />

The phase space density is: fo =δN/δV<br />

where δN is <strong>the</strong> number <strong>of</strong> ga<strong>the</strong>red particles falling into<br />

<strong>the</strong> phase space bin<br />

The directional differential flux is: j o =p 2 f o<br />

an <strong>of</strong>f-equatorial differential flux j at a latitude λ can be<br />

derived by adiabatic expansion<br />

Alpbach Summer School, 2002

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