Cosmic ray Simulation for Tracking Prototype Hyupwoo Lee MINERvA/Jupiter Group Meeting Oct, 31, 2007.

Slides:

Advertisements

Similar presentations

ORFEOv6r3 10. GeV muons This data MC comparison was made with the last version of ORFEO. Here a new version of the smearing tool is implemented, this is.

Advertisements

Proposal for a new design of LumiCal R. Ingbir, P. Ruzicka, V. Vrba October 07 Malá Skála.

Monte Carlo simulation of the background for the Drell-Yan COMPASS Marialaura Colantoni Laboratory of Nuclear Problems Dubna Marialaura.

$100 $200 $300 $400 $500 $100 $200 $300 $400 $500 $100 $200 $300 $400 $500 $100 $200 $300 $400 $500 $100 $200 $300 $400 $500 $100 $200 $300.

Shadows. Floor Wall Torch Solid Object.

Physics 2225: Optics 1 - Activities with Light Rays Purpose of this Minilab Apply the basics of ray tracing to learn about reflection and refraction of.

Estimating Energy Efficiency of Buildings Matthew Wysocki.

1 Alberto Montanari University of Bologna Simulation of synthetic rainfall series.

Daniele De Gruttola (TOF group – Salerno University and INFN ) 2009 cosmic rays data analysis 09/Dec/09 ALICE - TOF meeting - CERN.

22/5/2011 Particle-ID and Tracking performance in CLIC_ILD1/27 CLIC_ILD particle identification and tracking performance J. Nardulli This talk in 2 parts:

Objectives: Be able to draw an angle in standard position and find the positive and negative rotations. Be able to convert degrees into radians and radians.

Signs of functions in each quadrant. Page 4 III III IV To determine sign (pos or neg), just pick angle in quadrant and determine sign. Now do Quadrants.

Objectives: 1.Be able to draw an angle in standard position and find the positive and negative rotations. 2.Be able to convert degrees into radians and.

Mirrors Physics 202 Professor Lee Carkner Lecture 22.

Hall D Photon Beam Simulation and Rates Part 1: photon beam line Part 2: tagger Richard Jones, University of Connecticut Hall D Beam Line and Tagger Review.

Veto Wall Test Hyupwoo Lee MINERvA/Jupiter Group Meeting Oct, 3, 2007.

OD Calorimetry Study Update — Z vertex position dependence Jaewon Park University of Rochester MINERvA/Jupiter Group Meeting, May 17, 2006.

Markov Chain Update. GIS Coastline Rasterize Coastline in Matlab.

Detector Alignment using cosmic muon data Jaewon Park University of Rochester MINERvA/Jupiter group Meeting, Oct 31, 2007.

Calorimetry Study Update Jaewon Park University of Rochester MINERvA/Jupiter Group Meeting, Mar 22, 2006.

1 Veto Wall Test Hyupwoo Lee MINERvA/Jupiter Group Meeting June 20, 2007.

Final state study Jaewon Park University of Rochester MINERvA/Jupiter Group Meeting, Oct 10, 2007.

Veto Wall Test Hyupwoo Lee MINERvA/Jupiter Group Meeting Oct, 24, 2007.

Final state study Jaewon Park University of Rochester MINERvA/Jupiter Group Meeting, Jan 31, 2007.

Veto Wall Test Hyupwoo Lee MINERvA/Jupiter Group Meeting July 18, 2007.

Mirrors Physics 202 Professor Lee Carkner Lecture 22.

1 Calorimetry Study Update — Angle dependence with cut Jaewon Park University of Rochester MINERvA/Jupiter Group Meeting, May 03, 2006.

MonteCarlo simulation of neutrino interactions in PEANUT Giovanni De Lellis on behalf of Alberto Marotta and Andrea Russo Naples University.

Veto Wall Test Hyupwoo Lee MINERvA/Jupiter Group Meeting Apr, 16, 2008.

Update on the Time-of-Flight and Position Resolution Measurements in the Proposed Detectors and Cost Estimates – August 2014 WILLIAM TIREMAN NORTHERN MICHIGAN.

Commissioning data are taken with individual chambers TP data autotriggered Cosmic rays data  ( different configuration) Different cosmic track angle.

Optics 1 - Activities with Light Rays Purpose of this Minilab Apply the basics of ray tracing to learn about reflection and refraction of light.

Computational Lab in Physics: Final Project Monte Carlo Nuclear Collisions: Glauber Model.

8.2.2 – Graphing Polar Points, Converting Equations.

6.1: Angles and their measure January 5, Objectives Learn basic concepts about angles Apply degree measure to problems Apply radian measure to problems.

$100 $200 $300 $400 $500 $100 $200 $300 $400 $500 $100 $200 $300 $400 $500 $100 $200 $300 $400 $500 $100 $200 $300 $400 $500 $100 $200 $300.

Response of AMANDA-II to Cosmic Ray Muons and study of Systematics Newt,Paolo and Teresa.

Section 4.1 Angles and Their Measures Trigonometry- measurement of angles IMPORTANT VOCABULARY: Angle- determined by rotating a ray about its endpoint.

Chapter 4 Trigonometric Functions. Angles Trigonometry means measurement of triangles. In Trigonometry, an angle often represents a rotation about a point.

Probability Refresher COMP5416 Advanced Network Technologies.

Section 6.3 Polar Coordinates. Another Way of Graphing The rectangular coordinate system we regularly use is not the only means we have of graphing points.

Bartol Flux Calculation presented by Giles Barr, Oxford ICRR-Kashiwa December 2004.

Preliminary Slice Test Track Fitting S. Durkin Sept. 8, 2005 Analyze RunNum1007Evs0to49999.bin using /AnalysisUtilities look for tracks in two separate.

Testing the T-tracker Straw Clustering Code and Stereo Hit Finding Clustering Code Recently implemented by Hans Wenzel (MakeStrawCluster_pluggin.cc) StrawClusters.

Financial Ratios Report Financial Report Results For all Divisions.

K 0 s reconstruction in ALICE Giuseppe Lo Re INFN, Sezione di Catania, and Dipartimento di Fisica e Astronomia, Università di Catania, Italy, March 2002.

Warm ups – solve and graph 1. |x + 4| = |4 – x| < |2x + 3| < 7 4. |2x – 1| < -5.

MP BACH MultiPixel Balloon-borne Air CHerenkov Detection of Iron Cosmic Rays Using Direct Cherenkov Radiation Imaged with a High Resolution Camera 1.

Aim: How do we look at angles as rotation? Do Now: Draw the following angles: a) 60  b) 150  c) 225  HW: p.361 # 4,6,12,14,16,18,20,22,24,33.

VISIBLE PROPERTIES OF COSMIC ANTI-STRING Kotvytskiy A.T., Shulga V.M. Institute of Radio Astronomy of Nat. Ac. Sci. of Ukraine Karazin Kharkov National.

Section 4.1.  A ray is a part of a line that has only one endpoint and extends forever in the opposite direction.  An angle is formed by two rays that.

FCAL Krakow meeting, 6. May LumiCal concept including the tracker R. Ingbir, P.Růžička, V. Vrba.

Can we detect a marble tomb with cosmic muons ? Corinne Goy, Max Chefdeville, Jean Jacquemier, Yannis Karyotakis 21 December 2015.

K. Holubyev HEP2007, Manchester, UK, July 2007 CP asymmetries at D0 Kostyantyn Holubyev (Lancaster University) representing D0 collaboration HEP2007,

Tips Need to Consider When Organizing a College Event

Mieke Bouwhuis on behalf of the ANTARES collaboration

Image #1 Image Analysis: What do you think is going on in this picture? Which person, thing, or event does this image relate to (which Word Wall term)?

Outline Analysis of some real data taken with the GLAST minitower (cosmic rays only). Offline analysis software used. Full Monte Carlo simulation using.

الأستاذ المساعد بقسم المناهج وطرق التدريس

Image #1 Image Analysis: What do you think is going on in this picture? Which person, thing, or event does this image relate to (which Word Wall term)?

ماجستير إدارة المعارض من بريطانيا

Image #1 Image Analysis: What do you think is going on in this picture? Which person, thing, or event does this image relate to (which Word Wall term)?

Image #1 Image Analysis: What do you think is going on in this picture? Which person, thing, or event does this image relate to (which Word Wall term)?

Forward-Backward Asymmetry Study in

Search for long distance correlations by selecting multi-tracks events Update n.1 P.La Rocca and F.Riggi.

low angle (Winkel) high angle (Winkel)

Image #1 Image Analysis: What do you think is going on in this picture? Which person, thing, or event does this image relate to (which Word Wall term)?

For More Details:

Image #1 Image Analysis: What do you think is going on in this picture? Which person, thing, or event does this image relate to (which Word Wall term)?

Presentation transcript:

Cosmic ray Simulation for Tracking Prototype Hyupwoo Lee MINERvA/Jupiter Group Meeting Oct, 31, 2007

2 TP - Wideband Purpose of simulation - To get event rate as a function of angle

3 Parameters & Intensity : Got from PDG data - Random generation : x, y,, a = 2.5 ’ = m b = 10 ’ = m

4 Result - Overall Intensity : Total event rate of hitting both panels

5 Result – theta (polar angle)

6 Result – beta This region should be reduced by wall Negative sign means backward going

7 Result – alpha Negative sign means backward going

8 Conclusion Distance : Keep close as possible as Height : Some value between 0 ~ 1m? => Need more details?