ar X iv : a st ro - p h / 02 05 50 9 v 1 2 9 M ay 2 00 2 1 Charging Processes for Dust Particles in Saturn ’ s Magnetosphere
نویسندگان
چکیده
We investigated the electrostatic charging behavior of submillimeter-sized dust particles located in Saturn's magnetosphere. The charging effects we considered included electron/ion capture from the magnetospheric plasma, electron/ion capture from the solar-wind plasma, the photoelectric effect from solar radiation, and secondary electron emission from energetic electrons. In our results, we show charging times and equilibrium potentials for particles located in different regions of Saturn's magnetosphere. We find that charging in Saturn's magnetosphere is not particularly sensitive to the dust particle's material properties. The equipotential ranges from The charging time for one micron-sized particles is a few minutes, and for 0.01 micron-sized particles the charging time is 6 hours (or more). The latter is a significant fraction of Saturn's rotation period. The dynamics of dust, submillimeter-sized dust grains, is a fascinating area of study of our solar system's dynamical evolution. Small particles, especially charged particles, respond to other forces than gravitational, in particular, electromagnetic forces. The dust particle's properties and dynamics fall into a complex regime between nuclear physics and electromagnetic physics and gravitational physics. In order to calculate charges on a dust particle around a planet, we must characterize: 2 • The planet's magnetospheric features: its magnetic field and plasma, • The physical processes onto the dust particle that generate currents, and • The material properties of the dust particle. In this paper, we make reference to results of charging of dust particles in Earth's magnetosphere ([2],[3]). Earth is an interesting charging environment for dust particles , in part, because the dynamic magnetospheric plasma shows steep changes in the electron and ion energies and densities, therefore, the electron energy can be quite high (e.g. a few thousand eV). Table 1 lists some basic parameters comparing Saturn's and Earth's magnetosphere.
منابع مشابه
ar X iv : a st ro - p h / 02 06 05 9 v 1 4 J un 2 00 2 1 IO REVEALED IN THE JOVIAN DUST STREAMS
The Jovian dust streams are high-speed bursts of submicron-sized particles traveling in the same direction from a source in the Jovian system. Since their discovery in 1992, they have been observed by three spacecraft: Ulysses, Galileo and Cassini. The source of the Jovian dust streams is dust from Io’s volcanoes. The charged and traveling dust stream particles have particular signatures in fre...
متن کاملar X iv : a st ro - p h / 05 02 36 3 v 2 1 9 M ay 2 00 5 Microlensing optical depth toward the Galactic Bulge using bright sources from OGLE - II
We present a measurement of the microlensing optical depth toward the Galactic Bulge based on 4 years of OGLE-II survey. We consider only bright sources in the extended Red Clump Giant (RCG) region of the Color-Magnitude
متن کاملar X iv : a st ro - p h / 05 05 55 5 v 1 2 7 M ay 2 00 5 Pulsars as Tools for Fundamental Physics & Astrophysics
X iv :a st ro -p h/ 05 05 55 5v 1 2 7 M ay 2 00 5 Pulsars as Tools for Fundamental Physics & Astrophysics J. M. Cordes, M. Kramer, T. J. W. Lazio , B. W. Stappers, D. C. Backer, S. Johnston Department of Astronomy and NAIC, Cornell University, Ithaca, NY USA University of Manchester, Jodrell Bank Observatory, Jodrell Bank, UK Naval Research Laboratory, Remote Sensing Division, Washington, DC US...
متن کاملar X iv : a st ro - p h / 02 05 50 4 v 1 2 9 M ay 2 00 2 Cosmology with Varying Constants
The idea of possible time or space variations of the ‘fundamental’ constants of nature, although not new, is only now beginning to be actively considered by large numbers of researchers in the particle physics, cosmology and astrophysics communities. This revival is mostly due to the claims of possible detection of such variations, in various different contexts and by several groups. Here, I pr...
متن کاملar X iv : a st ro - p h / 92 05 00 5 v 1 9 M ay 1 99 2 UCSBTH – 92 – 05 April 1992 CHAOTIC DARK MATTER
A very weakly coupled scalar field with mass m and initial vacuum expectation value V will provide enough mass to close the universe provided V ≃ (3 × 10 8 GeV)(100 GeV/m) 1/4. We discuss possible models in which such a field could arise. (a) Electronic address (internet): [email protected].
متن کامل