Standard

Dynamics of levitating microparticles of lunar regolith. / Yakovlev, A. B.

в: Solar System Research, Том 32, № 4, 15.08.1998, стр. 352-353.

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

Harvard

Yakovlev, AB 1998, 'Dynamics of levitating microparticles of lunar regolith', Solar System Research, Том. 32, № 4, стр. 352-353.

APA

Yakovlev, A. B. (1998). Dynamics of levitating microparticles of lunar regolith. Solar System Research, 32(4), 352-353.

Vancouver

Yakovlev AB. Dynamics of levitating microparticles of lunar regolith. Solar System Research. 1998 Авг. 15;32(4):352-353.

Author

Yakovlev, A. B. / Dynamics of levitating microparticles of lunar regolith. в: Solar System Research. 1998 ; Том 32, № 4. стр. 352-353.

BibTeX

@article{904b38b95ebf409cb3d24ac0bd970757,
title = "Dynamics of levitating microparticles of lunar regolith",
abstract = "A system of equations of motion is obtained for microparticles levitating near the lunar surface. An analysis of the system is carried out. The dust particles are shown to perform oscillatory motions with a period and an amplitude only weakly depending on the incidence angle of solar rays.",
author = "Yakovlev, {A. B.}",
year = "1998",
month = aug,
day = "15",
language = "English",
volume = "32",
pages = "352--353",
journal = "Solar System Research",
issn = "0038-0946",
publisher = "МАИК {"}Наука/Интерпериодика{"}",
number = "4",

}

RIS

TY - JOUR

T1 - Dynamics of levitating microparticles of lunar regolith

AU - Yakovlev, A. B.

PY - 1998/8/15

Y1 - 1998/8/15

N2 - A system of equations of motion is obtained for microparticles levitating near the lunar surface. An analysis of the system is carried out. The dust particles are shown to perform oscillatory motions with a period and an amplitude only weakly depending on the incidence angle of solar rays.

AB - A system of equations of motion is obtained for microparticles levitating near the lunar surface. An analysis of the system is carried out. The dust particles are shown to perform oscillatory motions with a period and an amplitude only weakly depending on the incidence angle of solar rays.

UR - http://www.scopus.com/inward/record.url?scp=27644598544&partnerID=8YFLogxK

M3 - Article

AN - SCOPUS:27644598544

VL - 32

SP - 352

EP - 353

JO - Solar System Research

JF - Solar System Research

SN - 0038-0946

IS - 4

ER -

ID: 15542293