|
|
18-21 November, 2009 |
|
|
|
|
|
|
Scientific Program and Presentation Files |
PHOTOS |
|
|
Scientific Rationale |
|
|
|
- Collisionless shocks are ubiquitous in astrophysical environments.
Many astrophysical phenomena are governed by them.
|
|
|
|
- In this workshop, turbulence and particle acceleration at astrophysical shocks are to be discussed. |
|
|
|
- Topics to be covered |
|
1. Collisionless shocks in astrophysical environments including shocks in heliosphere, supernova
remnants, AGN jets, gamma-ray bursts, and the large scale structure of the universe |
|
2. Instabilities at shocks, turbulent flow motions around shocks |
|
3. Magnetic field amplification at shocks, particle acceleration at shocks |
|
4. Simulations : DSA, Monte Carlo, hybrid, PIC, etc |
|
|
|
|
|