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 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.

scholarly journals Design of a celestial vault image capture device for its application in the solar radiation field

2013 ◽  
Vol 10 (3) ◽  
pp. 258-261
Author(s):  
E.P. Varo ◽  
R. Posadillo ◽  
M. Varo-Martínez ◽  
R. López-Luque
Keyword(s):  
Solar Radiation ◽  
Radiation Field ◽  
Image Capture

scholarly journals Trajectories of Sublimating Interplanetary Dust Grains

1980 ◽  
Vol 90 ◽  
pp. 319-320
Author(s):  
G. H. Schwehm
Keyword(s):  
Grain Size ◽  
Temperature Distribution ◽  
Radiation Field ◽  
Heliocentric Distance ◽  
Equation Of Motion ◽  
Interplanetary Dust ◽  
Dust Particles ◽  
The Sun ◽  
Dust Grains ◽  
Interplanetary Dust Particles

The equation of motion for interplanetary dust particles close to the Sun has been solved numerically taking into consideration the interaction with the radiation field of the Sun and the temperature distribution as a function of grain size and heliocentric distance for different materials.

The capture of small absorbing particles by the solar radiation field

1962 ◽  
Vol 9 (11) ◽  
pp. 801-809 ◽  
Author(s):  
G.T. Best ◽  
T.N.L. Patterson
Keyword(s):  
Solar Radiation ◽  
Radiation Field

The Definition of the Optimal Energy-Efficient form of the Building

2018 ◽  
Vol 7 (3.2) ◽  
pp. 667 ◽  
Author(s):  
Oleg Sergeychuk ◽  
Viacheslav Martynov ◽  
Dmytro Usenko
Keyword(s):  
Solar Radiation ◽  
Thermal Radiation ◽  
Point Source ◽  
Radiation Field ◽  
Thermal Energy ◽  
Energy Efficient ◽  
The Body ◽  
Geometrical Form ◽  
Point Source Of Heat ◽  
Definition Of

We consider the problem of finding a geometrical form of a body in a thermal radiation field, for which the thermal balance between the body and the surrounding air is minimal. The case of a point source of heat is investigated. To consider an analogous problem for buildings, one must know the value of incoming thermal energy to a unit square in relation to its orientation. We develop an application package in MATLAB that represents this relation in table form and takes into consideration the direct, diffuse, ground-reflected solar radiation and the thermal radiation of atmosphere.  

Influence of 3D cloud effects on spatial-angular characteristics of the reflected solar radiation field

2017 ◽  
Vol 30 (1) ◽  
pp. 103-110 ◽  
Author(s):  
T. B. Zhuravleva ◽  
I. M. Nasrtdinov ◽  
T. V. Russkova
Keyword(s):  
Solar Radiation ◽  
Radiation Field

scholarly journals On the Space–Time Scales of the Surface Solar Radiation Field

1998 ◽  
Vol 11 (1) ◽  
pp. 88-96 ◽  
Author(s):  
T. P. Barnett ◽  
J. Ritchie ◽  
J. Foat ◽  
G. Stokes
Keyword(s):  
Solar Radiation ◽  
Radiation Field ◽  
Time Scales ◽  
Space Time ◽  
Surface Solar Radiation
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