'Scale structures' presentation slideshows

Characterization of Materials using the PDF

Characterization of Materials using the PDF. Thomas Proffen Manuel Lujan Jr. Neutron Scattering Center Los Alamos National Laboratory tproffen@lanl.gov. LA-UR 05-0111. Why do we care about the atomic structure?. Diamond hard transparent insulating expensive Graphite soft black

809 views • 57 slides

MADRID LECTURE # 5

MADRID LECTURE # 5. Numerical solution of Eikonal equations. 1. Historical Background. Motivated by the analysis of nonlinear models from micro-Mechanics and Material. Science , B. Dacorogna (EPFL-Math) was lead to investigate the properties of the solutions (including the

401 views • 34 slides

Cosmology from Topology of Large Scale Structure of the Universe

RESCEU 2008. Cosmology from Topology of Large Scale Structure of the Universe. RESCEU Symposium on Astroparticle Physics and Cosmology 11-14, November 2008 Changbom Park (Korea Institute for Advanced Study). Why is the topology study useful?. Direct intuitive meanings

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Phasing ALMA for VLBI: Building an Event Horizon Telescope

Phasing ALMA for VLBI: Building an Event Horizon Telescope. Big Questions. Is there an Event Horizon? Does GR hold near BH? How does matter accrete/outflow near a BH? Do Black Holes have spin? How do Black Holes launch jets? EHT addresses ASTRO 2010 questions and discovery areas:

505 views • 31 slides

Optical Observations of High-Latitude Clouds

Optical Observations of High-Latitude Clouds. Adolf N. Witt University of Toledo. Collaborators: Steve Mandel, Hidden Valley Obs., Soquel, CA Thomas G. Dixon, Univ. of Hertfordshire, UK Paul H. Sell, Univ. of Toledo Karl D. Gordon, Univ. of Arizona Uma P. Vijh, STScI With support from:

341 views • 24 slides

Development of music perception

Development of music perception. Dowling, W.J. (1999). Development of music perception and cognition . In Deutsch, D. The Psychology of Music, Chapter 15. A. Infancy. Prenatal experience Perceptual grouping Pitch Melodic pitch patterns Rhythm. Prenatal experience.

443 views • 23 slides

Public Star Party

Public Star Party. Organized by Institute for Astronomy, University of Hawaii. Contact person: Prof. Jim Heasley. When? Tonight between 8:30 and 10 pm Where? Kapiolani Park, Honolulu How to get there? Intersection Paki Avenue with Noela Street What about the weather? Check 956-6195.

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Yusei Koyama (NAOJ)

TMT science workshop @ Asahi- seimei building , 16/ 10/2013. From MAHALO-Subaru to ALOHA-TMT: unveiling internal physics of distant galaxies across environment. Yusei Koyama (NAOJ).

354 views • 17 slides

The International Heliophysical Year and Universal Processes In Space Science

Heliospheric Plasma Physics. A Universal Science. The International Heliophysical Year and Universal Processes In Space Science. Howard J. Singer NOAA Space Environment Center. Review of North American Science Plans Universal Processes and IHY Science .

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Los Alamos National Laboratory Wins Four 2005 R&D 100 Awards

U N C L A S S I F I E D. U N C L A S S I F I E D. Los Alamos National Laboratory Wins Four 2005 R&D 100 Awards. CartaBlanca: A High-Efficiency, Object-Oriented, General-Purpose Computer Simulation Environment MESA: Measuring Enzyme-Substrate Affinities

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Cosmic Microwave Background

Cosmic Microwave Background. Detecting CMB. Approximately 1% of the static noise created by an untuned radio is from the CMB. This is the same for old, untuned television sets.

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The emergence of band structure in nanoscale insulators Jay A. Gupta, Ohio State University Research Foundation, DMR 064

The emergence of band structure in nanoscale insulators Jay A. Gupta, Ohio State University Research Foundation, DMR 0645451

698 views • 2 slides

National Science Foundation Industry/University Cooperative Research Center

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K.Kleidis, D. B.Papadopoulos*, L.Vlahos Aristotle University of Thessaloniki, 54124 Greece

159 views • 1 slides