PMMA (polymethyl methacrylate) doped with a scintillating fluor 2 ft x 2 ft x ½ inch Read out by 10 stage EMI 9256 photomultiplier tube The Chicago Air.

Slides:



Advertisements
Similar presentations
Zoll Monitor Upload Required for all ALS calls where an EKG/12 lead are performed.
Advertisements

Importing from a HydraFLASH Project file (.prj)
Measuring Cosmic Ray Flux with a trigger and CAMAC readout - Page 1 Connect the Fluke 415 HV supply output to the input of the voltage distribution box.
COSMIC RAY MUON DETECTION USING SCINTILLATION COUNTER AND WAVELENGTH SHIFTING FIBERS ARUNODAYA BHATTACHARYA VSRP-2009,TIFR,MUMBAI 6/7/09.
MS-Word XP Lesson 3. Undo 1.Click on edit menu 2.Click on undo … menu item 3.Also you can use undo button in standard tool bar 4.Shortcut Ctrl+Z Redo.
Cosmic Rays Basic particle discovery. Cosmic Rays at Earth – Primaries (protons, nuclei) – Secondaries (pions) – Decay products (muons, photons, electrons)
WATERLOO HIGH SCHOOL. COSMIC RAY OBSERVATORY PROJECT  Goal of the statewide project  Install cosmic ray detectors at high schools around the state of.
Cosmic e-Lab Collaboration Bob Peterson Fermi National Accelerator Lab.
By Jeff Headlee Bancroft-Rosalie Who Was Involved? Haverah Park was operated by the Physics Department of the University of Leeds Goal Record extensive.
1st of year Checkout 1.Powering up detector(s) 1 st in the DARK Ramping up voltages slowly in 50 v steps 2. Look for signals 3. Check rates 4. Light leak.
A Statewide Outreach and Education Experiment in Nebraska The Cosmic Ray Observatory Project Dan Claes University of Nebraska APS-DPF JPS2006 Monday,
Aspen High School, Aspen, CO Basalt High School, Basalt, CO Roaring Fork Valley High School, Carbondale, CO Lake County High School, Leadville, CO The.
1. Connect the detector signal cable with a 50 ohm “T” into Ch 1 adapter50 ohm “T” 2. Turn the oscilloscope on by depressing the power button. 3. The display.
Experimental Procedures Arrival at Desktop BASE Check that computer and DAQcard are still running. Sign in and start logbook entry (date and time). Note.
Search Catalog Online Ordering EN.04.1 You may control this presentation by clicking the right mouse button at any time. When you have finished viewing,
CPSC 203 Introduction to Computers T43, T46 & T68 TA: Jie (Jeff) Gao.
Jimmy McCarthy International Cosmic Ray Day 26 th September 2012 Detecting Cosmic Rays.
Cosmic Ray Muon Detection Department of Physics and Space Sciences Florida Institute of Technology Georgia Karagiorgi Julie Slanker Advisor: Dr. M. Hohlmann.
CPSC 203 Introduction to Computers Tutorial 03 & 29 Jie (Jeff) Gao September 15 & 16.
A crude (lower limit) estimation of resolution and event rate Development and Construction of an Extensive Air Shower Array in HOU Antonis Leisos, Hellenic.
Cosmic Ray Observatory Project Fr Michael LieblAGU Conference Mount Michael Benedictine High SchoolDecember 6, 2005 Elkhorn Ne
Graphical Analysis Tutorial Version GA 3.2. Entering Data Enter your independent (x) data and dependent (y) data into the columns shown By double-clicking.
Scratch Internet- Open Chrome hit “Create” 1.
RADAR Detection of Extensive Air Showers Nils Scharf III. Physikalisches Institut A Bad Honnef Nils Scharf III. Physikalisches Institut A Bad.
Vladimir Frolov for Torino group. Experimental activities: The system for testing the MRPC in the Torino INFN laboratory has been fully mounted and checked;
CROP 2005 Summer Workshop July 18-22, 2005 Equipment check in is in Ferguson 114.
Mv 0 mv f  (mv) =  recoil momentum of target ( )  mv 0 mv f large impact parameter b and/or large projectile speed v 0 v f  v o For small scattering.
QuarkNet Muon Data Analysis with Shower Array Studies J.L. FISCHER, A. CITATI, M. HOHLMANN Physics and Space Sciences Department, Florida Institute of.
New Mexico Computer Science For All Interface Output in NetLogo (Part 1) Maureen Psaila-Dombrowski.
High School Cosmic Ray Projects and Training Basalt High School Math and Science Club October 14, 2004.
Energy Distribution of Cosmic Ray Muons Paul Hinrichs With David Lee Advised by Phil Dudero.
Nebraska’s Statewide Outreach and Education Experiment The Cosmic Ray Observatory Project Dan Claes University of Nebraska-Lincoln Washington Area Large.
Detection of cosmic rays in the SKALTA experiment Marek Bombara (P. J. Šafárik University Košice), Kysak, August 2011.
James Westover Dan Linford.  Background  Production and Lifetime  The Apparatus  Discussion of our procedure and results  Questions.
Nebraska’s Statewide Outreach and Education Experiment The Cosmic Ray Observatory Project Dan Claes University of Nebraska-Lincoln Thursday, December 11,
Experiment Design SCIPP Teacher Workshop Mary Jo Nordyke August 2010.
TECHNICAL TRAINING SMART COMMANDER System Requirements CPU : 800MHz and aboveCPU : 800MHz and above Memory : 256MB RAM or HigherMemory : 256MB.
Creating and Saving College Essays and Documents Presented by Minnesota College Success Corps Anoka Ramsey Community College.
Programmable logic device Time-to-digital converters 5 Volt DC power To PC serial port Four analog PMT inputs Discriminator threshold adjust GPS input.
The Cosmic Ray Observatory Project (CROP) Gregory R. Snow University of Nebraska / USA CRSP Meeting NIKHEF, Amsterdam March 7, 2005 Overview Staff and.
Brian Lowery July 11,  Primary  From space ▪ Lower energy cosmic rays come from sun ▪ Higher energy cosmic rays come from other places in the.
IEAP CTU Project CZELTA Karel Smolek IEAP CTU
Time over Threshold electronics for an underwater neutrino telescope G. Bourlis, A.G.Tsirigotis, S.E.Tzamarias Physics Laboratory, School of Science and.
QuarkNet and Cosmic Ray Muon Flux Experiments Florida Academy of Sciences Spring Conference 2009 Alfred Menendez and Michael Abercrombie with Dr. Marcus.
The Cosmic Ray Observatory Project in Nebraska Conference on Teacher Research Experiences University of Rhode Island April 2005 An education and.
Calibration instructions for Quarknet Cosmic-Ray Detector How to Plateau the Counters A friendly guide for students and teachers Edited by Jeremy Paschke,
AMIGA – A direct measurement of muons in Pierre Auger Observatory
Wikispaces Timer Begin!. Station # 1 Click the Discussion Tab to record different thoughts the group has to the question. The recorder will type as many.
Cut and Paste PowerPoint Timers
Horizon Icemaker for Vision Satellite-fill Installation Installation Best Practices To navigate through the presentation, press the → and ← keys on your.
Accidental Coincidences Learning Objectives Understand the difference between real and accidental coincidences in an experiment using  2 scintillators.
When iPhone users to want to sync songs or pictures to their device, they can take advantage of iTunes and sync the whole playlist or folder to their.
Using sensors with Flowol 2. There are 2 ways that you can use sensors with Flowol 2 software. 1.You can use SIMULATION mode – when you use a MIMIC 2.You.
Cut and Paste PowerPoint Timers
Calibration Instructions for Quarknet Cosmic Ray Detector
University of Nebraska
Using the Lego Mindstorms Edu NXT Software
Jeopardy Q $100 Q $100 Q $100 Q $100 Q $100 Q $200 Q $200 Q $200
QuarkNet and Cosmic Ray Muon Flux Experiments
Dan Claes Susan Pfiffner Brian Jones
Display Trouble Shooting
Holdings Management Adding, Editing, and Assigning Notes
WEATHER STATION MODEL Wind Speed Cloud Cover Temperature Wind
On your bingo cards, write your responses to:
Setting Up Classes and Groups in EbD-BUZZ A Tutorial for EbD Teachers
DING CONGJIN LU GUICHI MARSEILLE
Green Screen Moviemaking
Lab 1 – Understanding Graphs of Motion
The Cosmic Ray Observatory Project (CROP) in Nebraska
Courses Tab Press the Courses tab
Presentation transcript:

PMMA (polymethyl methacrylate) doped with a scintillating fluor 2 ft x 2 ft x ½ inch Read out by 10 stage EMI 9256 photomultiplier tube The Chicago Air Shower Array recycling retired detectors from the Chicago Air Shower Array located in the Utah Desert: 1089 stations, 15m spacing covering 0.23 square km

Barometric Pressure (mmHg) Fold Coincidences / 2 hours Statistical error bars shown 1.3% decrease per mmHg Marian High School’s Measurement of Cosmic Ray Rate vs. Barometric Pressure

Mount Michael Benedictine High School “The Science Teacher”, November 2001

Cosmic Ray Observatory Project Collecting Data with CROP DAQ Card Interface Doing an Efficiency Scan 1.Disconnect the 4 signal cables from the DAQ card. These are the cables that connect to your 4 detectors. 2.Open the CROP_DAQ LabVIEW Program. 3. Click on the "Efficiency" tab make sure the Efficiency Scan button is ON(lit up). 4. Click on the "Threshold Scan" tab make sure the Threshold Scan button is OFF. 5. Click on the "Data Collection Settings" tab and set the timer ON (green button lit up). 6. Click on the "Data Acquisition" tab and to begin run click on (upper left corner under the Edit menu). Online help and tutorials available.

On-Line Oscilloscope Cheat Sheets