PPT-m m-wave and THz acceleration

Steven Jamison Lancaster University amp UK mmwave acceleration steering group SP Jamison High Gradient Accelerator T ownhall 31 st May 2021 Lancaster University University of . Time Ti me s ec onds Acceleratio m eterssec2 brPage 7br JMP Acceleration in Human Terms Acceleration in Human Terms What are some g reference points Description g level brPage 8br JMP Whats the point Whats the point Why measure acceleration brPage 9 2014 . Device Research Conference, June 22-24, Santa Barbara, CA.. M.J.W. Rodwell, UCSB. S. Lee, C.-Y. Huang, D. Elias, V. Chobpattanna, J. Rode, . H.-W. Chiang, P. Choudhary, R. Maurer, , A.C. Gossard, . Meeting. Siegen, February 23, 2016 . Summary of activities. Frankfurt. Hartmut G. . R. oskos. Key Points. Scientific Work . Report . D.1.7 (and 3.3). Publication(s). Information Policy. Financial Aspects . Beating . in Rubidium at 2.1 THz and 18.2 THz:. Long-Range Rb. *. -Rb Interactions.. WILLIAM . GOLDSHLAG. , BRIAN . J. . RICCONI, J. GARY EDEN. Laboratory for Optical Physics and Engineering,. Department of Electrical and Computer Engineering, . Peng Wang, Sergey . Shilov, Bruker . Optics, Bruker Corporation. Key components of FTIR spectrometer. Two internal sources. The standard MIR source . Glowbar. provides wide spectral range. Two detector options. Bell Ringer 11-7-13. Compare and Contrast Speed, Velocity and Acceleration. is the speed of an object in a particular direction. MYP Unit Question: What Moves YOU!!. Area of Interaction: Human Ingenuity. Acceleration is a change in velocity. Speed or direction. Centripetal Acceleration. Acceleration can mean a change in direction, not just speed. Centripetal acceleration. Acceleration that occurs in a circular motion. What is acceleration?. If you’re traveling in a car at a constant speed of 50 mph, are you accelerating?. No, you’re not. . Acceleration is the rate of change of velocity. . Acceleration. In order for acceleration to occur, velocity MUST be . SOFIA Tele-Talk. Paul Goldsmith. Imran Mehdi,. Jose . Siles. , Jon Kawamura. Jet Propulsion Laboratory. January 22, 2014. 1. Outline. Objectives and Goals. Objectives and goals of investigation. Submillimeter Tracers of High-Mass Star Formation. Siming. Liu. University of Glasgow. Collaborators. Vahe. ’ . Petrosian. , . Yanwei. Jiang: Stanford University. Zhonghui. Fan: Yunnan University. Oct. 2008 Krakow, Poland . Outline. I: Observations: Distribution. RIGI-DS202Non-destructive testingIndustrial process controlSensitive to Toptica AG TDS spectrometersImage using QCL THz sourceFrequency 46 THzPower 06 0WIntegration time 50 sAcquisition Single shotPi ELI-ALPS . laser. . facility. The ELI . project. :. a. . laser. . user. . facility. . at. 3 . sites. 3 . complimentary. . pillars. (CZ+HU+RO). Mission. of . the. ELI-ALPS . pillar. :. . generate. SASE FEL at . PITZ with 3D PIC code WARP. Background. Simulation results with Warp. Conclusion. Xiangkun. . LI. DESY-TEMF winter . meeting. DESY. , . Hamburg, 28.11.2019. B. ackground. A . proof-of-principle experiment on . . Electron. . Diffraction. , . 17 . June. 2019, PSI, . Switzerland. . THz . Sources. :. . Key . Enabling. . Technology. . for. . Novel. . Accelerators. Institute of . Physics. www.physics.ttk.pte.hu.