PPT-JUNO central detector and

Author : pamella-moone | Published Date : 2017-05-10

its calibration strategy Mengjiao Xiao University of Maryland College Park On behalf of the JUNO collaboration 20161103 NNN16 November 35 2016 IHEP Beijing China

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JUNO central detector and: Transcript


its calibration strategy Mengjiao Xiao University of Maryland College Park On behalf of the JUNO collaboration 20161103 NNN16 November 35 2016 IHEP Beijing China Outline Introduction to JUNO experiment. The LEGe detector is fabricated with a thin front and side contact The rear contact is of less than full area which gives a lower detector capacitance compared to a planar device of similar size Since preampli64257er noise increases with detector ca 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. Queen of the Gods and Goddess of Marriage . . Juno enjoys wearing a diadem. . Facts . Lives on Mt. Olympus . . After Juno’s mother gave birth to her. She was then swallowed by . Saturn . .. . Shun Zhou. IHEP, CAS, Beijing. on . behalf of the JUNO Collaboration. The 8. th. Workshop of France-China Particle Physics Laboratory. USTC, Hefei, April 8 - 10, 2015. T. he JUNO Experiment. 20 . kton. Contributor. :. . Yuanqing. Wang. , . Zongyi. Wang. Speaker. : . Z. ongyi. Wang. Department of civil engineering, Tsinghua University . 2015-06-05. 1. Outline. Introduction of the whole structure . Brennan Thomason. Tamara Reed. Edmond Wilson. Project Goal. Design a detector for a high resolution spectrograph that provides electromagnetic radiation intensity data as a function of wavelength in the range of 400 nm to 1000 nm.. Configuration. Juno Spacecraft. en route to. Jupiter. (Arrives July 4. th. 2016). . National Aeronautics and. Space Administration. Goddard Space Flight Center. Jet Propulsion Laboratory. PI: Scott Bolton SWRI . Further developments of detectors with resistive electrodes:. R. Oliveira. 1. , V. Peskov. 1,2. , F. Pietropaolo. 3. , P. Picchi. 4. 1. CERN, Geneva, Switzerland. 2. NAM, Mexico. 3. INFN Padova, Ialy. side. Wago. 2002-1201 . Wago. 2002-3203 . Door open. 800x600x200 mm. 0.93x60 cm. 10 cm. 4.9 cm. 4.9 cm. GSM cable. Gas pipes. ~25cm. ~25cm. NSYS3D8620. Inputs. Outputs. 600. 8. 00. 200. 60cm. 90 ˚ turn. In addition to Smirnov, . Petcov. , . Razzaque. , Mena, . Palomarez-Ruis. APC: . Semikov. , Allard, . Parizot. Brazil (phenomenologist). UNICAMP: Orlando . L. G. . Peres, Pedro . C. de . Holanda. , Marcelo . to the JUNO Simulation (1). JUNO uses . SNiPER. as underlying framework. . D. etector simulation framework and digitization simulation are implemented.. Detector Simulation Framework. Integrate Geant4 and . Multi-Wavelength “Eyes. ”. Glenn Orton. Background:. . Observations of Jupiter from various instruments on board the Juno spacecraft reveal a 3-Dimensional view of the planet.. Data & Results:. Do you need an Amazon Echo or similar Master device to use Juno AI fixturesThe Juno AI voice-controlled speaker light with Alexa built in can act as your Master device in an installation with other Al

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