PPT-EEE-Nanuk A modular cosmic ray scintillator detector

from a module 15x15 already available 15x15 cm scintillator read out pair of SiPM Advansid directly coupled to the scintillator without fiber Scientific purposes longterm measurements of. 6405 provides different installation options on adjustable feet or ss castors when in 465636 The extensive range of models allows you to best utilise space by either placing units in a single line or back to back can also be combined with Domina 9 Pierre Auger Observatory. Lawrence Wiencke. Colorado School of Mines. IS@AO, Apr. 18 2011, Cambridge. 1. 2. Wiencke. Logarithmic Scale. Linear Scale. Linsleys. x10. 5. Linsleys. TA. The Pierre Auger Observatory. 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. of Plastic Scintillator. Oct. 2, 2009. IP-BSM Group. 1. Schematic . Drawing . of. new Gamma Detector. 2. sandwich type calorimeter. SUS and plastic scintillation plate. wavelength-shifting fiber (WLSF) for light transmission. at. . Hartnell. . College. : A Case Study in Successful Undergraduate Research at a Two-Year College. Leo . Osornio. Hartnell. College. Presented at the 2012 AAPT Summer Meeting, Philadelphia. July 30, 2012. Ohio University (Athens, OH, USA). Uniplast Ltd Co. (Vladimir, . Russia. ). PHENIX Calorimetery Workshop. 12/14/2010 BNL. Main Idea. We have done some preliminary calculations/considerations for the basic parameters of a few more “conventional” options: . 37. K. . Erin France. Motivation. To test the Standard Model via the correlation parameters. Measure the beta asymmetry, and compare it to the Standard Model . prediction. Beta asymmetry: the magnitude of the tendency for a beta to be emitted (anti)parallel to the nuclear spin. QuarkNet. Student Investigations. DAQ Detector e-Lab. Mark Adams. Fermilab. DAQ Detector e-Lab. Global Cosmic Ray Effort. Outline. QuarkNet. 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. contribution”. U.Kose, M. Nessi, P. Sala. ICARUS . CRT Technical . Workshop, 21 September 2016. 1. detailed note : https://edms.cern.ch/document/1689906. 2. Cosmic Ray Tagger options studied in FLUKA simulations:. Varchaswi K S Kashyap*. On behalf of NISER group. Facilities at NISER. Gas mixing system:. 5 channel gas mixing system (Freon, . iso. -butane, SF. 6. , . Ar. and CO. 2. ). Supply gas to 8 detectors simultaneously with a maximum flow rate of 50 . Glenn . Sembroski. QuarkNet. Summer Workshop. July 24,2012. The Big Question. Which has become the Big Mystery. Where do Cosmic Rays come from?. A multi-part question. i.e. Lots of small mysteries. Different answers for different energy regimes. J. Huston. Michigan State University. Reminder. The MBTS counters were somewhat of an afterthought, with thinking/plans not started until ~2004. The idea was that it was very useful/critical to have a trigger signal for the early running of ATLAS, such that we would know which crossings had interactions (at very low luminosity). Liceo scientifico statale Giuseppe . Peano. Monterotondo(. Rm. ) . Italy. Professor . A.Tiscioni. , . C.Giammarini. , . M.F. . . Erardi. . LSS. . G.Peano. Erice 29-31 . may. 2017.