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Physical properties of interplanetary dust: laboratory and numerical simulations
2010Laboratory light scattering measurements with the PROGRA2 experiment, in A300-CNES and ESA dedicated microgravity flights or in ground based configurations, offer an alternative to models for exploring the scattering properties of particles with structures too complex to be easily handled by computer simulations [1,2].
Hadamcik, Edith +9 more
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Planetary and Space Science, 1994
The suggestion that significant quantities of interplanetary dust are produced by both main-belt asteroids and comets is based on the Infrared Astronomical Satellite (IRAS) detection of dust trails or bands associated with these objects. Gravitational focusing strongly biases all near-Earth collections of interplanetary dust in favor of particles with ...
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The suggestion that significant quantities of interplanetary dust are produced by both main-belt asteroids and comets is based on the Infrared Astronomical Satellite (IRAS) detection of dust trails or bands associated with these objects. Gravitational focusing strongly biases all near-Earth collections of interplanetary dust in favor of particles with ...
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Interplanetary Dust - Its Physical Nature and Entry into the Atmosphere of Terrestrial Planets
1981Studies of extraterrestrial particles collected in the stratosphere and from the sea floor indicate that the majority of interplanetary dust is a black, fine grained material similar to carbonaceous chondrites but different from known meteorites in mineralogy and structure.
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PHYSICS OF INTERPLANETARY PLASMA AND LABORATORY EXPERIMENTS
Soviet Physics Uspekhi, 1970I M Podgornyĭ, Renad Z Sagdeev
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2002
Information about the physical properties of cosmic dust is mainly provided by remote observations. Results about phase angle and wavelength dependence of the polarization of dust in comets are updated, and the phase angle dependence of the (positive) rate of increase of the wavelength dependence is estimated in the visible domain.
Levasseur-Regourd, Anny Chantal +2 more
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Information about the physical properties of cosmic dust is mainly provided by remote observations. Results about phase angle and wavelength dependence of the polarization of dust in comets are updated, and the phase angle dependence of the (positive) rate of increase of the wavelength dependence is estimated in the visible domain.
Levasseur-Regourd, Anny Chantal +2 more
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What Solar–Terrestrial Link Researchers Should Know about Interplanetary Drivers
Universe, 2021Yuri I Yermolaev
exaly
Physics of interplanetary plasma and laboratory experiments
Uspekhi Fizicheskih Nauk, 1969I.M. Podgornyi, Roal'd Z. Sagdeev
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2007
Physical properties of the interplanetary dust such as the local polarization and temperature, together with their heliocentric variations, may be derived from scattered and emitted light observations. With a realistic size distribution typical of the interplanetary dust, a very good fit of the polarization phase curve near 1 AU is obtained for a ...
Lasue, Jérémie +1 more
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Physical properties of the interplanetary dust such as the local polarization and temperature, together with their heliocentric variations, may be derived from scattered and emitted light observations. With a realistic size distribution typical of the interplanetary dust, a very good fit of the polarization phase curve near 1 AU is obtained for a ...
Lasue, Jérémie +1 more
openaire +1 more source