Astronomy and Astrophysics – Astronomy
Scientific paper
Mar 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992cemda..54..241k&link_type=abstract
Celestial Mechanics and Dynamical Astronomy (ISSN 0923-2958), vol. 54, no. 1-3, p. 241-244.
Astronomy and Astrophysics
Astronomy
1
Charged Particles, Interplanetary Dust, Plasma-Particle Interactions, Solar Magnetic Field, Solar Wind, Gravitational Effects, Particle Motion, Poynting-Robertson Effect, Radiation Pressure
Scientific paper
An analysis is presented of the charging processes for the dust particles in the circumsolar dust band at 4 solar radii, as well as the effects of the interactions between these charged particles and the magnetized ambient solar wind plasma on the evolution of their orbits. It is concluded that due to the higher values of the potential on the dust particle and the ambient solar wind magnetic field, the Lorentz force affects a much wider size range of particles in the near-solar regions. Since the magnitude of the Lorentz force is much higher and its characteristic time to affect the particle's orbit is much lower than those for the Poynting-Robertson drag force, the Lorentz force is a major perturbing force for dust particles in the circumsolar dust band at 4 solar radii.
Isobe Syuzo
Kumar Ajith S.
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