scholarly journals Orbital variation of the rotating non-spherical dust grains due to change of the solar radiation forces by shape effect

2004 ◽  
Vol 56 (6) ◽  
pp. 613-620
Author(s):  
Md. Abu Saklayen ◽  
Tadashi Mukai
Keyword(s):  
Solar Radiation ◽  
Shape Effect ◽  
Dust Grains ◽  
Radiation Forces ◽  
Solar Radiation Forces ◽  
Orbital Variation

Determination of solar radiation forces on satellite materials.

AIAA Journal ◽  
1968 ◽  
Vol 6 (8) ◽  
pp. 1569-1570 ◽  
Author(s):  
F. SHAHROKHI ◽  
H. T. CLARK
Keyword(s):  
Solar Radiation ◽  
Radiation Forces ◽  
Solar Radiation Forces

scholarly journals The Evolution of Meteoroid Streams

1996 ◽  
Vol 150 ◽  
pp. 89-99 ◽  
Author(s):  
I.P. Williams
Keyword(s):  
Solar Radiation ◽  
Dust Particles ◽  
Collective Phenomena ◽  
Meteoroid Streams ◽  
Gravitational Perturbations ◽  
Current State ◽  
Radiation Forces ◽  
The Subject ◽  
Subsequent Motion ◽  
Solar Radiation Forces

AbstractThe existence of meteoroid streams is indicated by the regular appearance of coherent meteor activity at specified times during the year. Since it is the interaction of the meteoroid with the atmosphere that is detected, the meteoroid has to be greater than about 100 micrometers in radius. Observation of these interactions gives information on individual meteoroids as well as collective phenomena. It is generally agreed that streams form through the ejection of dust particles from the surfaces of comets and asteroids at speeds considerably lower than the orbital speed. The subsequent motion of these particles is affected by gravitational perturbations from the planets and the effects of solar radiation forces. This review is intended to present an overview of the development of the subject and of our current state of knowledge.

scholarly journals Strong Solar Radiation Forces from Anomalously Reflecting Metasurfaces for Solar Sail Attitude Control

2018 ◽  
Vol 8 (1) ◽  
Author(s):  
Dylan C. Ullery ◽  
Sina Soleymani ◽  
Andrew Heaton ◽  
Juan Orphee ◽  
Les Johnson ◽  
...  
Keyword(s):  
Solar Radiation ◽  
Attitude Control ◽  
Solar Sail ◽  
Radiation Forces ◽  
Solar Radiation Forces

scholarly journals Radiation forces between dust grains in a plasma

2008 ◽  
Vol 74 (2) ◽  
pp. 145-150
Author(s):  
J. T. MENDONÇA ◽  
L. STENFLO
Keyword(s):  
Incident Radiation ◽  
Repulsive Force ◽  
Repulsive Interaction ◽  
Dust Grains ◽  
Physical Conditions ◽  
Dust Charge ◽  
Radiation Forces ◽  
Definition Of ◽  
General Physical ◽  
Dust Grain

AbstractIn this work we show that a repulsive force between nearby dust grains in a plasma can exist, due to scattering of the incident radiation. Two types of forces are discussed, one of them being formally identical to electrostatic repulsion. This leads to the definition of an effective dust charge of the dust grain, which only depends on the scattering process. Our discussion shows that such a repulsive interaction occurs in quite general physical conditions.

Interaction of relativistic dust grains with the solar radiation field

1993 ◽  
Vol 205 (2) ◽  
pp. 355-358 ◽  
Author(s):  
B. McBreen ◽  
S. Plunkett ◽  
C. J. Lambert
Keyword(s):  
Solar Radiation ◽  
Radiation Field ◽  
Dust Grains

scholarly journals Dynamics of dust grains in an electron–dust plasma induced by solar radiation under microgravity conditions

2003 ◽  
Vol 5 ◽  
pp. 102-102 ◽  
Author(s):  
V E Fortov ◽  
A P Nefedov ◽  
O S Vaulina ◽  
O F Petrov ◽  
I E Dranzhevski ◽  
...  
Keyword(s):  
Solar Radiation ◽  
Dust Grains ◽  
Microgravity Conditions ◽  
Dust Plasma

Dynamics of dust grains in a two-component dusty plasma induced by solar radiation under microgravity conditions

2003 ◽  
Vol 29 (1) ◽  
pp. 31-41
Author(s):  
A. P. Nefedov ◽  
O. S. Vaulina ◽  
O. F. Petrov ◽  
V. E. Fortov ◽  
I. E. Dranzhevskii ◽  
...  
Keyword(s):  
Solar Radiation ◽  
Dusty Plasma ◽  
Dust Grains ◽  
Two Component ◽  
Microgravity Conditions

scholarly journals 5.4 Orbital Evolution of Circum-Solar Dust Grains

1976 ◽  
Vol 31 ◽  
pp. 437-442 ◽  
Author(s):  
Ph. Lamy
Keyword(s):  
Solar Wind ◽  
Solar Radiation ◽  
Numerical Integration ◽  
Radiation Field ◽  
Equations Of Motion ◽  
Orbital Evolution ◽  
Dust Grains ◽  
Classical Approximation

AbstractThe orbital evolution of circum-solar dust grains is obtained by numerical integration of the equations of motion which includes the grains’ interactions with the solar radiation field and the solar wind. Our past solution (Lamy, 1974) is improved by avoiding a classical approximation for the Poynting-Robertson term and leads to an important revision of the orbital behaviour. Results are presented for obsidian grains whose inward spiraling is stopped by the effect of sublimation.

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