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Theory of Shock Acceleration of Hot Ion Populations. Marty Lee Durham, New Hampshire USA. Current Issues & Challenges. Theory of Planar Stationary Diffusive Shock Acceleration Injection Rates and Injection Thresholds “Hot” and “Cold” Seed Particle Populations Quasilinear Wave Excitation
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Theory of Shock Acceleration of Hot Ion Populations Marty Lee Durham, New Hampshire USA
Current Issues & Challenges • Theory of Planar Stationary Diffusive Shock Acceleration • Injection Rates and Injection Thresholds • “Hot” and “Cold” Seed Particle Populations • Quasilinear Wave Excitation • Ion Fractionation Upstream of the Shock • Power-law Index: Observations Versus Theory • Varying Magnetic Obliquity Within an Event • Geometry: Earth’s Bow Shock & Solar Wind Termination Shock • Nonlinear Waves & SLAMS
Current Issues & Challenges • Theory of Planar Stationary Diffusive Shock Acceleration • Injection Rates and Injection Thresholds • “Hot” and “Cold” Seed Particle Populations • Quasilinear Wave Excitation • Ion Fractionation Upstream of the Shock • Power-law Index: Observations Versus Theory • Varying Magnetic Obliquity Within an Event • Geometry: Earth’s Bow Shock & Solar Wind Termination Shock • Nonlinear Waves & SLAMS
Injection and Shock Obliquity Tylka et al., 2005
Anisotropy Limitation Giacalone and Jokipii, 1999
“Energetic Storm Particle” Event Complexity Van Nes et al., 1984
Ion Features Van Nes et al., 1984
ACE Shock Survey Lario et al., 2005
Quasi-Perpendicular Shock Simulation Giacalone, 1999
Shock Energetic Particle Correlation Lengths Neugebauer et al., 2006
Current Issues & Challenges • Theory of Planar Stationary Diffusive Shock Acceleration • Injection Rates and Injection Thresholds • “Hot” and “Cold” Seed Particle Populations • Quasilinear Wave Excitation • Ion Fractionation Upstream of the Shock • Power-law Index: Observations Versus Theory • Varying Magnetic Obliquity Within an Event • Geometry: Earth’s Bow Shock & Solar Wind Termination Shock • Nonlinear Waves & SLAMS
Example Event:1999 / 47-49(Cold Seeds) Density compression: d/u ~ 2.9 Clear proton foreshock of appropriate scale. Softening particle spectra on the same ESP scale. Particle intensity index appropriate to shock strength. Small proton anisotropy. Wave foreshock appropriate scale. Argued and confirmed to be cold ion seed population leading to shock acceleration.
Example Event:1998 / 217-219(Hot Seeds) Density compression: d/u ~ 1.8 Very modest or questionable proton foreshock if SEP event is properly recognized. Softening particle spectra on SEP scale. Moderate proton anisotropy. Nonexistent wave foreshock. Argued and confirmed to be hot ion seed population leading to shock acceleration.
Current Issues & Challenges • Theory of Planar Stationary Diffusive Shock Acceleration • Injection Rates and Injection Thresholds • “Hot” and “Cold” Seed Particle Populations • Quasilinear Wave Excitation • Ion Fractionation Upstream of the Shock • Power-law Index: Observations Versus Theory • Varying Magnetic Obliquity Within an Event • Geometry: Earth’s Bow Shock & Solar Wind Termination Shock • Nonlinear Waves & SLAMS
Wave Excitation - III = 7; I0(k) 0
Current Issues & Challenges • Theory of Planar Stationary Diffusive Shock Acceleration • Injection Rates and Injection Thresholds • “Hot” and “Cold” Seed Particle Populations • Quasilinear Wave Excitation • Ion Fractionation Upstream of the Shock • Power-law Index: Observations Versus Theory • Varying Magnetic Obliquity Within an Event • Geometry: Earth’s Bow Shock & Solar Wind Termination Shock • Nonlinear Waves & SLAMS
Ion Fractionation Tylka et al., 1999
Current Issues & Challenges • Theory of Planar Stationary Diffusive Shock Acceleration • Injection Rates and Injection Thresholds • “Hot” and “Cold” Seed Particle Populations • Quasilinear Wave Excitation • Ion Fractionation Upstream of the Shock • Power-law Index: Observations Versus Theory • Varying Magnetic Obliquity Within an Event • Geometry: Earth’s Bow Shock & Solar Wind Termination Shock • Nonlinear Waves & SLAMS
Complications within DSA Wave-frame compression ratio: Van Nes et al., 1984
Current Issues & Challenges • Theory of Planar Stationary Diffusive Shock Acceleration • Injection Rates and Injection Thresholds • “Hot” and “Cold” Seed Particle Populations • Quasilinear Wave Excitation • Ion Fractionation Upstream of the Shock • Power-law Index: Observations Versus Theory • Varying Magnetic Obliquity Within an Event • Geometry: Earth’s Bow Shock & Solar Wind Termination Shock • Nonlinear Waves & SLAMS
Fe/O Versus Energy Tylka et al., 2005
A Simple Model for Composition Tylka and Lee, 2006
Fe/O Versus Energy Tylka and Lee, 2006
Current Issues & Challenges • Theory of Planar Stationary Diffusive Shock Acceleration • Injection Rates and Injection Thresholds • “Hot” and “Cold” Seed Particle Populations • Quasilinear Wave Excitation • Ion Fractionation Upstream of the Shock • Power-law Index: Observations Versus Theory • Varying Magnetic Obliquity Within an Event • Geometry: Earth’s Bow Shock & Solar Wind Termination Shock • Nonlinear Waves & SLAMS
The Blunt Termination Shock McComas and Schwadron, 2006
Current Issues & Challenges • Theory of Planar Stationary Diffusive Shock Acceleration • Injection Rates and Injection Thresholds • “Hot” and “Cold” Seed Particle Populations • Quasilinear Wave Excitation • Ion Fractionation Upstream of the Shock • Power-law Index: Observations Versus Theory • Varying Magnetic Obliquity Within an Event • Geometry: Earth’s Bow Shock & Solar Wind Termination Shock • Nonlinear Waves & SLAMS
Upstream Waves Hoppe et al., 1981
SLAMS Lucek et al., 2008