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By shengArtifacts in the characterization of skin layers and ultrathin films by X-ray diffraction. D. Pesquera , F. Sanchez, G. Herranz , J. Fontcuberta ICMAB, Barcelona. X. Marti , V. Holy Charles University, Prague P. Ferrer , T. Schulli ESRF, Grenoble J. Herrero-Albillos
By allaynaGEOMETRICAL DESIGN STUDIES. ACOUSTICS OF CONCERT HALLS AND ROOMS. Handbook of Acoustics, Chapter 9 Long, Architectural Acoustics, Chapter 19. THE LISTENING ENVIRONMENT. • STRONG LATERAL REFLECTIONS SO AUDIENCE FEELS ENVELOPED • A STRONG REVERBERANT FIELD
By yaphetThe Imaging Chain for X-Ray Astronomy. Pop quiz (1): Which is the X-ray Image?. B. A. Answer: B!!! (But You Knew That). B. A. Pop quiz (2): Which of These is the X-Ray Image?. A. B. C. The dying star (“planetary nebula”) BD +30 3639. Answer = C! ( Not So Easy!). A. C. B.
By kaponoUV laser-induced damage to grazing-incidence metal mirrors. M. S. Tillack, J. Pulsifer, K. Sequoia. 4th US-Japan Workshop on Laser-Driven Inertial Fusion Energy Technology Osaka University March 13-15, 2003. Design concept for a grazing-incidence metal mirror.
By cedricLinac Coherent Light Source Update John N. Galayda 22 July 2002. Project scope Cost estimate DOE Review 23-25 April - results Future. L INAC C OHERENT L IGHT S OURCE. I-280. Sand Hill Rd. N. S. N. S. N. S. N. N. S. N. S. N. S. N. S. N. N. N. N. S. S. S. S. N. N.
By lanaiAstronomers Learn to Work in Space. Detectors Pointing and Stability Data Storage Contamination Thermal Control Background radiation. Technical Challenges. V-2 Rocket October 10, 1946 Ultraviolet spectrum of sun 340 nm – 240 nm Bead entrance UV film. First Astronomy from Space.
By anktiMAXIM Pathfinder. Keith Gendreau, Webster Cash, Ann Shipley, and Nick White. MAXIM Pathfinder. Science Goals Provide Scientific Context for MAXIM Study stellar coronae, AGN jets, accretion disks, and more Technical Role and Issues
By daciaEUS Meeting March, 3rd 2006. Grazing-incidence vs. normal-incidence design. L. Poletto CNR - National Institute for the Physics of Matter Department of Information Engineering - Padova (Italy). slit. spectrometer. telescope. detector. Normal-incidence vs. grazing-incidence design (1/2).
By lane-gillespiePolarization Modulation with PEM for CD (courtesy Hinds Instr.). Linear Dichroism Schematic (courtesy Hinds Instr.). Spectrometer UV or IR. Linear polarizer. PEM. Variable angle of incidence. Linear Dichroism - Reflection (IRRAS) (courtesy Hinds Instruments).
By cambree-jonesX-ray Interferometry. The Future of X-ray Astronomy. Webster Cash University of Colorado. Co-Investigators. Steve Kahn - Columbia University Mark Schattenburg - MIT David Windt – Columbia University Dennis Gallagher – Ball Aerospace. A Sufficiently Good Image is Like a Visit.
By giselle-barreraMAXIM: The Blackhole Imager. Keith Gendreau Study Scientist Code 662 NASA Goddard Space Flight Center. Fiscal Year 2002 IRAD Colloquium…Science and Technology Accomplishments: Dec. 2002. Science Driver for MAXIM.
By jelani-mooreLinac Coherent Light Source Update John N. Galayda 22 July 2002. Project scope Cost estimate DOE Review 23-25 April - results Future. L INAC C OHERENT L IGHT S OURCE. I-280. Sand Hill Rd. N. S. N. S. N. S. N. N. S. N. S. N. S. N. S. N. N. N. N. S. S. S. S. N. N.
By amandawhalenMAXIM: The Blackhole Imager. Keith Gendreau Study Scientist Code 662 NASA Goddard Space Flight Center. Fiscal Year 2002 IRAD Colloquium…Science and Technology Accomplishments: Dec. 2002. Science Driver for MAXIM.
By gordonrNuSTAR , ITS BACKGROUND AND CLUSTERS OF GALAXIES. FABIO GASTALDELLO INAF, IASF-Milano And The Galaxy Clusters NuSTAR Team. The NuSTAR satellite and its focusing capabilities in the hard X-ray band NuSTAR science with galaxy clusters: IC emission and very hot thermal emission
By collierpNormal Laser Incidence on Cathode D. H. Dowell, SLAC LCLS Week July 19, 2005. Grazing vs. Normal Incidence Issues Grazing Incidence Technical Risk Schemes for Normal Incidence Wakes Mechanical Layout Costs Summary. Grazing Incidence vs. Normal Incidence. Grazing Incidence Optical System.
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