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Table of contents
1 The Search for Ultra High Energy Cosmic Rays
1.1 A brief history of Cosmic Ray research
1.2 Cosmic ray energy spectrum
1.3 Extensive Air Showers
1.4 UHECR detection Methods
2 Towards Space Detectors of UHECR: The JEM-EUSO Framework
2.1 The JEM-EUSO Mission
2.2 JEM-EUSO Pathfinders
2.3 Future projects in the JEM-EUSO framework
2.4 Projects integrated in the JEM-EUSO Framework
3 The Optics performance of the JEM-EUSO balloon pathfinders
3.1 Introduction
3.2 History and principle of Fresnel Lenses
3.3 Description of the EUSO-Balloon and EUSO-SPB1 optics
3.4 EUSO-Balloon optics characterization
3.5 EUSO-SPB1 Optics characterization
3.6 Post Characterization conclusions
3.7 Observation of diffraction effects by the Fresnel lenses
3.8 Scattering of light by small-scale structure of the lens surface
3.9 Fresnel lens diffusion experiment
3.10 Model of the EUSO-Balloon optics
3.11 Improvement of the Fresnel optics
4 The EUSO-SPB1 campaign
4.1 Introduction
4.2 EUSO-SPB1 optics characterization and end to end tests
4.3 Wanaka balloon launch campaign
5 Data analysis of EUSO-SPB1
5.1 Introduction
5.2 Instrument flight performance
5.3 Data Structure
5.4 Analysis method of the EUSO-SPB1 data
5.5 Analysis results of the event database
6 Conclusion (English)
6.1 The optics performance of the balloon pathfinders
6.2 Classification of the triggered events in EUSO-SPB1
7 Conclusion (Français)
7.1 La performance optique des démonstrateurs ballon
7.2 Classification des événements enregistrés dans EUSO-SPB1
Bibliography
