Analytical research on the possibility of long orbital existence of submicron particles in the Earth’s plasmasphere by the methods of the KAM theory

2017 ◽  
Vol 83 (3) ◽  
Author(s):  
A. B. Yakovlev ◽  
E. K. Kolesnikov ◽  
S. V. Chernov

Particles which move in the magnetosphere’s plasma gain an electric charge which depends on the density and temperature of the plasma and the sunlight stream. If motion is slow enough, it is possible to consider that the micro-particle’s electric charge is in quasi-equilibrium. For certain conditions, the Hamilton function can be written for the problem with a variable electric charge and, hence, the methods of the analysis of systems of Hamilton equations can be applied for research of such micro-particle motion. Although these conditions are strong enough, they correspond to the statement of many real problems. The spatial distribution of plasma in the Earth’s plasmasphere is described by a model of a two-component plasma. In the present paper, the capability of propagation of results which were received earlier for a case of the motion of a quasi-equilibrium electric charge in the Earth plasmasphere has been shown. The received result shows that there is an opportunity for long orbital holding (not less than one month) of micro-particles of space dust in the Earth’s plasmasphere.

2018 ◽  
Vol 84 (6) ◽  
Author(s):  
A. B. Yakovlev ◽  
E. K. Kolesnikov ◽  
S. V. Chernov

The influence of the corotational electric field on the possibility of long holding of micro-particles with radii of the order of some hundredths of micrometers and quasi-equilibrium charge moving along weakly elliptic orbits in the plasmasphere of the Earth is considered by analytical and numerical methods. It is shown that, unlike the magnetic field, the corotational electric field causes a slow change in the shape of the orbit.


Nature ◽  
1933 ◽  
Vol 132 (3332) ◽  
pp. 407-407 ◽  
Author(s):  
W. KOLHÖRSTER

2005 ◽  
Vol 53 (9) ◽  
pp. 903-923 ◽  
Author(s):  
A.J. Tuzzolino ◽  
T.E. Economou ◽  
R.B. McKibben ◽  
J.A. Simpson ◽  
S. BenZvi ◽  
...  
Keyword(s):  

2001 ◽  
Vol 49 (7) ◽  
pp. 689-703 ◽  
Author(s):  
A.J Tuzzolino ◽  
R.B McKibben ◽  
J.A Simpson ◽  
S BenZvi ◽  
H.D Voss ◽  
...  
Keyword(s):  

2001 ◽  
Vol 49 (7) ◽  
pp. 705-729 ◽  
Author(s):  
A.J. Tuzzolino ◽  
R.B. McKibben ◽  
J.A. Simpson ◽  
S. BenZvi ◽  
H.D. Voss ◽  
...  
Keyword(s):  

1980 ◽  
Vol 90 ◽  
pp. 421-424
Author(s):  
J. D. Chamberlain ◽  
W. M. Alexander ◽  
J. D. Corbin

Flux measurements of picogram dust particles near the lunar surface and in selenocentric and cis-lunar space made by Lunar Explorer 35, HEOS, and ALSOP dust experiments all indicate, to varying degrees, ejecta from lunar impacts of interplanetary dust particles. The orbits of these submicron particles in the earth-moon system are significantly altered by radiation pressure. Recent orbit calculations show that, in favorable lunar phases, as many as 80% of the ejecta may enter the magnetosphere and 20% may enter the earth's atmosphere. The results of this analysis are presented, and their implications are discussed.


2019 ◽  
Vol 60 (3) ◽  
pp. 3.38-3.42 ◽  
Author(s):  
Penny J Wozniakiewicz ◽  
Mark J Burchell
Keyword(s):  

1993 ◽  
Vol 139 ◽  
pp. 284-284
Author(s):  
G. Wuchterl

AbstractNonlinear oscillations of proto-giant-planets have been found in recent numerical calculations relevant to planetary formation. Pulsations are excited in two phases of the protoplanetary evolution, (a) In an ‘instability strip’ at core masses of typically 0.2M⊙ (M⊕ is the earth mass). Perturbations grow into the nonlinear domain and saturate into perodic variations with relative luminosity-amplitudes of 0.2m (b) At the so called critical mass (typically at Mcore ≈ 15M⊕). There the pulsations drive a strong mass loss. A large portion of the envelope is ejected. Then the mass loss fades and the envelope settles into a new quasi-equilibrium. This remnant — a post nucleated instability protoplanet — has a compact envelope and is in core and envelope mass similar to Uranus and Neptune.


Author(s):  
L.V. Grunskaya ◽  
◽  
V.V. Isakevich ◽  
D.V. Isakevich ◽  
◽  
...  

A model is proposed which explains the observed effect of gravity-wave influence of relativistic binaries to the Earth’s electric field vertical projection in the near-ground atmosphere layer. The considered mechanism is a perturbation of the Earth’s orbit by the gravity waves which leads to a small displacement between the Earth and the Earth’s atmosphere free electric charge. The proposed model give amplitude estimations of Ez components spectrally localized at the relativistic binaries gravity waves’ frequencies which do not contradict to the observations.


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