Solution stabilization algorithms for the estimation of small bodies orbital parameters
Труды ИПА РАН, вып. 8, 45–46 (2002)
Ключевые слова: Very Long Baseline Interferometry (VLBI), celestial mechanics, orbital parameters, small celestial bodies
Текст статьиАннотация
Sometimes there is not enough information for the correct improvement of the orbits of the Solar system small bodies. As a rule it is caused by lack of observations or by too short arc of orbit covered by observations. Therefore one can obtain only a set X of acceptable solutions satisfying the given observations with the adequate accuracy. In this work some stabilization algorithms for solution of such problems have been considered. Algorithms have been constructed on the basis of a linear least squares method using additional a priori information about the solution. This additional information is given as restrictions on the solution or its components.
Цитирование
L. E. Bykova, V. P. Titarenko. Solution stabilization algorithms for the estimation of small bodies orbital parameters // Труды ИПА РАН. — 2002. — Вып. 8. — С. 45–46.
@article{bykova2002,
abstract = {Sometimes there is not enough information for the correct improvement of the orbits of the Solar system small bodies. As a rule it is caused by lack of observations or by too short arc of orbit covered by observations. Therefore one can obtain only a set X of acceptable solutions satisfying the given observations with the adequate accuracy.
In this work some stabilization algorithms for solution of such problems have been considered. Algorithms have been constructed on the basis of a linear least squares method using additional a priori information about the solution. This additional information is given as restrictions on the solution or its components.},
author = {L.~E. Bykova and V.~P. Titarenko},
issue = {8},
journal = {Труды ИПА РАН},
keyword = {Very Long Baseline Interferometry (VLBI), celestial mechanics, orbital parameters, small celestial bodies},
pages = {45--46},
title = {Solution stabilization algorithms for the estimation of small bodies orbital parameters},
url = {http://iaaras.ru/library/paper/316/},
year = {2002}
}
TY - JOUR
TI - Solution stabilization algorithms for the estimation of small bodies orbital parameters
AU - Bykova, L. E.
AU - Titarenko, V. P.
PY - 2002
T2 - Труды ИПА РАН
IS - 8
SP - 45
AB - Sometimes there is not enough information for the correct improvement
of the orbits of the Solar system small bodies. As a rule it is
caused by lack of observations or by too short arc of orbit covered
by observations. Therefore one can obtain only a set X of acceptable
solutions satisfying the given observations with the adequate
accuracy. In this work some stabilization algorithms for solution of
such problems have been considered. Algorithms have been constructed
on the basis of a linear least squares method using additional a
priori information about the solution. This additional information is
given as restrictions on the solution or its components.
UR - http://iaaras.ru/library/paper/316/
ER -