椭球体
地图投影
方位角
等距
几何学
球体
大地测量学
投影(关系代数)
地质学
数学
物理
计算机科学
算法
计算机视觉
生物化学
化学
体外
作者
Maxim V. Nyrtsov,Maria E. Fleis,Michael M. Borisov,Philip J. Stooke
标识
DOI:10.1080/00087041.2015.1119471
摘要
Many small solar system bodies such as asteroids or small satellites have irregular shapes, often approximated by the reference surface of a triaxial ellipsoid. Map projections for the triaxial ellipsoid are needed to present the incoming data in the form of maps. In this paper the formulae of equal-area cylindrical and azimuthal projections of the triaxial ellipsoid were derived and practically implemented for the first time using as an example the asteroid 253 Mathilde. This paper is the final in a series of papers devoted to all main classes of projections of the triaxial ellipsoid. Before this, the authors obtained equidistant along meridians projection and Jacobi conformal projection for the triaxial ellipsoid.
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