PowerPoint Presentation - Shock Acceleration of Cosmic Rays in Various Astrophysical Situations การเร่งของรังสีคอสมิกที่คลื่นกระแทก ในสถานการณ์ต่างๆ ทางดาราศาสตร์

July 14, 2005 2005 SHINE Workshop Keauhou, Hawaii, USA

… but wait – there’s more!
Key processes of interplanetary transport

ï Scattering

ï Focusing (a.k.a. mirroring)

ï 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]


	ïIf the mean free path were much smaller than 1 AU, the distance …, then you could use the diffusion approx. …
	ïIf much larger, free streaming
	ïBut when the mean free path is of the same order as the distance of interest, the problem is more difficult