Cosmic Ray e-Lab Bob Peterson Fermi National Accelerator Lab.

Slides:

Advertisements

Similar presentations

The QuarkNet Collaboration: How Doing Science is Changing Science Education.

Advertisements

1. Cable connection - Adjust Gain to make Mn K signal (5.895 keV) around 2 V on oscilloscope. (Full range : 10 V)

QUARKNET 2011 SESSION 1 1. Abstract Week One Hardware Performance Plateauing Flux Shower Lifetime Purpose, Research Question, Hypothesis Experimental.

Al / a la / del / de la / en el / en la ALTA-VISTA, A school of SPANISH Language 2006.

27/02/2002M.D.P. - ATLAS Muon Week1 First results of Atlas RPC cosmic rays test Massimo Della Pietra Atlas RPC Group Napoli ( M. Alviggi, V. Canale, M.

T. Jordan, Advisory Board Meeting - November 2002 Advisory Board Meeting T. Jordan, Advisory Board Meeting - November 2002 Data Projects Thomas Jordan.

COSMIC RAY MUON DETECTION USING SCINTILLATION COUNTER AND WAVELENGTH SHIFTING FIBERS ARUNODAYA BHATTACHARYA VSRP-2009,TIFR,MUMBAI 6/7/09.

Introduction This project used cosmic rays to test a prototype Minimum Bias Trigger Scintillator (MBTS) that will be used in the ATLAS experiment at CERN.

Cosmic Ray e-Lab Overview. Teaching and Learning with the Cosmic Ray e-Lab

Quark Net 2010 Wayne State University Physics Department.

Welcome to Quark Net 2011 Wayne State University Physics Department.

Cosmic Rays Basic particle discovery. Cosmic Rays at Earth – Primaries (protons, nuclei) – Secondaries (pions) – Decay products (muons, photons, electrons)

Cosmic Ray e-Lab Bob Peterson Fermi National Accelerator Lab.

Cosmic e-Lab Collaboration Bob Peterson Fermi National Accelerator Lab.

CRAnE: A JAS-based Data Acquisition System for Cosmic Rays Jennifer Docktor & Manuel Reyes Mentors Tom Glanzman & Willy Langeveld August 13, 2003 Department.

Muon Lifetime Eric Chu & Joseph St. Marie. Goals of our Experience Gain an understanding of electronics Design and run a working muon experiment Analyze.

Cosmic Rays Ty Fredriks SCIPP QuarkNet Summer Institute.

Atlas SemiConductor Tracker Andrée Robichaud-Véronneau.

Quarknet Seminar Alisa Bredensteiner Endeavour Institute Santa Cruz Institute of Particle Physics Quarknet August 2010.

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.

P. Karchin – PMTs for Scintillator Based Muon Systempage 11/7/2004 January 7, 2004 American Linear Collider Physics Group 2004 Workshop Stanford Linear.

Cosmic Ray Detection Experimental Report Alisa Bredensteiner Endeavour Institute Santa Cruz Institute of Particle Physics Quarknet August 2010.

QuarkNet 2011 Mohamed Ali-Hussein Ayasha Jabber. Cosmic Rays Discovered by Victor Hess in 1912 High energy particles (atoms, protons, electrons) traveling.

Time over Threshold Electronics for Neutrino Telescopy George Bourlis + multiplicity.

Cosmic Ray Muon Detection Department of Physics and Space Sciences Florida Institute of Technology Georgia Karagiorgi Julie Slanker Advisor: Dr. M. Hohlmann.

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 e-Lab Collaboration Bob Peterson Fermi National Accelerator Lab.

M. Bardeen, BCNET Conference, April 2004 The QuarkNet/Grid Project Developing Our “e-Lab” for High School Students & Their Teachers Marge Bardeen, Fermilab.

Vanderbilt University July 26, 2010 Introduction to QuarkNet for the Vanderbilt University Center Ken Cecire University of Notre Dame

Cosmic Ray e-Lab Bob Peterson Fermi National Accelerator Lab.

Kris Whelan-AGU 2005 Teaching and Learning with Cosmic Rays and the QuarkNet/Cosmic Ray Data Portal quarknet.fnal.gov/e-labs/ Kris Whelan Lawrence Berkeley.

Teaching and Learning with Open Science Grid quarknet.fnal.gov/e-labs/

EUs: Data are collected using careful measurement and/or observation. Data are organized into charts, tables, and/or plots for data analysis; so doing.

M. Bardeen & K. Cecire, Dresden, November 2011 Helping Develop America’s Technological WorkforceTechnological Workforce The QuarkNet Collaboration.

QuarkNet Muon Data Analysis with Shower Array Studies J.L. FISCHER, A. CITATI, M. HOHLMANN Physics and Space Sciences Department, Florida Institute of.

The Thinking Behind an e-Lab A Marriage Between High School Physics & Grid Computing M. Bardeen, EPPOG, April 2010 Marge Bardeen Fermilab.

Cosmic Ray e-Lab Bob Peterson Fermi National Accelerator Lab.

Energy Distribution of Cosmic Ray Muons Paul Hinrichs With David Lee Advised by Phil Dudero.

US CMS Education and Outreach Dan Karmgard University of Notre Dame.

Helping Develop America’s Technological Workforce K. Whelan Oregon QuarkNet Meeting, June 2012 QuarkNet 101 Kris Whelan University of Washington.

Dr. Sascha Schmeling CERN/EP HST Programme 2001

Experiment Design SCIPP Teacher Workshop Mary Jo Nordyke August 2010.

Teaching and Learning with the Cosmic Ray e-Lab

Use of Cosmic Ray eLab to Teach the Research Process Deborah Roudebush Oakton High School 2900 Sutton Road Vienna, VA AAPT 2009 Winter Meeting February.

Teaching & Learning with Particle Physics “Stuff” Marge Bardeen Fermilab Bardeen, AAPT, Chicago, 2/2009.

Gap Production for Upscope of the Endcap RPCs Sung Keun Park Korea Detector Laboratory Korea University February 5, 2010 Workshop on the Forward CMS RPC.

CERN and Physics Education Mayaguez, PR March 11, 2006 In 2007, the Large Hadron Collider (LHC) at CERN will begin to generate opposing 7 TeV proton beams.

Status Report for KEK-PS E391a KEK IPNS G.Y.Lim 14 April 2003.

Time over Threshold Electronics for Neutrino Telescopes

Programmable logic device Time-to-digital converters 5 Volt DC power To PC serial port Four analog PMT inputs Discriminator threshold adjust GPS input.

Update on the Triple GEM Detectors for Muon Tomography K. Gnanvo, M. Hohlmann, L. Grasso, A. Quintero Florida Institute of Technology, Melbourne, FL.

PMT Readout and Floor Triggering Charge estimation using the times over the thresholds Event Building and Triggering + multiplicity George Bourlis.

Info and Interesting Items Ken Cecire. Over 500 U.S. high school teachers Over 50 physicist mentors 4 staff National program International reach QuarkNet.

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.

Pr ducts panel. COSMIX, a portable cosmic ray detector  Designed and built by the Bordeaux-Gradignan IN2P3 lab (CENBG)  2 scintillator bars reused from.

K. Whelan, Summer 2010 The QuarkNet Collaboration.

Calibration instructions for Quarknet Cosmic-Ray Detector How to Plateau the Counters A friendly guide for students and teachers Edited by Jeremy Paschke,

UC QuarkNet Workshop Mike Sokoloff Brian Meadows Jeff Rodriguez.

Quick guide to ASIMON configuration For version 3.0 or greater SAFETY AT WORK Date: 3/18/2009.

Measurement of the Charge Ratio of Cosmic Muons using CMS Data M. Aldaya, P. García-Abia (CIEMAT-Madrid) On behalf of the CMS Collaboration Sector 10 Sector.

Rutherford Appleton Laboratory September 1999Fifth Workshop on Electronics for LHC Presented by S. Quinton.

Cosmic Ray e-Lab Bob Peterson Fermi National Accelerator Lab.

The data-logger for computers and CASIO Graphical calculators

Calibration Instructions for Quarknet Cosmic Ray Detector

QuarkNet Beyond the First Year

Quarknet Vanderbilt University July 2016

QuarkNet and Cosmic Ray Muon Flux Experiments

NI Data Acquisition (DAQ) Wiring and Connections

Presentation transcript:

Cosmic Ray e-Lab Bob Peterson Fermi National Accelerator Lab

Teaching and Learning with Cosmic Rays Workshop Objectives: Assemble CRMD: plateau, geometry, data-take. Design e-Lab investigation: data, tools, plots. Begin poster, present results. Discuss implementation strategy.

Teaching and Learning with Cosmic Rays Por el gran parte del taller, estamos alumnos. Podemos tener la experiencia del “CR e-Lab” con la vista de un alumno Aprender bazado en investigacion

Teaching and Learning with Cosmic Rays Active QuarkNet Centers

Teaching and Learning with Cosmic Rays QuarkNet hace collaboraciones: Profesores  Alumnos Profesores  Fisicos (Mentores) Colegios con detectores  Colegios sin detectores Y redes mundiales: Alumnos  Alumnos Profesores  Profesores …y mas

Teaching and Learning with Cosmic Rays CRMD Expectation:  Not “plug & play”  Assembling and thinking required Detectores en el LHC estan grandes y complicados, pero el CR detector usa tecnicas basicas ATLAS CMS QuarkNet Note: Images are not to scale

Teaching and Learning with Cosmic Rays Typical QuarkNet Detector Setup 1. Counters-scintillators, photomultiplier tubes (two shown) 2. QuarkNet DAQ board 3. 5 VDC adapter 4. GPS receiver 5. GPS extension cable 6. Computer (PC preferred) 7. USB adapter or cable 8. Lemo or BNC signal cables 9. Daisy-chained power cables The QuarkNet Cosmic Ray Muon Detector (CRMD) 6

Teachers & students: –Assemble. –Calibrate. –Set-up and run. Teaching and Learning with Cosmic Rays

Teaching and Learning with Cosmic Rays

02F17C70 AE 3E BAB A F0A B BD A F0B A 1814BD A F0C BD A B23 A E 3A 2203DEA A Raw Data Teaching and Learning with the Cosmic Ray e-Lab

There has to be an easier way...  Cosmic Ray e-Lab Lower the threshold to analyzing real data. Teaching and Learning with the Cosmic Ray e-Lab

Teaching and Learning with the Cosmic Ray e-Lab

Teaching and Learning with the Cosmic Ray e-Lab Go to: REGISTRATION 1st: Change password.  Update your previously created groups. !! min 6 characters : max 10 characters !! !! alpha/numeric !! !! no spaces !! 2nd: Create student group.  Register student research groups. Select “pencil”: yes pre/post test 3rd: Add DAQ #.  Update detector IDs for your group.