'Velocity structure' presentation slideshows

Accretion Disk MHD Winds as X-ray Absorbers in AGN and GBHC

Accretion Disk MHD Winds as X-ray Absorbers in AGN and GBHC. Demos Kazanas with Keigo Fukumura Ehud Behar (Technion) John Contopoulos (Academy of Athens). ApJ (2010), 715, 636 (FKCBa) ApJ (2010), 723, L228 (FKCBb). Credit: NASA/CXC. Acknowledgements to:. J. Garcia (CUA/GSFC)

666 views • 53 slides

EART162: PLANETARY INTERIORS

477 views • 32 slides

Broadband Ground Motion Simulations for a Mw 7.8 Southern San Andreas Earthquake: ShakeOut

Broadband Ground Motion Simulations for a Mw 7.8 Southern San Andreas Earthquake: ShakeOut. Robert W. Graves (URS Corporation) Brad Aagaard (US Geological Survey, Menlo Park) Ken Hudnut (US Geological Survey, Pasadena). Support: SCEC (USGS, NSF) USGS

353 views • 22 slides

Philamentary Structure and Velocity Gradients in the Orion A Cloud

Red: CO from Mini survey. Philamentary Structure and Velocity Gradients in the Orion A Cloud. Spitzer Orion Cloud Survey: 10 sq. degrees in Orion A and Orion B mapped between 2004-2009 IR-ex: 3352 IR-ex + coup: 3845 IR-ex + coup + corr: 4300 Megeath et al. (y+1) y = current year. Orion B.

391 views • 20 slides

S eismic wave P ropagation and I maging in C omplex media: a E uropean network

S eismic wave P ropagation and I maging in C omplex media: a E uropean network. RENETA BLAGOEVA RAYKOVA Experienced Researcher Host Institution: INGV Bologna Place of Origin: Sofia, Bulgaria Appointment Time: November 2005

201 views • 6 slides

Lunar interior

Lunar interior. Yao Yao. Earthquake Seismograms. Moonquake Seismograms. Outstanding Questions. Apollo seismic data has not yet been completely used Some moonquake nests were incorrectly classified What is the vertical structure of the Lunar Crust? Any discontinuity layers?

154 views • 6 slides