Orbital Evolution of Dust Particles in the Sublimation Zone near the Sun
- 22 Downloads
We have performed the calculations of the orbital evolution of dust particles from volcanic glass (p-obsidian), basalt, astrosilicate, olivine, and pyroxene in the sublimation zone near the Sun. The sublimation (evaporation) rate is determined by the temperature of dust particles depending on their radius, material, and distance to the Sun. All practically important parameters that characterize the interaction of spherical dust particles with the radiation are calculated using the Mie theory. The influence of radiation and solar wind pressure, as well as the Poynting–Robertson drag force effects on the dust dynamics, are also taken into account. According to the observations (Shestakova and Demchenko, 2016), the boundary of the dust-free zone is 7.0–7.6 solar radii for standard particles of the zodiacal cloud and 9.1–9.2 solar radii for cometary particles. The closest agreement is obtained for basalt particles and certain kinds of olivine, pyroxene, and volcanic glass.
KeywordsF-corona near-solar dust sublimation (evaporation) zodiacal cloud dust dynamics
Unable to display preview. Download preview PDF.
- Boren, C.F. and Hafmen, D.R., Absorption and Scattering of Light by Small Particles, New York: Wiley, 1983.Google Scholar
- Kelsall, T., Weiland, J.L., Franz, B.A. Reach, W.T., Arendt, R.G., Dwek, E., Freudenreich, H.T., Hauser, M.G., Moseley, S.H., and Odegard, N.P., The COBE diffuse infrared background experiment search for the cosmic infrared background. II. Model of the interplanetary dust cloud, Astrophys. J., 1998, vol. 508, pp. 44–73.CrossRefADSGoogle Scholar
- Makarov, E.A., Kharitonov, A.V., and Kazachevskaya, T.V., Potok solnechnogo izlucheniya (The Flux of Solar Radiation), Moscow: Nauka, 1991.Google Scholar
- Masafumi, M. and Munezo, S., Polarization efficiency and phase function, calculated on the basis of the Mie theory, Sci. Rep. Tohoku Univ., Ser. 8, 1985, vol. 6, no. 1, pp. 11–48.Google Scholar
- Shestakova, L.I. and Tambovtseva, L.V., Dynamics of dust grains near the Sun, Astron. Astrophys., 1995, vol. 8, pp. 59–81.Google Scholar
- Shestakova, L.I., Demchenko, B.I., Rspaev, F.K., Minasyants, G.S., and Dubovitskii, A.I., Observation of the radial velocities of dust in the F-corona during a total solar eclipse on August 1, 2008, Izv. Akad. Nauk Resp. Kazakh., Ser. Fiz.-Matem., 2009, no. 4, pp. 97–104.Google Scholar
- Veselovskii, I.S., Solar wind and heliospheric magnetic field, in Model’ kosmosa. Tom 1. Fizicheskie usloviya v kosmicheskom prostranstve (Space Model, Vol. 1: Physical Conditions in the Space), Panasyuk, M.I. and Novikov, L.S., Eds., Moscow: Universitet, 2007, pp. 314–359.Google Scholar