Standard

Dust Torus Produced by Particles Ejected in the Apsidal Points. / Orlov, S.A.; Kholshevnikov, K.V.

в: Solar System Research, Том 46, № 3, 2012, стр. 208-219.

Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование

Harvard

Orlov, SA & Kholshevnikov, KV 2012, 'Dust Torus Produced by Particles Ejected in the Apsidal Points', Solar System Research, Том. 46, № 3, стр. 208-219. <http://link.springer.com/article/10.1134%2FS0038094612020098>

APA

Orlov, S. A., & Kholshevnikov, K. V. (2012). Dust Torus Produced by Particles Ejected in the Apsidal Points. Solar System Research, 46(3), 208-219. http://link.springer.com/article/10.1134%2FS0038094612020098

Vancouver

Orlov SA, Kholshevnikov KV. Dust Torus Produced by Particles Ejected in the Apsidal Points. Solar System Research. 2012;46(3):208-219.

Author

Orlov, S.A. ; Kholshevnikov, K.V. / Dust Torus Produced by Particles Ejected in the Apsidal Points. в: Solar System Research. 2012 ; Том 46, № 3. стр. 208-219.

BibTeX

@article{44380c1978f64341a21591c9e2c1f4b6,
title = "Dust Torus Produced by Particles Ejected in the Apsidal Points",
abstract = "Dust complexes form one of the Solar System components. There are many ways of their forming: ejection of matter from comets and satellites due to volcanic (geyser) eruptions and meteorites bombardement, explosions and collisions of artificial satellites, etc. Many works are dedicated to describe the distribution of matter in such complexes. In the present paper we find the shape of a typical complex under reasonable assumptions (the main one is the smallness of perturbations) using purely analytical methods.",
keywords = "dust complex, family of Keplerian ellipses, filled up by trajectories domain, enveloping surface",
author = "S.A. Orlov and K.V. Kholshevnikov",
year = "2012",
language = "English",
volume = "46",
pages = "208--219",
journal = "Solar System Research",
issn = "0038-0946",
publisher = "МАИК {"}Наука/Интерпериодика{"}",
number = "3",

}

RIS

TY - JOUR

T1 - Dust Torus Produced by Particles Ejected in the Apsidal Points

AU - Orlov, S.A.

AU - Kholshevnikov, K.V.

PY - 2012

Y1 - 2012

N2 - Dust complexes form one of the Solar System components. There are many ways of their forming: ejection of matter from comets and satellites due to volcanic (geyser) eruptions and meteorites bombardement, explosions and collisions of artificial satellites, etc. Many works are dedicated to describe the distribution of matter in such complexes. In the present paper we find the shape of a typical complex under reasonable assumptions (the main one is the smallness of perturbations) using purely analytical methods.

AB - Dust complexes form one of the Solar System components. There are many ways of their forming: ejection of matter from comets and satellites due to volcanic (geyser) eruptions and meteorites bombardement, explosions and collisions of artificial satellites, etc. Many works are dedicated to describe the distribution of matter in such complexes. In the present paper we find the shape of a typical complex under reasonable assumptions (the main one is the smallness of perturbations) using purely analytical methods.

KW - dust complex

KW - family of Keplerian ellipses

KW - filled up by trajectories domain

KW - enveloping surface

M3 - Article

VL - 46

SP - 208

EP - 219

JO - Solar System Research

JF - Solar System Research

SN - 0038-0946

IS - 3

ER -

ID: 5382971