1 |
Secular perturbations arising from the action of Saturn upon Mars an application of the method of Arndt /Barton, Samuel Goodwin, January 1906 (has links)
Thesis (Ph. D.)--University of Pennsylvania, 1906.
|
2 |
Secular perturbations arising from the action of Saturn upon Mars an application of the method of Arndt /Barton, Samuel Goodwin, January 1906 (has links)
Thesis (Ph. D.)--University of Pennsylvania, 1906.
|
3 |
Sur les variations séculaires des éléments des planètesChoquet, Charles January 1900 (has links)
Thèse : Astronomie : Paris, Faculté des sciences : 1842. / Titre provenant de l'écran-titre.
|
4 |
Attraction et figure des planètes Théorie des perturbations des mouvements planétaires /Vasnier, Charles Felix January 1900 (has links)
Thèse : Mécanique : Paris, Faculté des sciences : 1839. Thèse : Astronomie : Paris, Faculté des sciences : 1839. / Titre provenant de l'écran-titre.
|
5 |
On the secular equation in perturbation theory.January 1975 (has links)
Milton W.Y. Wan. / Title also in Chinese. / Thesis (M.Phil.)--Chinese University of Hong Kong. / Bibliography: leaf [37]
|
6 |
Perturbation methods in geophysics and oceanographyLu, Richard Shih-Ming 16 August 1973 (has links)
The perturbation method is applied to solve two numerical
problems in the earth sciences, viz., (l)the computation of deep sea
currents in the coastal region of the northeast Pacific and (2) the
interpretation of D.C. conduction data in exploration geophysics.
The perturbation method is largely equivalent to the method of successive
approximation. The variational method is also used in the
study of the dynamics of the deep sea currents.
The deep sea currents in the coastal region of the northeast
Pacific can be calculated approximately by solving the linearized
equations for long waves in shallow basins. Both the perturbation
and the variational methods are employed to solve these equations in
the case of step shelf models approximating the shelf contours in the
region. It is concluded that the perturbation method using the
Fourier transform technique is to be preferred for the problem at
hand. The results show that the topography of the continental shelf
and the continental slope has only a minor effect on the deep sea
currents in the abyssal plain region.
In the case of the D.C. conduction exploration method, the
perturbation method is applied both to the problem of computing
the surface potential due to a given conductivity distribution and also
to the inverse problem of interpreting given field data. The first
case involves the solving of an ordinary second order differential
equation by numerical methods followed by a numerical Hankel
transformation. The inversion procedure involves, in particular,
the numerical inversion of a Laplace transformation. The application
of these methods to two- and three-layer cases is demonstrated
by working out some examples. It is shown that the perturbation
method can be applied with good results provided certain conditions
are satisfied. The main practical difficulty is encountered in the
numerical Laplace inversion which is an improperly posed problem. / Graduation date: 1974
|
7 |
The Mechanism of Interaction by Two Progressive Gravity Wave Trains in Water of Uniform DepthLin, Zhi-Zhe 14 August 2007 (has links)
For a wave system of three dimension, produced by the interactions betw een two progressive gravity wave trains on the free water surface in uniform water depth, a perturbation expansion method with chain rule has been applied to obtain the third order solution, including the resonant and non-resonant cases
In the resonant case, the growth of the induced resonant wave motion with time and its propagating time distance is displayed in the form of mathematics and figure clearly, by applying the transmission of the energy flux.
As for verifying the accuracy of this paper, the third order solution is valid when the wave system is degenerated into a progressive gravity wave train on the free water surface and the standing waves respectively. Furthermore, the experimental results of Longuet-Higgins & Smith (1966) and McGoldrick et al.(1966) are cited to compare, presenting the analytical results in this paper are great agreements.
|
8 |
Secular perturbations arising from the action of Jupiter on MarsTurner, Arthur Bertram, January 1902 (has links)
Thesis (Ph. D.)--University of Pennsylvania. / "Biographical": p. 36.
|
9 |
Tables for the computation of the Jupiter perturbations of the group of small planets whose mean daily motions are in the neighbourhood of 750"Wilson, Delonza Tate, January 1914 (has links)
Thesis (PH. D.)--University of Chicago, 1905. / Published also as Astronomiska iakttagelser och undersökningar, band 10, no. 1. Includes bibliographical references.
|
10 |
Tables for the computation of the Jupiter perturbations of the group of small planets whose mean daily motions are in the neighbourhood of 750" /Wilson, Delonza Tate, January 1914 (has links)
Thesis (PH. D.)--University of Chicago, 1905. / Published also as Astronomiska iakttagelser och undersökningar, band 10, no. 1. Includes bibliographical references. Also available on the Internet.
|
Page generated in 0.1159 seconds