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Online Theses Library of MG University
Category Title / Sections Scholar Branch of Study Year
Page Fig.5.3. Volume Emission Rate profiles of OI (1304 A) produced by e-SO2 (dashed line) and e-O (solid line) collisions using the model atmosphere of Wong and Johnson (1996). (Thesis: Model for electron degradation and production of emissions in the atmosphere of Io ) Marykutty Michael Physics 2001
Page Table 5.1. calculated column and Observed Intensities on Io in Rayleigh. (Thesis: Model for electron degradation and production of emissions in the atmosphere of Io Marykutty Michael Physics 2001
Page Fig.5.6. Volume emission rate profile of OI (1304 A) produced via e-SO2 collision, assuming all the photoelectrons are of 100 eV, using the model atmosphere of Wong and Johnson (1996). (Thesis: Model for electron degradation and production of emissions in the atmosphere of Io ) Marykutty Michael Physics 2001
Page Fig.5.8. Volume Emission Rate profiles of OI (1304 A) produced by e-O collision using the model atmosphere presented in Figure 5.7 for solar minimum and solar maximum conditions.. (Thesis: Model for electron degradation and production of emissions in the atmosphere of Io Marykutty Michael Physics 2001
Page Table 5.2. calculated column and Averaged intensities of Emissions on Io in Rayleigh. (Thesis: Model for electron degradation and production of emissions in the atmosphere of Io ) Marykutty Michael Physics 2001
Page 5.6. conclusions. (Thesis: Model for electron degradation and production of emissions in the atmosphere of Io Marykutty Michael Physics 2001
Page Fig.6.1. Galileo Energetic Particle detector (EPD) observed magnetically field aligned electron flux during closest approach of Io on 7, December 1995 at 1745: 46 UT.. (Thesis: Model for electron degradation and production of emissions in the atmosphere of Io ) Marykutty Michael Physics 2001
Page Fig.6.2. Galileo Plasma Science (PLS) instrument observed magnetically field aligned electron flux during closest approach of Io on 7, December 1995 at 1746: 43 UT.. (Thesis: Model for electron degradation and production of emissions in the atmosphere of Io Marykutty Michael Physics 2001
Page 6.2. Model calculation. (Thesis: Model for electron degradation and production of emissions in the atmosphere of Io ) Marykutty Michael Physics 2001
Page Fig. 6.3. Electron impact cross section of Na producing 5890+5896 A emission.. (Thesis: Model for electron degradation and production of emissions in the atmosphere of Io Marykutty Michael Physics 2001
Page Table 6.1. columi Production Rates in cm-2 S-1 for Monoenergetic Unit Electron Flux. (Thesis: Model for electron degradation and production of emissions in the atmosphere of Io ) Marykutty Michael Physics 2001
Page Table 6.2. Model calculated and HST-Observed Disk-Averaged Intensities of FUV Emissions on IO. (Thesis: Model for electron degradation and production of emissions in the atmosphere of Io Marykutty Michael Physics 2001
Page 6.5. correlation between Emissions of Io and Jupiter. (Thesis: Model for electron degradation and production of emissions in the atmosphere of Io ) Marykutty Michael Physics 2001
Page 6.6. conclusion. (Thesis: Model for electron degradation and production of emissions in the atmosphere of Io Marykutty Michael Physics 2001
Page cERTIFIcATE. (Thesis: Kamala Das as a painter-poet: An analysis of her paintings and poems ) Devika, M P English literature 2002



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