Dynamics, power budget, and optical scattering properties of interplanetary dust particles: Results of the interpretation of the HELIOS data (E 10 Z)

Details Dynamics, power budget, and optical scattering properties of interplanetary dust particles: Results of the interpretation of the HELIOS data (E 10 Z) Dynamics, power budget, and optical scattering properties of interplanetary dust particles: Results of the interpretation of the HELIOS data (E 10 Z)

Dec 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ruhr.rept.....g&link_type=abstract

Final Report, Jun. 1982 Ruhr Univ., Bochum (Germany, F.R.). Bereich Extraterrestrische Physik.

Physics

Interplanetary Dust, Light Scattering, Micrometeorites, Zodiacal Light, Energy Budgets, Helios Project, Orbits, Radiation Pressure

Scientific paper

Results of the Micrometeoroid Detector and Zodiacal Light Experiment published or directly provided by the Helios-Investigators were used in an effort of cooperative interpretation. Analysis of orbital elements derived from impacts led to low inclination orbits for larger and mainly hyperbolic trajectories of smaller micrometeorites, both with negligible percentage of retrograde cases. Radiation pressure, energy budget, and the orbits of dust particles evaporating near the Sun were investigated, taking into account the effects of size variation. It was found, that there is no appreciable production of Beta-meteoroids by evaporation, since in most cases this effect leads to total destruction faster than the particle can escape by radiation pressure. Scattering properties of irregular, fluffy and meteoritic particles were investigated by calculations, microwave and laser scattering experiments.

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