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

More documents

Recommendations

Info

MANY THANKS FOR YOUR ATTENTION! (IFSI web site http://www.ifsi.rm.cnr.it) Alpbach Summer School, 2002 Alpbach Summer School, 2002
[Ebihara and Ejiri, JGR,105, 15843, 2000] In the equatorial plane the state of a particle is characterized by 4 variables: R, φ (MLT), W, α ο. The elementary volume in this 4-dimensional phase space is: δV=δxδp The phase space density is: fo =δN/δV where δN is the number of gathered particles falling into the phase space bin The directional differential flux is: j o =p 2 f o an off-equatorial differential flux j at a latitude λ can be derived by adiabatic expansion 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 and 32: ∞ ∫ 0 Alpbach Summer School, 20
Page 33 and 34: ε = 1 2 Alpbach Summer School, 200
Page 35: Alpbach Summer School, 2002 SUMMARY

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

Create successful ePaper yourself

Delete template?

Save as template?