'Loss cone' presentation slideshows

Radiation Belt Variability John Sample Space Sciences Laboratory

Radiation Belt Variability John Sample Space Sciences Laboratory University of California, Berkeley. Outline: Introduction to the Radiation Belts Structure Variability Invariants Importance of magnetic field models Acceleration Processes ULF Local Wave Heating Loss Processes

516 views • 40 slides

Dynamics of Galactic Nuclei

Dynamics of Galactic Nuclei. MODEST 6 Evanston, 2005. M B < -20. ?. ? ~ R - ? ? < 0.5. Sersic n > 4. R. M B < -20. ?. ? ~ R - ? ? < 0.5. Sersic n > 4. R. Sersic n ? 4. M B < -20. -18 < M B < -20. ? ~ R - ? 0.5 < ? < 1.2. ?. ? ~ R - ? ? < 0.5. Sersic n > 4.

421 views • 31 slides

Radiation Belt Relativistic Electron Loss Processes

422 views • 23 slides

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323 views • 17 slides

Astrophysics of Captures

Astrophysics of Captures. Steinn Sigurdsson Dept Astro & Astrop, & CGWP Penn State. M BH >> m *. Consider supermassive black holes in centres of galaxies. M BH ~ 10 6 M sun Surrounded by a dense cluster of stars

295 views • 17 slides

Exploring the MEO Space Particle Regime

Exploring the MEO Space Particle Regime. Briefing to the National Space Weather Program Assessment Team 6 Jan 2006. Gregory Ginet AFRL/VSBX Space Vehicles Directorate Air Force Research Laboratory. Exploring MEO Why Bother?.

379 views • 17 slides

Exploring the MEO Space Particle Regime

Exploring the MEO Space Particle Regime. Briefing to the National Space Weather Program Assessment Team 6 Jan 2006. Gregory Ginet AFRL/VSBX Space Vehicles Directorate Air Force Research Laboratory. Exploring MEO Why Bother?.

461 views • 17 slides

Astrophysics of Captures

Astrophysics of Captures. Steinn Sigurdsson Dept Astro & Astrop, & CGWP Penn State. M BH >> m *. Consider supermassive black holes in centres of galaxies. M BH ~ 10 6 M sun Surrounded by a dense cluster of stars

197 views • 17 slides