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July 14, 20052005 SHINE WorkshopKeauhou, Hawaii, USA
É but wait Ð thereÕs more!
Key processes of interplanetary transport
• Scattering
• Focusing (a.k.a. mirroring)
• Solar wind effects
- Convection
- Adiabatic deceleration
Note: mean free path is ~ 0.1 to 3 AU
Aim to quantitatively explain profiles of intensity & anisotropy vs. time
[Jokipii 1966]
[Roelof 1969]
[DR 1995]