Thermal physics of asteroids - IV. Thermal infrared beaming

Thermal physics of asteroids - IV. Thermal infrared beaming

The so called beaming is an important factor when studying the thermal emission from the atmosphereless bodies of the solar system. The emission is non-Lambertian and has a tendency to be "beamed" in the solar direction. The small scale surface roughness

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:Astronomy and astrophysics (Berlin) 1998-04, Vol.332 (3), p.1123
1. Verfasser: Lagerros, JSV
Format: Artikel
Sprache:eng
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
Beschreibung
Zusammenfassung:The so called beaming is an important factor when studying the thermal emission from the atmosphereless bodies of the solar system. The emission is non-Lambertian and has a tendency to be "beamed" in the solar direction. The small scale surface roughness
ISSN:0004-6361