Methods of Correcting Moon's Tabular Longitude
نویسندگان
چکیده
منابع مشابه
A Comparison of Tabular PDF Inversion Methods
The most common form of tabular inversion used in computer graphics is to compute the cumulative distribution table of a pdf and then search within it to transform points, using an O(logn) binary search. Besides the standard inversion method, however, several other discrete inversion algorithms exist that can perform the same transformation in O(1) time per point. In this paper, we examine the ...
متن کاملDynamics of Distant Moons of Asteroids
solar perturbations dominate. Since the detailed mass distribution within the asteroid is relatively unimportant in We introduce a new analytic method for treating the orbital motions of objects about asteroids and planets. For an asteroid this regime, orbits about one asteroid are similar to those following a circular path around the Sun, we rewrite Jacobi’s about another as long as the eccent...
متن کاملTabular and Textual Methods for Selecting Objects from a Group
The accurate formulation of boolean expressions is a notorious problem in programming languages and database query tools. This paper studies the ways that untrained users naturally express and interpret queries, revealing some of the underlying reasons why this task is so difficult. Among the study's findings are: people interpret the word AND to mean either conjunction or disjunction depending...
متن کاملLatitude and longitude vertical disparities.
The literature on vertical disparity is complicated by the fact that several different definitions of the term "vertical disparity" are in common use, often without a clear statement about which is intended or a widespread appreciation of the properties of the different definitions. Here, we examine two definitions of retinal vertical disparity: elevation-latitude and elevation-longitude dispar...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
ژورنال
عنوان ژورنال: Monthly Notices of the Royal Astronomical Society
سال: 1904
ISSN: 0035-8711,1365-2966
DOI: 10.1093/mnras/64.7.571