PPT-Detector Status

J Brunner 12092014 Highlights Line 3 Optical Margins Line 5 UPS Situation Data Taking Status Planned Operations Line 3 250614 Several short power cuts at IMP Power cut of the Detector . Matthew Mendonca. Woodside High . School. Mentor. : Dr. . Doug Higinbotham and Lawrence . Selvy. Abstract. The particles that make up the nucleus of an atom are so infinitesimally small that it takes a detector of large magnitude in order to predict where protons and neutrons are located. This certain device requires the construction and utilization of one-meter-long rectangular plastic bars called scintillators. Attached to the left and right ends of each bar are Photomultiplier Tubes (PMTs) and bases with outlets for high voltage and signal wires. In experiments, there is a thick wall of lead positioned in front of the detector which excludes nearly all charged particles and permits primarily neutrons to enter and react with the nuclei inside the bars. When charged particles do pass through the scintillators, photons are released and bounce around until they reach a light guide and are collected by the PMTs. Within these there is liberation of electrons which in turn provide an analog signal to the electronics. A data acquisition system (DAQ) comprised of ADCs (Analog-to-Digital Converters) and TDCs (Time-to-Digital Converters) then store the data into files for later replay and analysis. By doing so, we can better measure the type of particle detected, it’s trajectory, and the amount of energy that it deposits. To ensure that these complex apparatuses are working at an acceptable level, scientists manipulate the constant flux (100 particles/m. B.Satyanarayana, Tata Institute of Fundamental Research, Mumbai. Lecture – I. Saturday, July 2, 2011. B.Satyanarayana, TIFR, Mumbai Resistive Plate Chambers & INO’s ICAL detector SERCEHEP11, VECC, Kolkata. Choice of assembly procedure. Screwing versus . glueing. Pro’s and con’s . MMM Würzburg, 30/01/2014. P. Ponsot/J. Wotschack. 1. Glueing. or screwing ?. The purpose of this presentation is to introduce the discussion on the first choice that we have to make in order to arrive at an agreed assembly procedure. Lab Methods Day. June 25, 2013. Taylor . Myers. 2. Carbon Monoxide Concentration. % of CO, by volume, in the air. Digital readout. Analog output 0/2/4 to 20 mA. Carbon Dioxide Concentration. % of . CO2, . 2012/3/2. Y.Sugimoto. Background. Request for more space from DESY team. Several installation works in parallel. Depends on total allowed construction perio. d . Design of common cryogenic system. ILD, . Week 3. Very few detectors will count every interaction. Each detector will have its own counting efficiency. Eff. =CPM/DPM. Can use efficiency and count rate to determine amount of material present. Philip Anderson. National Sales Manager. System Sensor Canada. A hospital is like a city. Living areas. Machinery, high technology. Food prep/service. Retail, public spaces. Open spaces, parking. Wide range of application challenges. Brian . Kross. – mechanical design and construction / gas systems. Seungjoon. Lee – advanced image recon algorithms / mechanical / detectors. John . McKisson. – software / data acquisition / electronics. Mark Stewart. Materials Characterisation. Workshop on low gain fast silicon detectors for EM and synchrotron applications Nov 25th. Welcome to the National Physical Laboratory. Workshop on low gain fast silicon detectors for EM and synchrotron applications. MicroTCA. platform with embedded sub-ns WR synchronization. G. .. Kasprowicz (WUT). 2. Outline. NICA . collider. & . Cosmic Ray Detector – Goals. SIPM AFE. SIPM readout chain based on Open Source HW. FCC week Washington. 23. -27 March . 2015. W. . Riegler. D. . Denisov. , H. . ten. Kate, L. . Lienssen. , F. . Lanni. , M. . Abbrescia. , R. Richter, Y. . Onel. , W. Smith, S. . C. hekanov. Exploration + Higgs as a tool for . results during isotopic analysis Traditionally it was recodetector with a full width half-maximum FWHMHowever in many cases when using large detectors or when using a short amplifier time constant thi Innovative silicon sensors for future trackers. N. . Cartiglia. M. . Mandurrino. INFN - Italy. Part II: Principles of operation of RSD. Single point precision and charge sharing. Signal formation. Charge sharing: RSD master formula. IceCube. Justin Vandenbroucke, June 9, 2021. IceCube. Bootcamp, WIPAC, UW–Madison. Outline. Neutrino interactions and cross sections. Muon lifetime. Charged particles losing energy in matter. Ionization.