COSMIC RAYS AT EARTH

Size: px
Start display at page:

Download "COSMIC RAYS AT EARTH"

Transcription

1 COSMIC RAYS AT EARTH Researcher's Reference Manual and Data Book Peter K.R Grieder Institute of Physics University of Bern Bern, Switzerland 2001 ELSEVIER Amsterdam - London - New York - Oxford - Paris - Shannon -Tokyo

2 Contents Preface Comments for Reader Acknowledgements v viii ix Cosmic Ray Properties, Relations and Definitions Introduction General Comments Heliospheric Effects and Solar Modulation Propagation of the Hadronic Component in the Atmosphere Strong Interactions Energy Transport Secondary Particles Production of Secondary Particles Energy Spectra of Secondary Particles Decay of Secondaries Decay versus Interaction of Secondaries Electromagnetic Processes and Energy Losses Ionization and Excitation Bremsstrahlung and Pair Production Vertical Development in the Atmosphere Definition of Common Observables Directional Intensity Flux Omnidirectional or Integrated Intensity Zenith Angle Dependence Attenuation Length Altitude Dependence Differential Energy Spectrum 27 XI

3 xii CONTENTS Integral Energy Spectrum The Atmosphere Characteristic Data and Relations Zenith Angle Dependence of the Atmospheric Thickness or Column Density Geomagnetic and Heliospheric Effects East-West, Latitude and Longitude Effects Time Variation and Modulation Geomagnetic Cutoff Cosmic Ray Cutoff Terminology Definitions of Geomagnetic Terms 42 References 47 2 Cosmic Rays in the Atmosphere Introduction Charged Hadrons Introduction Flux Measurements and Intensities Energy Spectra Ratio of Neutral to Charged Hadrons Pions and Pion to Proton Ratio Theoretical Aspects and Calculations 68 References 69 Figures Neutrons Introduction Altitude Dependence of Flux and Intensities Energy Spectra Theoretical Contributions 105 References 106 Figures Gamma Rays Introduction Energy Spectra Below 1 TeV Energy Spectra in the TeV-Range Altitude Dependence of Flux and Intensities Zenith Angle Dependence Monochromatic Gamma Lines Theoretical Contributions 142 References 142 Figures 148

4 CONTENTS xiii 2.5 Electrons (Negatrons and Positrons) Introduction Altitude Dependence of Flux and Intensities Energy Spectra Albedo Component Positrons Charge Ratio and Related Data 203 References 203 Figures Muons Introduction Altitude Dependence of Integral Intensity Momentum and Energy Spectra Charge Ratio Theoretical Contributions 241 References 241 Figures Nuclei Introduction Altitude Dependence of Flux and Intensities Fragmentation Probabilities of Nuclei Momentum Spectra Theoretical Aspects 279 References 280 Figures Antinucleons, Antinuclei Introduction, Experimental Data Theoretical Studies and Expected Intensities References 297 Figures Cosmic Rays at Sea Level Introduction 305 References Charged Hadrons Flux Measurements and Intensities Momentum and Energy Spectra Zenith Angle Dependence Charged Pions Charge and Particle Ratios 313

5 xiv CONTENTS Theoretical Contributions 315 References 316 Figures Neutrons Flux Measurements and Intensities Energy Spectra Zenith Angle Dependence 336 References 336 Figures Gamma Rays Experimental Aspects and Data 342 References 342 Figures Electrons (Negatrons and Positrons) Flux Measurements and Intensities Energy Spectra Charge Ratio Zenith Angle Dependence 347 References 347 Figures Muons Introduction Absolute Flux Measurements and Intensities Momentum and Energy Spectra Zenith and Azimuthal Angular Dependence Charge Ratio : Geomagnetic Latitude Dependence Backscattered Muons at Ground Level Theoretical Contributions 378 References 386 Figures Nuclei General Comments 454 References 454 Figures Antinucleons, Antinuclei General Comments 457 References 457

6 CONTENTS xv 4 Cosmic Rays Underground, Underwater and Under Ice Introduction Theoretical Aspects of Muon Physics Introductory Comments Energy Loss and Survival Probability of Muons in Dense Matter Average Range-Energy Relation of Muons Range Fluctuations of Muons Underground and in Water Average Depth-Intensity Relation of Muons Indirect Determination of the Energy Spectrum Underground and Average Energy 474 References Muons Underground General Comments Rock Composition, Standard Rock and Conversion Formula Depth-Intensity Relations and Data Zenith Angle Dependence and Relations Stopping Muons Prompt or Direct Muons Energy Loss Data of Muons Range-Energy Data of Muons Underground Momentum and Energy Spectra of Muons Underground and Derived Sea Level Spectrum Multi-Muon Events and Decoherence 514 References 520 Figures Muons Under Water and Ice General Comments Intensity versus Depth in Water Zenith Angle Dependence at Great Depth in Water Intensity versus Depth in Ice Theoretical Contributions 596 References 598 Figures Neutrinos, General and Atmospheric Introduction Experimental Aspects and Detection Methods Atmospheric Neutrino Production, Properties

7 xvi CONTENTS Theoretical Neutrino Spectra and Data Experimental Results, Early Work Experimental Results, Modern Work 636 References 641 Figures Primary Cosmic Radiation Introduction 669 References Hadrons, Spectra and Composition Introduction All-Particle Spectrum Charge Resolved Energy Spectra and Chemical Composition Isotopic Composition Conclusions from Composition Observations References 705 Figures? Electrons (Positrons and Negatrons) Introduction Energy Spectra Positron Fraction Atmospheric Secondary Electron Contamination Theoretical Contributions 772 References 773 Figures X- and Gamma Rays Introduction General Survey of Gamma Radiation Diffuse Galactic Gamma Radiation Diffuse Cosmic Gamma Radiation Point Sources Gamma Ray Line Spectra Gamma Ray Fraction of Cosmic Radiation 806 References 806 Figures Neutrinos and Antineutrinos General Comments Neutrinos from the Supernova SN-1987A Energetic Neutrinos from Astrophysical Sources.. 843

8 CONTENTS xvii Experimental Upper Limits of Neutrino Fluxes from Astrophysical Point Sources 845 References 848 Figures Antiprotons and Antimatter Discovery of Cosmic Ray Antiprotons Detection Methods Measured Antiproton Intensities and p/p Ratios Antinuclei Theoretical Studies 871 References 874 Figures Heliospheric Phenomena Introduction 893 References Heliospheric, Magnetospheric and Terrestrial Magnetic Fields ^ Introduction ' Heliospheric Magnetic Field and Solar Wind Geomagnetic and Magnetospheric Fields Interplanetary Magnetic Fields 900 References 900 Figures Time Variation and Modulation Effects Introduction Atmospherically Induced Variations Solar Diurnal Variations Sidereal Variations and Anisotropies Compton-Getting Effect Forbush Decreases Day Variations Year and 22-Year Variations Long-Term Variations 913 References 916 Figures Energetic Solar Particles and Photons Introduction Solar Flares Photons and Particles from Solar Flares Ionospheric Effects 931

9 xviii CONTENTS References 931 Figures Anomalous Cosmic Rays Introduction Theoretical Aspects Current Status of Anomalous Cosmic Rays 940 References 940 Figures Solar Neutrinos Introduction The Solar Neutrino Unit (SNU) The Solar Neutrino Problem and Recent Results Homestake Chlorine Detector and Data GALLEX Detector and Data SAGE Detector and Data Kamiokande Detector and Data Super-Kamiokande (SK) Detector and Data New and Future Detectors 959 References 960 Figures Miscellaneous Topics General Comments Cosmogenic Nuclides Introductory Comments Cosmogenic Nuclides in the Atmosphere Cosmogenic Nuclides in Rock 981 References '. 982 Figures Galactic and Intergalactic Magnetic Fields Introduction Galactic Magnetic Fields Intergalactic Magnetic Fields Magnetic Fields of Astrophysical Objects 991 References 992 Figures Antarctic Atmosphere General Comments Determination of Atmospheric Profile and Data References Optical and Related Properties of Water and Ice 996

10 CONTENTS xix General Comments Definitions Depth Profiles of Ocean Parameters Optical Attenuation in Water and Ice Optical Background in Water and Ice Sedimentation in the Ocean 1008 References 1009 Figures 1014 A Miscellaneous Data: Tables 1029 A.I Comments to Tables 1029 A. 1.1 COSPAR Reference Atmosphere 1029 A. 1.2 Solar System Elemental Abundances 1029 A. 1.3 Radiation Lengths and Critical Energies of Materials 1029 A. 1.4 Elements and their Material Parameters 1029 A. 1.5 Muon Energy Losses in Elements and Compounds... p 1030 A. 1.6 Units, Conversion Factors, Constants and Parameters 1031 A.2 COSPAR Reference Atmosphere 1032 A.3 Solar System Elemental Abundances 1035 A.4 Radiation Lengths and Critical Energies 1039 A.5 Elements and their Material Parameters 1040 A.6 Muon Energy Loss in Various Elements 1041 A.7 Muon Energy Loss in Compounds 1043 A.8 Units and Conversion Factors 1045 A.9 Constants and Parameters 1046 References 1047 B Miscellaneous Data: Figures 1049 B.I Comments to Figures 1049 References 1049 B.2 Kinetic Energy - Rigidity Conversion 1051 B.3 Gyroradius versus Proton Energy 1052 B.4 Ionization versus Depth in Atmosphere 1053 B.5 Nucleon Lifetime Limits 1054 C Cosmic Ray Experiments of Past and Present 1055 C.I Cosmic Ray Ground Level Facilities 1055 C.I.I Comments to Tables 1055

11 xx CONTENTS C.1.2 EAS Array Sites of Past and Present 1056 C.I.3 Air Cherenkov Array /Telescope Sites 1058 References 1058 C.I.4 Emulsion Chamber Sites 1059 C.2 Balloon Experiments 1059 C.3 Underground, Underwater, Under Ice Experiments 1060 D Miscellany 1061 D.I Acronyms of some Experiments 1061 D.2 List of Symbols 1064 D.3 List of Abbreviations 1067 D.4 List of Cosmic Ray Conferences 1069 Index 1070

Nuclear Physics. Nuclear Physics comprises the study of:

Nuclear Physics. Nuclear Physics comprises the study of: Nuclear Physics Nuclear Physics comprises the study of: The general properties of nuclei The particles contained in the nucleus The interaction between these particles Radioactivity and nuclear reactions

More information

Ay 122 - Fall 2004. The Sun. And The Birth of Neutrino Astronomy. This printout: Many pictures missing, in order to keep the file size reasonable

Ay 122 - Fall 2004. The Sun. And The Birth of Neutrino Astronomy. This printout: Many pictures missing, in order to keep the file size reasonable Ay 122 - Fall 2004 The Sun And The Birth of Neutrino Astronomy This printout: Many pictures missing, in order to keep the file size reasonable Why Study the Sun? The nearest star - can study it in a greater

More information

Cosmic Ray Astrophysics with AMS-02 Daniel Haas - Université de Genève on behalf of the AMS collaboration

Cosmic Ray Astrophysics with AMS-02 Daniel Haas - Université de Genève on behalf of the AMS collaboration Cosmic Ray Astrophysics with AMS-02 Daniel Haas - Université de Genève on behalf of the AMS collaboration Overview of AMS-02 Cosmic ray studies p/he, Z>2, p/e +, γ-rays Comparison AMS vs. GLAST AMS vs.

More information

Masses in Atomic Units

Masses in Atomic Units Nuclear Composition - the forces binding protons and neutrons in the nucleus are much stronger (binding energy of MeV) than the forces binding electrons to the atom (binding energy of ev) - the constituents

More information

Main properties of atoms and nucleus

Main properties of atoms and nucleus Main properties of atoms and nucleus. Atom Structure.... Structure of Nuclei... 3. Definition of Isotopes... 4. Energy Characteristics of Nuclei... 5. Laws of Radioactive Nuclei Transformation... 3. Atom

More information

Interstellar Cosmic-Ray Spectrum from Gamma Rays and Synchrotron

Interstellar Cosmic-Ray Spectrum from Gamma Rays and Synchrotron Interstellar Cosmic-Ray Spectrum from Gamma Rays and Synchrotron Chuck Naval Research Laboratory, Washington, DC charles.dermer@nrl.navy.mil Andy Strong Max-Planck-Institut für extraterrestrische Physik,

More information

Discovery of neutrino oscillations

Discovery of neutrino oscillations INSTITUTE OF PHYSICS PUBLISHING Rep. Prog. Phys. 69 (2006) 1607 1635 REPORTS ON PROGRESS IN PHYSICS doi:10.1088/0034-4885/69/6/r01 Discovery of neutrino oscillations Takaaki Kajita Research Center for

More information

Atomic and Nuclear Physics Laboratory (Physics 4780)

Atomic and Nuclear Physics Laboratory (Physics 4780) Gamma Ray Spectroscopy Week of September 27, 2010 Atomic and Nuclear Physics Laboratory (Physics 4780) The University of Toledo Instructor: Randy Ellingson Gamma Ray Production: Co 60 60 60 27Co28Ni *

More information

Objectives. PAM1014 Introduction to Radiation Physics. Constituents of Atoms. Atoms. Atoms. Atoms. Basic Atomic Theory

Objectives. PAM1014 Introduction to Radiation Physics. Constituents of Atoms. Atoms. Atoms. Atoms. Basic Atomic Theory PAM1014 Introduction to Radiation Physics Basic Atomic Theory Objectives Introduce and Molecules The periodic Table Electronic Energy Levels Atomic excitation & de-excitation Ionisation Molecules Constituents

More information

UNIVERSITA DEGLI STUDI DI MILANO FACOLTA DI SCIENZE MATEMATICHE, FISICHE E NATURALI DOTTORATO DI RICERCA IN FISICA, ASTROFISICA E FISICA APPLICATA

UNIVERSITA DEGLI STUDI DI MILANO FACOLTA DI SCIENZE MATEMATICHE, FISICHE E NATURALI DOTTORATO DI RICERCA IN FISICA, ASTROFISICA E FISICA APPLICATA UNIVERSITA DEGLI STUDI DI MILANO FACOLTA DI SCIENZE MATEMATICHE, FISICHE E NATURALI DOTTORATO DI RICERCA IN FISICA, ASTROFISICA E FISICA APPLICATA THE CALCULATION OF ATMOSPHERIC MUON FLUX USING THE FLUKA

More information

Solar Ast ro p h y s ics

Solar Ast ro p h y s ics Peter V. Foukal Solar Ast ro p h y s ics Second, Revised Edition WI LEY- VCH WILEY-VCH Verlag Co. KCaA Contents Preface 1 1.1 1.2 1.3 1.4 1.5 1.6 1.7 1.8 1.9 2 2.1 2.1.1 2.1.2 2.2 2.2.1 2.2.2 2.2.3 2.3

More information

Chemistry 1000 Lecture 2: Nuclear reactions and radiation. Marc R. Roussel

Chemistry 1000 Lecture 2: Nuclear reactions and radiation. Marc R. Roussel Chemistry 1000 Lecture 2: Nuclear reactions and radiation Marc R. Roussel Nuclear reactions Ordinary chemical reactions do not involve the nuclei, so we can balance these reactions by making sure that

More information

Space Weather: An Introduction C. L. Waters. Centre for Space Physics University of Newcastle, Australia

Space Weather: An Introduction C. L. Waters. Centre for Space Physics University of Newcastle, Australia Space Weather: An Introduction C. L. Waters Centre for Space Physics University of Newcastle, Australia 1 Outline Space weather: Conditions on the Sun and in the solar wind, magnetosphere, ionosphere and

More information

CHEM 1411 Chapter 5 Homework Answers

CHEM 1411 Chapter 5 Homework Answers 1 CHEM 1411 Chapter 5 Homework Answers 1. Which statement regarding the gold foil experiment is false? (a) It was performed by Rutherford and his research group early in the 20 th century. (b) Most of

More information

SPACE WEATHER SUPPORT FOR COMMUNICATIONS. Overview

SPACE WEATHER SUPPORT FOR COMMUNICATIONS. Overview SPACE WEATHER SUPPORT FOR COMMUNICATIONS Overview Ionospheric variability (space weather) significantly impacts ground and space-based communications. In essence, the electrically charged particles of

More information

ASTROPARTICLE PHYSICS WITH AMS-02: THE QUEST OF ANTIMATTER

ASTROPARTICLE PHYSICS WITH AMS-02: THE QUEST OF ANTIMATTER ASTROPARTICLE PHYSICS WITH AMS-02: THE QUEST OF ANTIMATTER C.Sbarra a on behalf of the AMS collaboration INFN of Bologna, Viale B.Pichat 6/2 I-40127 Bologna, Italy Abstract.The Alpha Magnetic Spectrometer,

More information

Pearson Physics Level 30 Unit VIII Atomic Physics: Chapter 17 Solutions

Pearson Physics Level 30 Unit VIII Atomic Physics: Chapter 17 Solutions Pearson Physics Level 30 Unit VIII Atomic Physics: Chapter 17 Solutions Student Book page 831 Concept Check Since neutrons have no charge, they do not create ions when passing through the liquid in a bubble

More information

Solar Activity and Earth's Climate

Solar Activity and Earth's Climate Rasmus E. Benestad Solar Activity and Earth's Climate Second Edition Published in association with Springer Praxis ids Publishing Publisl PRAXI Chichester, UK Contents Preface to the second edition Preface

More information

R. Singh B. Veenadhari S. Alex Indian Institute of Geomagnetism, Navi Mumbai - 410218

R. Singh B. Veenadhari S. Alex Indian Institute of Geomagnetism, Navi Mumbai - 410218 Very Low Frequency (VLF) studies of ionospheric-magnetospheric electromagnetic phenomena in Indian low latitude region using AWESOME receivers R. Singh B. Veenadhari S. Alex Indian Institute of Geomagnetism,

More information

............... [2] At the time of purchase of a Strontium-90 source, the activity is 3.7 10 6 Bq.

............... [2] At the time of purchase of a Strontium-90 source, the activity is 3.7 10 6 Bq. 1 Strontium-90 decays with the emission of a β-particle to form Yttrium-90. The reaction is represented by the equation 90 38 The decay constant is 0.025 year 1. 90 39 0 1 Sr Y + e + 0.55 MeV. (a) Suggest,

More information

Basics of Nuclear Physics and Fission

Basics of Nuclear Physics and Fission Basics of Nuclear Physics and Fission A basic background in nuclear physics for those who want to start at the beginning. Some of the terms used in this factsheet can be found in IEER s on-line glossary.

More information

Unit 1 Practice Test. Matching

Unit 1 Practice Test. Matching Unit 1 Practice Test Matching Match each item with the correct statement below. a. proton d. electron b. nucleus e. neutron c. atom 1. the smallest particle of an element that retains the properties of

More information

Basic Nuclear Concepts

Basic Nuclear Concepts Section 7: In this section, we present a basic description of atomic nuclei, the stored energy contained within them, their occurrence and stability Basic Nuclear Concepts EARLY DISCOVERIES [see also Section

More information

Noble Gases. Outline Nobel Gas Elements Radon and Health Chemistry Homework

Noble Gases. Outline Nobel Gas Elements Radon and Health Chemistry Homework Radon and Other Noble Gases The elements in the last column of the periodic table are all very stable, mono-atomic gases. Until 1962, they were called inert gases because they did not react with other

More information

For convenience, we may consider an atom in two parts: the nucleus and the electrons.

For convenience, we may consider an atom in two parts: the nucleus and the electrons. Atomic structure A. Introduction: In 1808, an English scientist called John Dalton proposed an atomic theory based on experimental findings. (1) Elements are made of extremely small particles called atoms.

More information

Space Users: Status, Requirements and Open Issues

Space Users: Status, Requirements and Open Issues Space Users: Status, Requirements and Open Issues Despite asking a number of key people, I only received 1.5 responses of user requirements... Are space users too busy or just simply happy? :-) I will

More information

Cosmic Rays: A Century of Mysteries

Cosmic Rays: A Century of Mysteries percorsi Cosmic Rays: A Century of Mysteries Angela V. Olinto* Department of Astronomy & Astrophysics Kavli Institute for Cosmological Physics Enrico Fermi Institute, The University of Chicago, Chicago,

More information

Introduction to Nuclear Physics

Introduction to Nuclear Physics Introduction to Nuclear Physics 1. Atomic Structure and the Periodic Table According to the Bohr-Rutherford model of the atom, also called the solar system model, the atom consists of a central nucleus

More information

F321 THE STRUCTURE OF ATOMS. ATOMS Atoms consist of a number of fundamental particles, the most important are... in the nucleus of an atom

F321 THE STRUCTURE OF ATOMS. ATOMS Atoms consist of a number of fundamental particles, the most important are... in the nucleus of an atom Atomic Structure F32 TE STRUCTURE OF ATOMS ATOMS Atoms consist of a number of fundamental particles, the most important are... Mass / kg Charge / C Relative mass Relative Charge PROTON NEUTRON ELECTRON

More information

The solar wind (in 90 minutes) Mathew Owens

The solar wind (in 90 minutes) Mathew Owens The solar wind (in 90 minutes) Mathew Owens 5 th Sept 2013 STFC Advanced Summer School m.j.owens@reading.ac.uk Overview There s simply too much to cover in 90 minutes Hope to touch on: Formation of the

More information

Nuclear Physics and Radioactivity

Nuclear Physics and Radioactivity Nuclear Physics and Radioactivity 1. The number of electrons in an atom of atomic number Z and mass number A is 1) A 2) Z 3) A+Z 4) A-Z 2. The repulsive force between the positively charged protons does

More information

Jorge E. Fernández Laboratory of Montecuccolino (DIENCA), Alma Mater Studiorum University of Bologna, via dei Colli, 16, 40136 Bologna, Italy

Jorge E. Fernández Laboratory of Montecuccolino (DIENCA), Alma Mater Studiorum University of Bologna, via dei Colli, 16, 40136 Bologna, Italy Information technology (IT) for teaching X- and gamma-ray transport: the computer codes MUPLOT and SHAPE, and the web site dedicated to photon transport Jorge E. Fernández Laboratory of Montecuccolino

More information

Theoretical Particle Physics FYTN04: Oral Exam Questions, version ht15

Theoretical Particle Physics FYTN04: Oral Exam Questions, version ht15 Theoretical Particle Physics FYTN04: Oral Exam Questions, version ht15 Examples of The questions are roughly ordered by chapter but are often connected across the different chapters. Ordering is as in

More information

THE STOCKHOLM EDUCATIONAL AIR SHOWER ARRAY

THE STOCKHOLM EDUCATIONAL AIR SHOWER ARRAY THE STOCKHOLM EDUCATIONAL AIR SHOWER ARRAY Mark Pearce (1) (1) KTH, Department of Physics, AlbaNova University Centre, 10691 Stockholm, Sweden. Email: pearce@particle.kth.se ABSTRACT The primary goal of

More information

Mars Atmosphere and Volatile EvolutioN (MAVEN) Mission

Mars Atmosphere and Volatile EvolutioN (MAVEN) Mission Mars Atmosphere and Volatile EvolutioN (MAVEN) Mission MAVEN Science Community Workshop December 2, 2012 Particles and Fields Package Solar Energetic Particle Instrument (SEP) Davin Larson and the SEP

More information

AQA Level 1/2 Certificate in Physics PAPER 1 SPECIMEN MARK SCHEME. AQA Level 1/2 Certificate in Physics Paper 1 MS

AQA Level 1/2 Certificate in Physics PAPER 1 SPECIMEN MARK SCHEME. AQA Level 1/2 Certificate in Physics Paper 1 MS AQA Level /2 Certificate in Physics PAPER SPECIMEN MARK SCHEME AQA Level /2 Certificate in Physics Paper MS MARK SCHEME Information to Examiners. General The mark scheme for each question shows: the marks

More information

8.1 Radio Emission from Solar System objects

8.1 Radio Emission from Solar System objects 8.1 Radio Emission from Solar System objects 8.1.1 Moon and Terrestrial planets At visible wavelengths all the emission seen from these objects is due to light reflected from the sun. However at radio

More information

Titan: The Solar System s Abiotic Petroleum Factory

Titan: The Solar System s Abiotic Petroleum Factory Titan: The Solar System s Abiotic Petroleum Factory J. Hunter Waite, Ph.D. Institute Scientist Space Science & Engineering Division Southwest Research Institute Titan: The Solar System s Abiotic Petroleum

More information

CSSAR Space Science Cooperation

CSSAR Space Science Cooperation CSSAR Space Science Cooperation WANG Shuzhi Center for Space Science and Applied Research Chinese Academy of Science(CSSAR) Table of Contents Brief History of CSSAR International Cooperation CAS Strategic

More information

Particle Soup: Big Bang Nucleosynthesis

Particle Soup: Big Bang Nucleosynthesis Name: Partner(s): Lab #7 Particle Soup: Big Bang Nucleosynthesis Purpose The student explores how helium was made in the Big Bang. Introduction Very little helium is made in stars. Yet the universe is

More information

1 Introduction. 1 There may, of course, in principle, exist other universes, but they are not accessible to our

1 Introduction. 1 There may, of course, in principle, exist other universes, but they are not accessible to our 1 1 Introduction Cosmology is the study of the universe as a whole, its structure, its origin, and its evolution. Cosmology is soundly based on observations, mostly astronomical, and laws of physics. These

More information

arxiv:hep-ex/0203014v1 8 Mar 2002

arxiv:hep-ex/0203014v1 8 Mar 2002 Cosmogenesis Backgrounds, Experiment Depth and the Solar Neutrino TPC G. Bonvicini, A. Schreiner arxiv:hep-ex/0203014v1 8 Mar 2002 Abstract Wayne State University, Detroit MI 48201 A Time Projection Chamber

More information

Astrophysical Techniques. C R Kitchin

Astrophysical Techniques. C R Kitchin Astrophysical Techniques C R Kitchin University of Hertfordshire Observatory Third Edition SUB Gottingen 7 210 119 268 99 A 8843 Institute of Physics Publishing Bristol and Philadelphia Contents Preface

More information

The accurate calibration of all detectors is crucial for the subsequent data

The accurate calibration of all detectors is crucial for the subsequent data Chapter 4 Calibration The accurate calibration of all detectors is crucial for the subsequent data analysis. The stability of the gain and offset for energy and time calibration of all detectors involved

More information

hij Teacher Resource Bank GCE Physics A Other Guidance: Particle Physics By J Breithaupt

hij Teacher Resource Bank GCE Physics A Other Guidance: Particle Physics By J Breithaupt hij Teacher Resource Bank GCE Physics A Other Guidance: Particle Physics By J Breithaupt Copyright 2008 AQA and its licensors. All rights reserved. The Assessment and Qualifications Alliance (AQA) is a

More information

Search for supersymmetric Dark Matter with GLAST!!

Search for supersymmetric Dark Matter with GLAST!! Search for supersymmetric Dark Matter with GLAST!! Aldo Morselli INFN, Sezione di Roma 2 & Università di Roma Tor Vergata ICCRC2003 The 28th International Cosmic Ray Conference Tsukuba, Japan, July 31-

More information

Atomic Calculations. 2.1 Composition of the Atom. number of protons + number of neutrons = mass number

Atomic Calculations. 2.1 Composition of the Atom. number of protons + number of neutrons = mass number 2.1 Composition of the Atom Atomic Calculations number of protons + number of neutrons = mass number number of neutrons = mass number - number of protons number of protons = number of electrons IF positive

More information

Cross section, Flux, Luminosity, Scattering Rates

Cross section, Flux, Luminosity, Scattering Rates Cross section, Flux, Luminosity, Scattering Rates Table of Contents Paul Avery (Andrey Korytov) Sep. 9, 013 1 Introduction... 1 Cross section, flux and scattering... 1 3 Scattering length λ and λ ρ...

More information

Nuclear Fusion and Radiation

Nuclear Fusion and Radiation Nuclear Fusion and Radiation Lecture 8 (Meetings 19, 20, 21 & 22) Eugenio Schuster schuster@lehigh.edu Mechanical Engineering and Mechanics Lehigh University Nuclear Fusion and Radiation p. 1/66 The discovery

More information

Topic 3. Evidence for the Big Bang

Topic 3. Evidence for the Big Bang Topic 3 Primordial nucleosynthesis Evidence for the Big Bang! Back in the 1920s it was generally thought that the Universe was infinite! However a number of experimental observations started to question

More information

Objectives 404 CHAPTER 9 RADIATION

Objectives 404 CHAPTER 9 RADIATION Objectives Explain the difference between isotopes of the same element. Describe the force that holds nucleons together. Explain the relationship between mass and energy according to Einstein s theory

More information

Information about the T9 beam line and experimental facilities

Information about the T9 beam line and experimental facilities Information about the T9 beam line and experimental facilities The incoming proton beam from the PS accelerator impinges on the North target and thus produces the particles for the T9 beam line. The collisions

More information

Establishing and Using the real-time Neutron Monitor Database (NMDB)

Establishing and Using the real-time Neutron Monitor Database (NMDB) **FULL TITLE** ASP Conference Series, Vol. **VOLUME**, **YEAR OF PUBLICATION** **NAMES OF EDITORS** Establishing and Using the real-time Neutron Monitor Database (NMDB) H. Mavromichalaki, A. Papaioannou,

More information

The Birth of the Universe Newcomer Academy High School Visualization One

The Birth of the Universe Newcomer Academy High School Visualization One The Birth of the Universe Newcomer Academy High School Visualization One Chapter Topic Key Points of Discussion Notes & Vocabulary 1 Birth of The Big Bang Theory Activity 4A the How and when did the universe

More information

Chapter NP-5. Nuclear Physics. Nuclear Reactions TABLE OF CONTENTS INTRODUCTION OBJECTIVES 1.0 NUCLEAR REACTIONS 2.0 NEUTRON INTERACTIONS

Chapter NP-5. Nuclear Physics. Nuclear Reactions TABLE OF CONTENTS INTRODUCTION OBJECTIVES 1.0 NUCLEAR REACTIONS 2.0 NEUTRON INTERACTIONS Chapter NP-5 Nuclear Physics Nuclear Reactions TABLE OF CONTENTS INTRODUCTION OBJECTIVES 1.0 2.0 NEUTRON INTERACTIONS 2.1 ELASTIC SCATTERING 2.2 INELASTIC SCATTERING 2.3 RADIATIVE CAPTURE 2.4 PARTICLE

More information

Chapter 18: The Structure of the Atom

Chapter 18: The Structure of the Atom Chapter 18: The Structure of the Atom 1. For most elements, an atom has A. no neutrons in the nucleus. B. more protons than electrons. C. less neutrons than electrons. D. just as many electrons as protons.

More information

High Energy Physics. Lecture 4 More kinematics and a picture show of particle collisions

High Energy Physics. Lecture 4 More kinematics and a picture show of particle collisions High Energy Physics Lecture 4 More kinematics and a picture show of particle collisions 1 Recall from the previous lecture: the momentum of the scattered Particle in an elastic collision is given by p

More information

(3) Interaction of high energy photons with matter

(3) Interaction of high energy photons with matter (3) Interaction of high energy photons with matter Photoelectric Absorption (Inverse) Compton Scattering Electron-positron pair production Application in Detectors 1 Photoelectric Absorption Similar to

More information

3 Atomic Structure 15

3 Atomic Structure 15 3 Atomic Structure 15 3.1 Atoms You need to be familiar with the terms in italics The diameter of the nucleus is approximately 10-15 m and an atom 10-10 m. All matter consists of atoms. An atom can be

More information

The VHE future. A. Giuliani

The VHE future. A. Giuliani The VHE future A. Giuliani 1 The Cherenkov Telescope Array Low energy Medium energy High energy 4.5o FoV 7o FoV 10o FoV 2000 pixels 2000 pixels 2000 pixels ~ 0.1 ~ 0.18 ~ 0.2-0.3 The Cherenkov Telescope

More information

Atoms, Ions and Molecules The Building Blocks of Matter

Atoms, Ions and Molecules The Building Blocks of Matter Atoms, Ions and Molecules The Building Blocks of Matter Chapter 2 1 Chapter Outline 2.1 The Rutherford Model of Atomic Structure 2.2 Nuclides and Their Symbols 2.3 Navigating the Periodic Table 2.4 The

More information

Computer Animation of Extensive Air Showers Interacting with the Milagro Water Cherenkov Detector

Computer Animation of Extensive Air Showers Interacting with the Milagro Water Cherenkov Detector Computer Animation of Extensive Air Showers Interacting with the Milagro Water Cherenkov Detector Miguel F. Morales Department of Physics, University of California, Santa Cruz, CA 95064, USA We employ

More information

Gamma Rays from Molecular Clouds and the Origin of Galactic Cosmic Rays. Stefano Gabici APC, Paris

Gamma Rays from Molecular Clouds and the Origin of Galactic Cosmic Rays. Stefano Gabici APC, Paris Gamma Rays from Molecular Clouds and the Origin of Galactic Cosmic Rays Stefano Gabici APC, Paris The Origin of galactic Cosmic Rays Facts: the spectrum is (ALMOST) a single power law -> CR knee at few

More information

Evaluation Tools for the Performance of a NESTOR Test Detector

Evaluation Tools for the Performance of a NESTOR Test Detector Evaluation Tools for the Performance of a NESTOR Test Detector G. Bourlis, A. Leisos, S. E. Tzamarias and A. Tsirigotis Particle and Astroparticle Physics Group School of Science and Technology Hellenic

More information

Aviation Route Dose Calculation and its Numerical Basis

Aviation Route Dose Calculation and its Numerical Basis Aviation Route Dose Calculation and its Numerical Basis H.Schraube 1, W.Heinrich 2, G.Leuthold 1, V.Mares 3 and S.Roesler 4 1 GSF - National Research Center for Environment and Health, D-85758 Neuherberg,

More information

GCE Physics A. Mark Scheme for June 2014. Unit G485: Fields, Particles and Frontiers of Physics. Advanced GCE. Oxford Cambridge and RSA Examinations

GCE Physics A. Mark Scheme for June 2014. Unit G485: Fields, Particles and Frontiers of Physics. Advanced GCE. Oxford Cambridge and RSA Examinations GCE Physics A Unit G485: Fields, Particles and Frontiers of Physics Advanced GCE Mark Scheme for June 014 Oxford Cambridge and RSA Examinations OCR (Oxford Cambridge and RSA) is a leading UK awarding body,

More information

Tutorial 4.6 Gamma Spectrum Analysis

Tutorial 4.6 Gamma Spectrum Analysis Tutorial 4.6 Gamma Spectrum Analysis Slide 1. Gamma Spectrum Analysis In this module, we will apply the concepts that were discussed in Tutorial 4.1, Interactions of Radiation with Matter. Slide 2. Learning

More information

WELCOME to Aurorae In the Solar System. J.E. Klemaszewski

WELCOME to Aurorae In the Solar System. J.E. Klemaszewski WELCOME to Aurorae In the Solar System Aurorae in the Solar System Sponsoring Projects Galileo Europa Mission Jupiter System Data Analysis Program ACRIMSAT Supporting Projects Ulysses Project Outer Planets

More information

Malcolm S. Longair. Galaxy Formation. With 141 Figures and 12 Tables. Springer

Malcolm S. Longair. Galaxy Formation. With 141 Figures and 12 Tables. Springer Malcolm S. Longair Galaxy Formation With 141 Figures and 12 Tables Springer Contents Part I Preliminaries 1. Introduction, History and Outline 3 1.1 Prehistory 3 1.2 The Theory of the Expanding Universe

More information

Muon Fluence Measurements for Homeland Security Applications

Muon Fluence Measurements for Homeland Security Applications Muon Fluence Measurements for Homeland Security Applications Austin Ankney and Tim Berguson, Juniata College James Borgardt, Juniata College Faculty Richard T. Kouzes, PNNL Mentor July 2010 DISCLAIMER

More information

23. The Beginning of Time. Agenda. Agenda. ESA s Venus Express. Conditions in the Early Universe. 23.1 Running the Expansion Backward

23. The Beginning of Time. Agenda. Agenda. ESA s Venus Express. Conditions in the Early Universe. 23.1 Running the Expansion Backward 23. The Beginning of Time Somewhere, something incredible is waiting to be known. Agenda Announce: Solar Altitude Lab (#2) due today Read Ch. 24 for Thursday Observation make-up next week Project Presentations

More information

Curriculum for Excellence. Higher Physics. Success Guide

Curriculum for Excellence. Higher Physics. Success Guide Curriculum for Excellence Higher Physics Success Guide Electricity Our Dynamic Universe Particles and Waves Electricity Key Area Monitoring and Measuring A.C. Monitoring alternating current signals with

More information

Introduction to Geiger Counters

Introduction to Geiger Counters Introduction to Geiger Counters A Geiger counter (Geiger-Muller tube) is a device used for the detection and measurement of all types of radiation: alpha, beta and gamma radiation. Basically it consists

More information

REALIZING EINSTEIN S DREAM Exploring Our Mysterious Universe

REALIZING EINSTEIN S DREAM Exploring Our Mysterious Universe REALIZING EINSTEIN S DREAM Exploring Our Mysterious Universe The End of Physics Albert A. Michelson, at the dedication of Ryerson Physics Lab, U. of Chicago, 1894 The Miracle Year - 1905 Relativity Quantum

More information

ABSORPTION OF BETA AND GAMMA RADIATION

ABSORPTION OF BETA AND GAMMA RADIATION ABSORPTION OF BETA AND GAMMA RADIATION The purpose of this experiment is to understand the interaction of radiation and matter, and the application to radiation detection and shielding Apparatus: 137 Cs

More information

Biasing. 7 th FLUKA Course NEA Paris, Sept.29-Oct.3, 2008

Biasing. 7 th FLUKA Course NEA Paris, Sept.29-Oct.3, 2008 Biasing 7 th FLUKA Course NEA Paris, Sept.29-Oct.3, 2008 Overview General concepts: Analog vs. biased Monte Carlo calculation Biasing options (only the most important / common options available in FLUKA)

More information

1. Photon Beam Damage and Charging at Solid Surfaces John H. Thomas III

1. Photon Beam Damage and Charging at Solid Surfaces John H. Thomas III 1. Photon Beam Damage and Charging at Solid Surfaces John H. Thomas III 1. Introduction............................. 2. Electrostatic Charging of Samples in Photoemission Experiments............................

More information

Solar wind - atmospheric electricity - cloud microphysics connections to weather

Solar wind - atmospheric electricity - cloud microphysics connections to weather ISSI, Bern, Switzerland January 2015 Solar wind - atmospheric electricity - cloud microphysics connections to weather Mai Mai Lam (BAS) Brian A. Tinsley (University of Texas at Dallas) Outline Aerosols,

More information

The energy spectrum of cosmic rays measured with the HEAT extension at the Pierre Auger Observatory

The energy spectrum of cosmic rays measured with the HEAT extension at the Pierre Auger Observatory The energy spectrum of cosmic rays measured with the HEAT extension at the Pierre Auger Observatory Von der Fakultät für Mathematik, Informatik und Naturwissenschaften der RWTH Aachen University zur Erlangung

More information

Coordinate generators

Coordinate generators SPENVIS Upgrades Coordinate generators Merge orbit generator and grid generator: Simplification of model implementation Simplification of model presentation and navigation Orbit generator: Add NORAD Two

More information

Corso di Fisica Te T cnica Ambientale Solar Radiation

Corso di Fisica Te T cnica Ambientale Solar Radiation Solar Radiation Solar radiation i The Sun The Sun is the primary natural energy source for our planet. It has a diameter D = 1.39x10 6 km and a mass M = 1.989x10 30 kg and it is constituted by 1/3 of He

More information

Performance Studies for the KM3NeT Neutrino Telescope

Performance Studies for the KM3NeT Neutrino Telescope Performance Studies for the KM3NeT Neutrino Telescope Der Naturwissenschaftlichen Fakultät der Friedrich-Alexander-Universität Erlangen-Nürnberg zur Erlangung des Doktorgrades vorgelegt von Claudio Kopper

More information

1. In the general symbol cleus, which of the three letters. 2. What is the mass number of an alpha particle?

1. In the general symbol cleus, which of the three letters. 2. What is the mass number of an alpha particle? 1. In the general symbol cleus, which of the three letters Z A X for a nu represents the atomic number? 2. What is the mass number of an alpha particle? 3. What is the mass number of a beta particle? 4.

More information

Future Extensive Air Shower arrays: From Gamma-Ray Astronomy to Cosmic Rays

Future Extensive Air Shower arrays: From Gamma-Ray Astronomy to Cosmic Rays DOI:.51/epjconf/2016124005 Future Extensive Air Shower arrays: From Gamma-Ray Astronomy to Cosmic Rays Giuseppe Di Sciascio a INFN, Sezione Roma Tor Vergata Abstract. Despite large progresses in building

More information

EASA Safety Information Bulletin

EASA Safety Information Bulletin EASA Safety Information Bulletin SIB No.: 2012-09 Issued: 23 May 2012 Subject: Effects of Space Weather on Aviation Ref. Publication: 1. EU OPS 1.390 Cosmic Radiation; 2. SIB 2012-10 Single Event Effects

More information

KE A = PE MAX 1/2M v 2 = k q1 q2 /R

KE A = PE MAX 1/2M v 2 = k q1 q2 /R CHAPTER 13 NUCLEAR STRUCTURE NUCLEAR FORCE The nucleus is help firmly together by the nuclear or strong force, We can estimate the nuclear force by observing that protons residing about 1fm = 10-15m apart

More information

Fundamental Physics at Extreme High Energies

Fundamental Physics at Extreme High Energies Fundamental Physics at Extreme High Energies Michael Kachelrieß NTNU, Trondheim [] Outline: Introduction Testing (new?) strong interactions Lorentz invariance violation Topological defects & superheavy

More information

Environmental Health and Safety Radiation Safety. Module 1. Radiation Safety Fundamentals

Environmental Health and Safety Radiation Safety. Module 1. Radiation Safety Fundamentals Environmental Health and Safety Radiation Safety Module 1 Radiation Safety Fundamentals Atomic Structure Atoms are composed of a variety of subatomic particles. The three of interest to Health Physics

More information

NOTES ON The Structure of the Atom

NOTES ON The Structure of the Atom NOTES ON The Structure of the Atom Chemistry is the study of matter and its properties. Those properties can be explained by examining the atoms that compose the matter. An atom is the smallest particle

More information

SINP SPACE MONITORING DATA CENTER PORTAL

SINP SPACE MONITORING DATA CENTER PORTAL SINP SPACE MONITORING DATA CENTER PORTAL Parunakian D.A. 1, Kalegaev V.V. 2, Bobrovnikov S.Yu. 2, Barinova W.O. 2 1 Moscow State University Skobeltsyn Institute of Nuclear Physics 119991, Russia, e-mail:

More information

Solar neutrinos: from their production to their detection

Solar neutrinos: from their production to their detection : from their production to their detection Universitï degli Studi di Milano and Istituto Nazionale di Fisica Nucleare E-mail: Lino.Miramonti@mi.infn.it Nuclear fusion reactions take place in the core of

More information

Structure and Properties of Atoms

Structure and Properties of Atoms PS-2.1 Compare the subatomic particles (protons, neutrons, electrons) of an atom with regard to mass, location, and charge, and explain how these particles affect the properties of an atom (including identity,

More information

Monitoring and Forecasting of Great Solar Proton Events Using the Neutron Monitor Network in Real Time

Monitoring and Forecasting of Great Solar Proton Events Using the Neutron Monitor Network in Real Time IEEE for Plasma Science, 32, 4, part, 478-488, 2004. Monitoring and Forecasting of Great Solar Proton Events Using the Neutron Monitor Network in Real Time Dorman, L.I., L.A.Pustil nik, A. Sternlieb, I.G.

More information

CHAPTER 2 Energy and Earth

CHAPTER 2 Energy and Earth CHAPTER 2 Energy and Earth This chapter is concerned with the nature of energy and how it interacts with Earth. At this stage we are looking at energy in an abstract form though relate it to how it affect

More information

Olga Botner, Uppsala. Photo: Sven Lidström. Inspirationsdagar, 2015-03-17

Olga Botner, Uppsala. Photo: Sven Lidström. Inspirationsdagar, 2015-03-17 Olga Botner, Uppsala Photo: Sven Lidström Inspirationsdagar, 2015-03-17 OUTLINE OUTLINE WHY NEUTRINO ASTRONOMY? WHAT ARE NEUTRINOS? A CUBIC KILOMETER DETECTOR EXTRATERRESTRIAL NEUTRINOS WHAT NEXT? CONCLUSIONS

More information

Proposal of a Space Radiation Environment Generator interfaced to Geant4

Proposal of a Space Radiation Environment Generator interfaced to Geant4 Proposal of a Space Radiation Environment Generator interfaced to Geant4 S. Guatelli 1, P. Nieminen 2, M. G. Pia 1 2 ESA-ESTEC, 1 INFN Genova http://www.ge.infn.it/geant4/lowe/space The experience with

More information

Chemistry. The student will be able to identify and apply basic safety procedures and identify basic equipment.

Chemistry. The student will be able to identify and apply basic safety procedures and identify basic equipment. Chemistry UNIT I: Introduction to Chemistry The student will be able to describe what chemistry is and its scope. a. Define chemistry. b. Explain that chemistry overlaps many other areas of science. The

More information

Hadro-Production Experiments: Impact on T2K and LBNE

Hadro-Production Experiments: Impact on T2K and LBNE Hadro-Production Experiments: Impact on T2K and LBNE Alysia Marino University of Colorado Boulder LBNE Scientific Workshop, Santa Fe, NM April 25-26, 24 2 Outline T2K Datasets used Flux prediction Flux

More information

Measuring Data Quality for Ongoing Improvement

Measuring Data Quality for Ongoing Improvement Measuring Data Quality for Ongoing Improvement A Data Quality Assessment Framework Laura Sebastian-Coleman ELSEVIER AMSTERDAM BOSTON HEIDELBERG LONDON NEW YORK OXFORD PARIS SAN DIEGO SAN FRANCISCO SINGAPORE

More information

Medical Applications of radiation physics. Riccardo Faccini Universita di Roma La Sapienza

Medical Applications of radiation physics. Riccardo Faccini Universita di Roma La Sapienza Medical Applications of radiation physics Riccardo Faccini Universita di Roma La Sapienza Outlook Introduction to radiation which one? how does it interact with matter? how is it generated? Diagnostics

More information