'Radiation transfer' presentation slideshows

Spectroscopic observations of Lyman ? emitters in the Local Universe

757 views • 60 slides

Monte Carlo Radiation Transfer in Circumstellar Disks

Monte Carlo Radiation Transfer in Circumstellar Disks. Jon E. Bjorkman Ritter Observatory. Systems with Disks. Infall + Rotation Young Stellar Objects (T Tauri, Herbig Ae/Be) Mass Transfer Binaries Active Galactic Nuclei (Black Hole Accretion Disks) Outflow + Rotation (?)

688 views • 47 slides

513 views • 39 slides

396 views • 39 slides

Super-Eddington Accretion: Models and Applications

Super-Eddington Accretion: Models and Applications. Jian-Min Wang Institute of High Energy Physics 2005, 4, 26. Implications of SEA. Theoretical: one branch of accretion modes stable Applications: micro-quasars narrow line Seyfert 1 galaxies

538 views • 34 slides

Jim Stone Princeton University

356 views • 32 slides

Sternentstehung - Star Formation

Sternentstehung - Star Formation. Sommersemester 2006 Henrik Beuther & Thomas Henning. 24.4 Today: Introduction & Overview 1.5 Public Holiday: Tag der Arbeit 8.5 --- 15.5 Physical processes, heating & cooling, cloud thermal structure

337 views • 23 slides

Why Massive Black Holes are Small in Disk Galaxies ?

Why Massive Black Holes are Small in Disk Galaxies ?. Nozomu KAWAKATU Center for Computational Physics, University of Tsukuba. Collaborator. Masayuki UMEMURA. Center for Computational Physics, University of Tsukuba.

286 views • 20 slides

Variation of land surface albedo and its simulation

Earth Sciences Sector. Variation of land surface albedo and its simulation. Reducing Canada's vulnerability to climate change. Shusen Wang Andrew Davidson Canada Centre for Remote Sensing. Acknowledgment: CCAF, PFRA, BOREAS. Albedo and climate control surface radiation and energy balances

295 views • 18 slides

Accelerated Lambda Iteration

Accelerated Lambda Iteration. Motivation. Complete Linearization provides a solution scheme, solving the radiation transfer , the statistical equilibrium and the radiative equilibrium simultaneously.

282 views • 14 slides

Accelerated Lambda Iteration

Accelerated Lambda Iteration. Motivation. Complete Linearization provides a solution scheme, solving the radiation transfer , the statistical equilibrium and the radiative equilibrium simultaneously.

142 views • 14 slides

The Ionization of the Local Interstellar Cloud

The Ionization of the Local Interstellar Cloud. Jonathan Slavin Harvard-Smithsonian Center for Astrophysics. The Need for LIC Ionization Modeling. Heliosphere models rely on n e and n H as inputs (along with B ISM , v ISM , etc.)

260 views • 13 slides

Monte Carlo simulation of radiation transfer in optically anisotropic clouds

265 views • 11 slides

117 views • 11 slides

3. Radiation Field Basics II

3. Radiation Field Basics II. Rutten: 2.1, 2.2 Intensity moments Emission, extinction, source function Equation of radiation transfer Optical depth. Moments of the Radiation Field. We have defined the moment operator M operating on f :.

96 views • 9 slides

Test question 16.1

130 views • 5 slides

3D Radiation Hydrodynamics

P5. P3. Source. Target. P2. E4. E1. E2. E3. E5. P1. P4. Radiation Hydrodynamics with HMCS. HMCS realizes 3D Radiation Hydrodynamics. ? CP-PACS solves Smoothed Particle Hydrodynamics (SPH) and Radiation Transfer.

194 views • 2 slides