Spatially resolved absolute spectral reflectivity of Jupiter : 3390-8400 angstroms. The Jovian thermal structure from Pioneer 10 infrared radiometer data. Observations and analysis of 8-14 micron thermal emission of Jupiter : a model of thermal structure and cloud properties
NOTE: Text or symbols not renderable in plain ASCII are indicated by [...]. Abstract is included in .pdf document. Part 1 presents determinations of the absolute reflectivities of several visually distinct regions of Jupiter between 3390 and 8400Å, at 10Å resolution, from observations made on t...
Similar Items
-
AN ANALYSIS OF THE VOYAGER IMAGES OF JOVIAN LIGHTNING (JUPITER).
by: WILLIAMS, MARK ANDREW.
Published: (1986) -
Angular Dependence and Spatial Distribution of Jupiter's Centimeter‐Wave Thermal Emission From Juno's Microwave Radiometer
by: Fabiano Oyafuso, et al.
Published: (2020-11-01) -
Thermal tides on a hot Jupiter
by: Hsieh H.-F., et al.
Published: (2011-07-01) -
On the Inference of Thermal Inversions in Hot Jupiter Atmospheres
by: Madhusudhan, Nikku, et al.
Published: (2012) -
The Interaction of Thermal Tides with the Equatorial Winds on Hot Jupiters
by: Shang-Min Tsai, et al.
Published: (2011)