PPT-High finesse multi-mirror optical cavities

with feedback Fabry Perot cavity in cw mode feedback amp optical issues Comparison with Sapphire parameters Fabry Perot cavity in pulsed mode Comparison with Sapphire parameters Present . brPage 3br mirror mirror object reconstruction beam virtual mirror photo film brPage 5br film virtual image brPage 6br incident light line of view initial position loaded position Fleming NuINT 2004 Gran Sasso Laboratory brPage 2br Motivation for the FINeSSE scibath detector Low energy neutrino scattering physics below DIS Lots of physics to do at these low energies form factor measurements cross section measurements short ba Aims. Bridge. 1) Introduction to Bridge. Probability. 2) Number of Bridge hands. 3) Odds against a Yarborough. 4) Prior probabilities: Suit-Splits and Finesse. 5) Combining probabilities: Suit-Splits and Finesse. Sarah Gibson, . Giuliana. de . Toma. , Therese . Kucera. , Kathy Reeves, Donald . Schmit. , and Alphonse Sterling. Abstract. Coronal . mass ejections (. CMEs. ) and associated prominence eruptions are spectacular manifestations of the Sun's magnetic energy.  Elliptical regions of rarefied density, or cavities, are commonly observed surrounding coronal prominences, both quiescent and erupting.  The prominence-cavity system is structured by magnetism, providing clues to to the processes that destabilize these . April 2012 High finesse optical cavities R. Martin, G. Mueller, and D.B. Tanner University of Florida Margot Phelps, Liyuan Zhang, G. Billingsley and D. Reitze Caltech Vistas in Axion Physics April 2 On The Shelf. We’re studying lessons from. James to Christians which. have been scattered.. Thesis :. Christians must seek out . God’s standard and alter. their lives to conform.. James 1: 22-25. OPTICAL STRAIN GAUGE. . Marten’s mirror extensometer. Tuckerman optical strain gauge. Marten’s mirror extensometer. Working Principle. To measure Elongation. Developed by Peterson and Wahl in 1936. Segment Optics and Space Instruments. 1 . Department of Electrical and Telecommunications Engineering, New York City College of Technology. 2. Instrument Systems and Technology, Optics Division, NASA Goddard Space Flight Center. 5: Optical Resonant Cavities. Prof. Juejun (JJ) Hu. hujuejun@udel.edu. Optical resonance and resonant cavities. Optical resonant mode. A time-invariant, stable electromagnetic field pattern (complex amplitude): an . Foundation Standard 1: Academic Foundation . Understand human anatomy, physiology, common . diseases . and. disorders. , and medical math principles.. 1.13 . Analyze basic structures and functions of human . pathfinder Dual-Mirror telescope for the CTA-SST array . Rodolfo . Canestrari. . for the . ASTRI. collaboration. INAF. -Astronomical Observatory of . Brera. An overview on the optical design, telescope structure & . Joseph M. Howard, Garrett J. West. Optics Branch, Code 551, GSFC NASA. Agenda. Optical Design Lab (ODL). Optical Specifications. Refractive vs. Reflective. Freeform Optics. Examples. 2. Welcome to the ODL!!. Peter . Kneisel. Jefferson Lab. May 19, 2014. Since I believe that I am much better in talking about the past than “predicting” the future - my view is clouded by the past 47 years – I will start with some remarks about the past. beam. . power. 1979. What. do . we. . call. as High . Power. . Linac. ?. Beam. . power. . vs . Beam. . average. . power. I x E . x . duty. . cycle. but. . energy. . is. . measured. in .