Directional Characteristics of Thermal-Infrared Beaming from Atmosphereless Planetary Surfaces - A New Thermophysical Model
Ben Rozitis, Simon F. Green

TL;DR
This paper introduces a new thermophysical model for atmosphereless planetary surfaces that accurately predicts directional thermal emission by considering surface roughness, shadowing, and selfheating effects, improving surface property analysis.
Contribution
The paper presents the Advanced Thermophysical Model (ATPM), a novel approach explicitly incorporating surface roughness effects for better thermal emission predictions.
Findings
Model accurately reproduces lunar thermal emission measurements.
Beaming effect depends on illumination, viewing angles, and surface properties.
Roughness significantly influences thermal inertia and albedo.
Abstract
We present a new rough-surface thermophysical model (Advanced Thermophysical Model or ATPM) that describes the observed directional thermal emission from any atmosphereless planetary surface. It explicitly incorporates partial shadowing, scattering of sunlight, selfheating and thermal-infrared beaming (re-radiation of absorbed sunlight back towards the Sun as a result of surface roughness). The model is verified by accurately reproducing ground-based directional thermal emission measurements of the lunar surface using surface properties that are consistent with the findings of the Apollo missions and roughness characterised by an RMS slope of ~32 degrees. By considering the wide range of potential asteroid surface properties, the model implies a beaming effect that cannot be described by a simple parameter or function. It is highly dependent on the illumination and viewing angles as…
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Taxonomy
TopicsPlanetary Science and Exploration · Spacecraft and Cryogenic Technologies · Astro and Planetary Science
