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Solution stabilization algorithms for the estimation of small bodies orbital parameters

Transactions of IAA RAS, issue 8, 45–46 (2002)

Keywords: Very Long Baseline Interferometry (VLBI), celestial mechanics, orbital parameters, small celestial bodies

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.

Citation

Text

BibTeX

RIS

L. E. Bykova, V. P. Titarenko. Solution stabilization algorithms for the estimation of small bodies orbital parameters // Transactions of IAA RAS. — 2002. — Issue 8. — P. 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 = {Transactions of IAA RAS},
  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/en/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  - Transactions of IAA RAS
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/en/library/paper/316/
ER  -