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

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E Alpbach Summer School, 2002 Modeled storm time evolution <strong>of</strong> H + mean kinetic energy = 1 2 m ∞ ∫ 0 ∞ ∫ 0 f f (@ 90 o Pitch angle) ( v) ( v) v v 4 2 dv dv Reference model Alpbach Summer School, 2002
ε = 1 2 Alpbach Summer School, 2002 Modeled storm time evolution <strong>of</strong> ∞ ∫ 0 ( ) m f v energy density: v 4 dv Reference model Alpbach Summer School, 2002
Page 1 and 2: Global Monitoring of the Terrestria
Page 3 and 4: Alpbach Summer School, 2002 gyratio
Page 5 and 6: Alpbach Summer School, 2002 Conside
Page 7 and 8: Ring Current sources Inward transp
Page 9 and 10: [Ebihara and Ejiri, JGR,105, 15843,
Page 11 and 12: Model inputs H + data from geosynch
Page 13 and 14: ASTRID (SAC-B) CASSINI PROCESSES IN
Page 15 and 16: Alpbach Summer School, 2002 ENA flu
Page 17 and 18: Alpbach Summer School, 2002 Alpbach
Page 19 and 20: (fm fm.: .: D. Mitchell et al., Yos
Page 21 and 22: IMAGE Era Accomplishments in Substo
Page 23 and 24: Model validation. Comparison of the
Page 25 and 26: Modeled Storm Time Evolution Of Equ
Page 27 and 28: Alpbach Summer School, 2002 H + Flu
Page 29 and 30: Alpbach Summer School, 2002 Modeled
Page 31: ∞ ∫ 0 Alpbach Summer School, 20
Page 35 and 36: Alpbach Summer School, 2002 SUMMARY
Page 37: [Ebihara and Ejiri, JGR,105, 15843,

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