Method for determining dust particle density above the ecliptic plane

Details Method for determining dust particle density above the ecliptic plane Method for determining dust particle density above the ecliptic plane

Feb 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981p%26ss...29..137b&link_type=abstract

Planetary and Space Science, vol. 29, Feb. 1981, p. 137, 138.

Physics

4

Interplanetary Dust, Particle Density (Concentration), Space Observations (From Earth), Electromagnetic Scattering, S Matrix Theory, Volterra Equations

Scientific paper

A method for determining the variation in the density of dust particles is described. Here, the altitude above the symmetry plane of interplanetary dust is arrived at through ground-based observations. In describing the method, the geometric relation between sun-particle and particle-observer distances is given. It is intended to use measurements made with a six-channel fast photopolarimeter at the Observatorio del Teide in Spain in an application of the method.

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