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Inversion of shape statistics for small solar system bodies
Uppsala University.
Uppsala University.
1998 (English)In: ASTRONOMY AND ASTROPHYSICS, ISSN 0004-6361, Vol. 333, no 2, 753-761 p.Article in journal (Other scientific) Published
Abstract [en]

The irregular shapes of small solar system bodies are modelled by lognormal statistics, i.e., assuming that the shapes are realisations of the so-called Gaussian random sphere. The Gaussian sphere is fully described by the mean radius and the covariance f

Place, publisher, year, edition, pages
SPRINGER VERLAG , 1998. Vol. 333, no 2, 753-761 p.
Keyword [en]
minor planets; asteroids; methods : analytical methods : statistical; GAUSSIAN RANDOM PARTICLES; LIGHT-SCATTERING; TOPOGRAPHY; IMAGES
URN: urn:nbn:se:uu:diva-85313OAI: oai:DiVA.org:uu-85313DiVA: diva2:113221
Addresses: Muinonen K, Astron Observ, Box 515, S-75120 Uppsala, Sweden. Astron Observ, S-75120 Uppsala, Sweden. Univ Helsinki Observ, FIN-00014 Helsinki, Finland.Available from: 2008-10-17 Created: 2008-10-17 Last updated: 2011-01-14

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