de
en
Schliessen
Detailsuche
Bibliotheken
Projekt
Impressum
Datenschutz
de
en
Schliessen
Impressum
Datenschutz
zum Inhalt
Detailsuche
Schnellsuche:
OK
Ergebnisliste
Titel
Titel
Inhalt
Inhalt
Seite
Seite
Im Dokument suchen
Cosmic ray anisotropy study with the AMANDA neutrino telescope / vorgelegt von Maria Gurtner. 2013
Inhalt
Introduction
Cosmic rays
Origin of cosmic rays
Cosmic ray source candidates
Acceleration
CR Propagation in the interstellar medium
The interstellar medium
Propagation models
Cosmic rays at the top of the atmosphere
Composition
Energy
Cosmic ray interactions in the atmosphere
Ionisation losses
Radiation losses
Interactions of high energy photons
Neutrino interactions
Nuclear reactions
Extensive air showers
Detection of cosmic rays
Low energy particle detection methods
High energy detection methods
Anisotropy
Anisotropies at low energies (<100GeV)
Anisotropies caused by the Sun
Anisotropies at energies >100GeV
NFJ-Model
Compton-Getting-Effect
Stochastic supernova explosions
Analysis methods
Classical analysis
East-West-Analysis
Forward-Backward-Asymmetry method
Analysis and results from other experiments
Amplitudes and phases
The Antarctic Muon And Neutrino Detector Array(AMANDA)
Detection principle
AMANDA Setup
History
Instrumentation
Deployment
Data acquisition
Analysis
Input data-set - nanoDST
Time-related information
Energy-related information
Directional information
Trigger information
Numbers
Cuts and filters
Stability considerations
Data selection
Counting rates
Local azimuth distribution
The final data-set
Corrections
Right Ascension
Phi
Results
Analysis of the full data period (2000-2005)
1-dimensional analysis
2-dimensional analysis
The single years
First order harmonic fit
Second order harmonic fit
Temporal variation of the anisotropy
Discussion and outlook
Comparison with other experiments
Past problems and future plans
Summary and conclusions
Bibliography
Acknowledgements