Light pressure on homogeneous and inhomogeneous spheres

Details Light pressure on homogeneous and inhomogeneous spheres Light pressure on homogeneous and inhomogeneous spheres

Oct 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974hsde.rept..161s&link_type=abstract

In Arbeitsgemeinschaft für Weltraumforsch. Helios Satellite Sci. Data Evaluation p 161-169 (SEE N75-23393 14-88)

Physics

Interplanetary Dust, Orbits, Radiation Pressure, Spheres, Sunlight, Helios Project, Micrometeoroids, Particle Trajectories, Spatial Distribution

Scientific paper

The orbits of interplanetary dust particles, detected by micrometeoroid analyzers flown on space probes, were recalculated in order to determine the spatial distribution and dynamics of the interplanetary dust cloud. The gravitational attraction of the sun, as well as sunlight pressure was considered in the calculation. Results are presented in graphical form for homogeneous and inhomogeneous (mantle-core) particles.

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