1. Auxiliary slides

3. ISEE-1

4. ISEE-2

5. ISEE-1

6. B Locus of  = 90 degree pitch angles Will plot as a sinusoid on a latitude/longitude projection of the unit sphere ISEE-1 Energetic particle WAPS sensor

7. 24 keV < E < 45 keV

8. 63 keV < E < 95 keV

9. 142 keV < E < 210 keV

10. 24 keV < E < 45 keV

11. 63 keV < E < 95 keV

12. 142 keV < E < 210 keV

16. This and the another ISEE event described by Whitaker et al. [2006, 2007] are “smoking gun” events that establish that processes in the cusp accelerate particles in-situ to ring current energies. The questions that now remain are what effects, if any, these particles have on magnetospheric processes? Are they the source of the ring current via gradient and curvature drifts to the nightside inner magnetosphere? Do these particles create, via charge separation, the cross polar-cap potential? Conclusions

17. The Butterfly Pitch Angle Distribution Particle intensity with respect to pitch angle Reduction of locally mirroring particles

18. Electrons Protons Fritz, Space Science Reviews,Vol 95: 469-488, 2001.

19. 26 October 1999 Electron PADs Electron intensities plotted as functions of both pitch angle and time The butterfly depression occurs nearly simultaneously across the energy spectrum Measured fluxes and the strength of the butterfly PAD are also nearly constant for all ten energy channels Energy Klida and Fritz, Ann Geophys. Submitted 2007

20. 26 October 1999 Ion PADs Energy Pronounced Butterfly PAD in the middle energy channels As the energy range decreases, butterfly PAD onset is observed later Multiple observed injections with intensities peaked at 90º pitch angle at lower energies Overall decrease in total measured counts as the energy channel increases Klida and Fritz, Ann Geophys. Submitted 2007

21. 26 October 1999 Ion PADs (15.6 keV to 35.4 keV) Klida and Fritz, Ann Geophys. Submitted 2007

22. Single Ion Modeling in a T96 Magnetosphere Solar Wind Density 4.85 cm -3 Solar Wind Velocity 473 km s -1 Bx (GSM)0.40 nT B y (GSM)2.81 nT B z (GSM)-3.76 nT X (GSM)-6.17 R E Y (GSM)1.85 R E Z (GSM)-0.34 R E Dst-33 Initial Conditions Starting position modeled backward in time Klida and Fritz, Ann. Geophys. Submitted 2007

23. The extraterrestrial ring current: Consider the variation of the prep and parallel pressure terms in this formula with a variable cusp source