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Thermal physics of asteroids - IV. Thermal infrared beaming
Uppsala University.
1998 (English)In: ASTRONOMY AND ASTROPHYSICS, ISSN 0004-6361, Vol. 332, no 3, 1123-1132 p.Article in journal (Other scientific) Published
Abstract [en]

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

Place, publisher, year, edition, pages
SPRINGER VERLAG , 1998. Vol. 332, no 3, 1123-1132 p.
Keyword [en]
minor planets; asteroids; radiation mechanisms : thermal; infrared : solar system; Moon; planets and satellites : individual : 3 Juno; PLANETARY REGOLITHS; EMISSION-SPECTRA; ENERGY-TRANSFER; ROUGH-SURFACE; MODEL
Identifiers
URN: urn:nbn:se:uu:diva-85316OAI: oai:DiVA.org:uu-85316DiVA: diva2:113224
Note
Addresses: Lagerros JSV, Astron Observ, Box 515, S-75120 Uppsala, Sweden. Astron Observ, S-75120 Uppsala, Sweden.Available from: 2008-10-17 Created: 2008-10-17 Last updated: 2011-01-14

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