A.D.O.M Airborne.Detector.of.Muons Tye Barba Anna Chang Natalina DeFusco David Hood.

Slides:



Advertisements
Similar presentations
THE QUICK HISTORY OF COSMIC RAY MAN THE BIRTH OF AN EXTRAORDINARY PARTICLE… Wilson suspected the cause of the residue conductivity of the atmosphere might.
Advertisements

BASE Project DePauw University Ruizhe Ma, Mark Tolley, Professor Brooks.
Printed by Evaluating the Effects of Differing Elevations on the Cosmic Ray Detector Chris Allen, Jeff Allen, Drew Kemp-Baird, Nick.
Shantanu Menon Thomas Irons Michael Jacoutot. Cosmic Rays  High energy particles (mainly protons) from outer space.  Have up to 10 million times more.
Measurement of lifetime for muons captured inside nuclei Advisors: Tsung-Lung Li Wen-Chen Chang Student: Shiuan-Hal Shiu 2007/06/27.
Oxygen Levels and Temperature Alex, Brandon, Carly, and Danielle ABCD’s.
A Muon Veto for the Ultra-Cold Neutron Asymmetry Experiment Vince Bagnulo LANL Symposium 2006 Outline ● UCNA Experiment ● Muon background ● Proposed Veto.
A Strange Phenomenon There is a type of unstable particles called Muon. They are produced in the upper atmosphere 14 km above Earth’s surface and travel.
A Muon Veto for the Ultra Cold Neutron Asymmetry Experiment Vince Bagnulo with Dr. Jeff Martin Electrons Ultra Cold Neutrons Cosmic Ray Muons Protons Pions.
Cosmic Ray Lifetime Study A measurement of Special Relativity Richard Lasky – Summer 2010.
Conducted by: Adrian Lorenzana David Harris Muon Speed/Lifetime Study.
Cosmic rays in a thermos flask 1.European Physics Education Conference Bad Honnef Thomas Trefzger Universität Mainz.
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.
Muon Decay Experiment John Klumpp And Ainsley Niemkiewicz.
Presented by Steve Kliewer Muon Lifetime Experiment: A Model.
Detecting Cosmic Rays An inexpensive portable detector By: Danny Franke Quarknet 2004.
Victor Hess Before making balloon ascents himself, he determined the height at which ground radiation would stop producing ionization (about 500 meters)
SCIPP Summer Outreach Project July Cosmic Ray Detectors Cosmic Ray Detectors Detector Testing Detector Testing Muon Lifetime Experiment Muon Lifetime.
Using muon physics to teach relativity, radiation, and instrumentation Daniel W. Koon 1 and Jeremy Ouellette Department of Physics St. Lawrence University.
Cosmic Ray Workshop May 15, May 15, 2010 Rutgers Cosmic Ray Workshop.
Cosmic Ray Detection Experimental Report Alisa Bredensteiner Endeavour Institute Santa Cruz Institute of Particle Physics Quarknet August 2010.
Forward Detectors and Measurement of Proton-Antiproton Collision Rates by Zachary Einzig, Mentor Michele Gallinaro INTRODUCTION THE DETECTORS EXPERIMENTAL.
Abstract We constructed and tested seven scintillation counters using photomultiplier tubes, in order to create a fast electronic coincidence “trigger”
QuarkNet 2011 Mohamed Ali-Hussein Ayasha Jabber. Cosmic Rays Discovered by Victor Hess in 1912 High energy particles (atoms, protons, electrons) traveling.
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.
SOLAR POWER SATELLITE ANNAMACHARYA INSTITUTE OF TECHNOLOGY AND SCIENCES DEPATMENT OF ELECTRICAL AND ELECTRONICS ENGINEERING PRESENTED BY: P.AMARNATHS.ABEED.
Cosmic v12/1/09Cosmic Pre-PDR 1 Cosmic Ray Experiment Team Cosmic Jace Boudreaux Allen Bordelon.
S. W. A. T. amLeesamLees illTucayillTucay bigailSternsbigailSterns ylerVenessylerVeness.
Dominik Wermus (Virginia Military Institute, Lexington, VA 24450), Doug Higinbotham (Thomas Jefferson National Accelerator Facility, Newport News, VA,
QuarkNet Muon Data Analysis with Shower Array Studies J.L. FISCHER, A. CITATI, M. HOHLMANN Physics and Space Sciences Department, Florida Institute of.
Scintillators, DAQ boards, and PMTs Getting Familiarized With the Equipment By Melissa Sussmann and Alex Bonnifield.
A Cherenkov Radiation Detector for the Auger Project Katarzyna Oldak Research Adviser: Corbin Covault Department of Physics The purpose of this project.
Energy Distribution of Cosmic Ray Muons Paul Hinrichs With David Lee Advised by Phil Dudero.
Cosmic Rays The discovery of cosmic rays Discoveries made with cosmic rays Cosmic rays in modern physics education Let’s count cosmic rays around us.
Development and Testing of a Portable Gamma Ray Scintillator The Physics and Background of Gamma Ray Scintillator: This Gamma Ray Scintillator uses a Cesium.
Balloon Fest Team Ballair Andrew, John, Valerie, Bailey, Kindsay.
Keep the standard candle of electron observations burning Provide an intercalibration with PAMELA and AMS Search for the origin of the turn up in the low.
James Westover Dan Linford.  Background  Production and Lifetime  The Apparatus  Discussion of our procedure and results  Questions.
Monte Carlo simulations of a first prototype micropattern gas detector system used for muon tomography J. B. Locke, K. Gnanvo, M. Hohlmann Department of.
Project Inferred By: Kenneth Pay Michael Chun Nancy Nguyen Peter Ho.
Experiment Design SCIPP Teacher Workshop Mary Jo Nordyke August 2010.
By GR² Team from LSU LaACES. Science Background Cosmic rays are high energy particles constantly hitting the Earth’s atmosphere Cosmic rays are high energy.
Brian Lowery July 11,  Primary  From space ▪ Lower energy cosmic rays come from sun ▪ Higher energy cosmic rays come from other places in the.
MUONS!. What are we going to talk about? How muons are created Detecting methods Muon half life and decay rate Muon decay data Problems with the data.
O Level Physics Chapter :24: Radiation and Half Life Prepared By: Shakil Raiman.
Cosmic Ray Workshop May 15, Cosmic Ray Detector Kit.
Status of the ETL 9125FLB Photomultiplier Tubes Steve Bache UNC-Wilmington.
QuarkNet and Cosmic Ray Muon Flux Experiments Florida Academy of Sciences Spring Conference 2009 Alfred Menendez and Michael Abercrombie with Dr. Marcus.
LA ACES Neutron Detector (NeD)
9th April 2009based on a presentation prepared by D. Schinzel 1 COSMIC RAY DETECTOR.
Construction of the Balloon Project SCIPP Interns.
Balloon Detector SCIPP. Purpose To make a project that can be replicated by high school groups To gather data on Muon count rates at different altitudes.
Specs, Data, and Web By Ben Jolitz. Specs Professional projects use specifications  Ensures quality  Ensures product does what it should.  Example:
Scintillation Counter
Introduction Cosmic rays, originating from distant solar flares and supernova, bombard our planet constantly and collide with atomic nuclei at an altitude.
Geiger counter NTHU General Physics Laboratory
DETECTION OF NUCLEAR RADIATION
Cosmic Ray Detector at Work 3 Guys and a Cosmic Ray Detector Derek, Kurt, Doug and Teachers: Josh, Grace.
Alysha Dan Melissa Kyle Mr. Walter.  Subatomic particles from outer space, the exact location is still unknown.  These particles interact with our atmosphere.
By Rebecca Denison, Joe Ditmar, Oxana Kachtanova, Caitlin Kearns, and Sam Tencer With the greatly appreciated assistance of Maureen Michael and Stephanie.
A strong enough magnetic field will cause less cosmic radiation to reach a cosmic ray detector than a physical shield of lead.
The Effect of Artificial Lighting on a Cosmic Ray Detector
QuarkNet and Cosmic Ray Muon Flux Experiments
The Life and Times of Cosmic-ray Muons
Cosmic Ray Showers Cosmic ray activity Figure 3:
EagleSat 2: Design Development Lauren Barthenheier Dr
Pittsford Mendon High School, Physics Regents Honors period 1
How many protons, neutrons, and electrons does Hydrogen-2 have?
Presentation transcript:

A.D.O.M Airborne.Detector.of.Muons Tye Barba Anna Chang Natalina DeFusco David Hood

Background Info A muon is an elementary particle that is a very heavy electron Lifetime of 2.2 microseconds, makes up more then half of cosmic radiation Created when cosmic rays (mostly protons) from deep space hit the earth’s atmosphere at about 15,000m

Experiment Description Two Photomultiplier tubes (PMT), a scintillator panel and a QNET board are sent up to 1000 ft to detect a change in the rate of muons Hypothesis- more muons will be detected at a higher altitude

Description of equipment Scintillator panel PMT QNET board (a)‏ X-BEE Transmitter (b)‏ Power Supply (c)‏ (a)‏ (b)‏ (c)‏

Procedure A gondola was constructed and attached to a weather balloon and lifted to 1000 ft. Data was taken for 30 min. A XBEE transmitter transmits the data to a receiver on the ground. The counts are graphed and analyzed

The Data At ground level the rate was 2.6 counts per minute At 766ft the rate was 94.1 counts per minute We did have a very large discrepancy between the rates from the ground and at 766ft About 36 times more muons at 766ft than at ground level

Sample Data E966E0C7 BB E966E0C B B B E53FE6DC A9 2C F9087C B2 3D A54678A5 A B26F7C B FA3F9F AB A E AC CEF6D BE ][|\| |-|3X/-\|)3(][/\/\/-\|_!!! (hexadecimal)‏

Conclusion We checked the PMT and threshold voltages For this test, the data is valid If repeated, the data would probably change To improve, we would take more sets of data to reduce the error and take an average