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1. Spatially Resolved Absolute Spectral Reflectivity of Jupiter: 3390-8400 Angstroms. 2. The Jovian Thermal Structure from Pioneer 10 Infrared Radiometer Data. 3. Observations and Analysis of 8-14 Micron Thermal Emission of Jupiter: a Model of Thermal Structure and Cloud Properties
1975 · California Institute of Technology · doctoral · Planetary Sciences
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@misc{academicancestry_caltechthesis_caltechthesis_4308,
author = {{Academic Ancestry}},
title = {{1. Spatially Resolved Absolute Spectral Reflectivity of Jupiter: 3390-8400 Angstroms. 2. The Jovian Thermal Structure from Pioneer 10 Infrared Radiometer Data. 3. Observations and Analysis of 8-14 Micron Thermal Emission of Jupiter: a Model of Thermal Structure and Cloud Properties: record of a thesis}},
year = {2026},
url = {https://academicancestry.org/thesis/caltechthesis/caltechthesis%3A4308},
note = {read on 2026-10-22}
}apa
Academic Ancestry. (2026, October 22). 1. Spatially Resolved Absolute Spectral Reflectivity of Jupiter: 3390-8400 Angstroms. 2. The Jovian Thermal Structure from Pioneer 10 Infrared Radiometer Data. 3. Observations and Analysis of 8-14 Micron Thermal Emission of Jupiter: a Model of Thermal Structure and Cloud Properties: Record of a thesis [Read on 2026-10-22]. https://academicancestry.org/thesis/caltechthesis/caltechthesis%3A4308