'Code comparison' presentation slideshows

Chapter 17

Chapter 17. Code Review, Test Data, and Code Comparison. Audit Evidence Collection and Evaluation. What was expected to happen / not happen? What did happen?/not happen? What type of evidence do we have? Is the evidence reliable? What is the exposure and $ of risk.

460 views • 27 slides

Studying Cosmic acceleration and neutrino masses with DES. http://www.darkenergysurvey.org

Studying Cosmic acceleration and neutrino masses with DES. http://www.darkenergysurvey.org. Outline DES: what is it and update + probes used Dark energy from DES. Neutrino masses from DES. Filipe Batoni Abdalla. Future Dark Energy Surveys. WFIRST. The Dark Energy Survey (DES). Proposal:

388 views • 23 slides

Presented by K.Gokulprabhu & N.Kumaresan

Code Comparison between IS456-2000 and ACI 318. Presented by K.Gokulprabhu & N.Kumaresan. General basic comparison. Slender Columns with biaxial bending Isolated footing with Moment Click.

234 views • 15 slides

A comparison of radiation transport and diffusion using PDT and the CRASH code Fall 2011 Review

A comparison of radiation transport and diffusion using PDT and the CRASH code Fall 2011 Review. Eric S. Myra Wm. Daryl Hawkins. Our goal is to quantify error associated with using flux-limited diffusion in CRASH. Key goals:

242 views • 14 slides

T.G. Theofanous Center for Risk Studies and Safety University of California, Santa Barbara

STEAM EXPLOSIONS. T.G. Theofanous Center for Risk Studies and Safety University of California, Santa Barbara. Risk Complexity An Approach Based on Key Physics (ROAAM). Propagation Key Physics. Multiphase Thermal Detonation: Microinteractions. FUEL. NON-PARTICPATING COOLANT.

250 views • 14 slides

SPRINT

SPRINT. A S imple P arallel R INT erface. Overview. What is SPRINT How is SPRINT different from other parallel R packages Biological example: Post-genomic data analysis Code comparison. SPRINT. S imple P arallel R INT erface ( www.r-sprint.org )

452 views • 12 slides

Turbulence and Dissipation in the Solar Wind Plasma

Session Summary for Session 13:. Turbulence and Dissipation in the Solar Wind Plasma. Current Challenges and New Diagnostics. Chadi Salem (1) & Tulasi Parashar (2). Space Sciences Laboratory, University of California, Berkeley, CA University of Delaware, Newark, DE.

106 views • 10 slides

Svetlana Y. Kotchenova 1 , Eric F. Vermote 1,2 , Philip A. Farris 1 , & Jose G. Roa 1

206 views • 1 slides