PPT-Alpha Magnetic Spectrometer-02

Alpha Magnetic Spectrometer02 ISS Digital Data Recording System DDRS ISS DDRS Project ESCG Team Agenda Background Objectives Description Interface Diagram April 26 2010 ESCG 2 April 26 2010. In addition magnetic fields create a force only on moving charges The direction the magnetic field produced by a moving charge is perpendicular to the direction of motion The direction of the force due to a magnetic field is perpendicular to the dir A. Tannús – . 03/2011. IFSC - USP. Colóquio IFSC -. . Março. /2011. Major items of this talk:. Basic Principles;. Some methodologies for fast imaging;. NMR probes;. Digital NMR spectrometer. Basics. MICO 230. Steve Virostek. LBNL. August 7, 2013. Status of SS1. The magnet was cooled down to LHe temperature two weeks ago.. Iron shield with 60 cm hole has been mounted.. Low current testing (up to 50 A) revealed resistive behavior in the E2 coil 500 A HTS lead – worse than previous failed HTS lead.. Camera/photography. : . takes . images in . visible, infrared . and/or ultraviolet . light. . . REMOTE. Radar. : maps objects and their surface features (mountains/canyons, asteroids) . by sending . radio signals. Topic 2.2. Review of Topic 2.1. X. Mass Number (A). protons + neutrons. A. Atomic Number (Z). n. umber of protons. Z. n+/n-. Charge (n) . Atoms have no charge, so this is left blank.. Ions are atoms that have gained or lost electrons, the charge is indicated here.. Julie Cass. SULI Program 2011. SLAC National Accelerator Center. Advisor Josef Frisch. Overview of Spectrometer Optics . 90° . off-axis parabolic mirrors . (OAP) . . HeNe. laser . at 632.816 nm (visible) to align optics. Magnetic Forces. Objectives: . FLASHBACK. FLASHBACK: Sketch a stress-strain graph for a malleable materials and label a) the limit of proportionality b) the elastic limit c) the ultimate tensile strength d) the breaking point. Computation of transversal B-field on primary beam. CLIC main parameters. 9/25/2009. Detlef Swoboda. 2. Center of mass energy. 3 TeV. Peak Luminosity. 2. . 10. 34. cm. -2. s. -1. Repetition rate. Lab no. . 5. Introduction. The purpose of this instrument is to determine the amount of light of a specific wavelength absorbed by an . analyte. in a sample. . -Double beam spectrophotometer has . two light paths. muon. beam. A pair of identical, 3-m long spectrometer solenoids will provide a 4-tesla uniform field region at each end of the cooling channel. The . emittance. of the beam as it enters and exits the cooling channel will be measured within the 400 mm diameter magnet bores. The magnets incorporate a three-coil spectrometer magnet section and a two-coil section that matches the solenoid uniform field into the MICE cooling channel. The cold mass, radiation shield and leads are kept cold by means of a series of two-stage . Concept and Technology Development. © . 2013. CCAT. All Rights Reserved. .. CCAT Engineering Design Phase is partially supported by funding by the National Science Foundation’s Division of Astronomical . July 2011. Typical Components. Amplifiers. Mixers. Attenuators. Power Detectors. Synthesizers. Splitters. Couplers. Filters. Switches. Multipliers. Types of Filters. Edges are smoother than illustrated. SHOT II Balloon Payload Presentation. June 29, . 2012. Andrew Dianetti, Alex Wende, . Bryant Carlson, Joe Flannery. 1. Mission Overview. Test spectrometer data compression algorithm. Transmit compressed data to ground. transfer. . reactions. ?. Marlène . Assié. IPN Orsay, assie@ipno.in2p3.fr. 29/04/2019. ASSIE Marlène – IoP Recoil spectrometer - Liverpool 29th april 2019. 1. ©CEA/. P.Stroppa. INCIDENT BEAM.