| 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 |