Zobrazeno 1 - 10
of 124
pro vyhledávání: '"Komar L"'
The I-table contains luminous intensity values over the range of angles for the luminaires used in the road lighting in accordance with technical report CIE 121:1996. A limited number of angles causes smoothing of the luminous intensity diagram omitt
Externí odkaz:
http://arxiv.org/abs/2101.00880
Orbital evolution of spherical interplanetary dust particles in the Edgeworth-Kuiper belt zone is treated for semimajor axes 30-50 AU. Besides solar gravity, also solar electromagnetic and corpuscular radiation, and, fast interstellar gas flow are im
Externí odkaz:
http://arxiv.org/abs/1009.5860
Publikováno v:
Mon. Not. R. Astron. Soc., 415, 2637-2651 (2011)
Orbital evolution of an interplanetary dust particle under action of an interstellar gas flow is investigated. Secular time derivatives of the particle orbital elements, for arbitrary orbit orientation, are presented. An important result concerns sec
Externí odkaz:
http://arxiv.org/abs/1008.2484
The paper deals with several properties of the Oort cloud of comets. Sun, Galaxy (and Jupiter) gravitationally act on the comets. New physical model of galactic tide is considered. The main results can be summarized as follows: 1. Mass of the Oort cl
Externí odkaz:
http://arxiv.org/abs/1005.3414
Equation of motion for the galactic tide is treated for the case of a comet situated in the Oort cloud of comets. We take into account that galactic potential and mass density depend on a distance from the galactic equator and on a distance from the
Externí odkaz:
http://arxiv.org/abs/0912.3449
Equation of motion for a comet in the Oort cloud is numerically solved. Orbital evolution of the comet under the action of the gravity of the Sun and the Galaxy is presented for various initial conditions. Oscillations of the Sun with respect to the
Externí odkaz:
http://arxiv.org/abs/0912.3447
Action of solar wind on arbitrarily shaped interplanetary dust particle is investigated. The final relativistically covariant equation of motion of the particle contains both orbital evolution and change of particle's mass. Non-radial solar wind velo
Externí odkaz:
http://arxiv.org/abs/0904.2673
Physics of the Poynting-Robertson (P-R) effect is discussed and compared with the statements published in the past thirty years. Relativistically covariant formulation reveals the essence of the P-R effect and points out to nonphysical explanations i
Externí odkaz:
http://arxiv.org/abs/0904.0368
Publikováno v:
Celest. Mech. Dyn. Astron., 103, 343-364 (2009)
Effect of stellar electromagnetic radiation on motion of spherical dust particle in mean-motion orbital resonances with a planet is investigated. Planar circular restricted three-body problem with the Poynting-Robertson (P-R) effect yields monotonous
Externí odkaz:
http://arxiv.org/abs/0807.1425
Publikováno v:
In Solar Energy 15 July 2018 169:264-269
