Table of Contents

1. Introduction
   • 1.1 Jupiter’s Atmosphere
   • 1.2 Jovian Ionosphere
   • 1.3 Jovian Magnetosphere
   • 1.4 Jovian Aurorae
   • 1.5 H₃⁺
   • 1.6 H₃⁺ in the Jovian Aurorae
   • 1.7 Temperature
   • 1.8 Column Density
   • 1.9 Total Emission
   • 1.10 Morphology
   • 1.11 Previous Studies
2. Data Reduction
   • 2.1 Spectral Fitting – using FORTRAN
   • 2.2 Data Processing – using IDL
   • 2.3 Data Display
   • 2.4 Mapping
3. Results
   • 3.1 Auroral Morphology
   • 3.2 Temperature, column density and total emission variations
4. Discussion
   • 4.1 Temperature, column density and total emission profiles
   • 4.2 Correspondence between profiles
   • 4.3 Other Profiles
   • 4.4 Southern Aurora
   • 4.5 Temperature, column density and total emission maps
5. Conclusions
   • 5.1 Improvements and future work
6. Acknowledgements
7. References
8. Appendix A: List of programs
   • Example of FORTRAN code
   • Example of IDL code