Results 241 to 250 of about 932,549 (275)

Physical properties of interplanetary dust: laboratory and numerical simulations

2010
Laboratory 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, Lasue, Jérémie, Levasseur-Regourd, Anny Chantal, Renard, Jean-Baptiste, Buch, Arnaud, Carrasco, Nathalie, Cottin, Hervé, Fray, Nicolas, Yong Guan, Yuan, Szopa, Cyril   +9 more
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Propagation characteristics of coronal mass ejections (CMEs) in the corona and interplanetary space

Reviews of Modern Plasma Physics, 2022
Fang Shen, C. Shen, Mengjiao Xu, Yousheng Liu, Xueshang Feng, Yuming Wang   +5 more
semanticscholar   +1 more source

Interplanetary dust particles collected from the stratosphere: physical, chemical, and mineralogical properties and implications for their sources

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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Interplanetary Dust - Its Physical Nature and Entry into the Atmosphere of Terrestrial Planets

1981
Studies 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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PHYSICAL PROPERTIES OF METEORITES AND INTERPLANETARY DUST PARTICLES: CLUES TO THE PROPERTIES OF THE METEORS AND THEIR PARENT BODIES

Earth, Moon, and Planets, 2004
Meteorites, generally 1 cm or larger in size that are believed to sample asteroids, and interplanetary dust particles (IDPs), generally 5–50 μm in size that are believed to sample both asteroids and comets, span the size range of the meteors. Thus, the physical properties of the meteorites and the IDPs are likely to constrain the properties of the ...
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Band-splitting of Coronal and Interplanetary Type II Bursts: III. Physical conditions in the upper corona and interplanetary space

Astronomy & astrophysics, 2004
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Interplanetary Physics*

2022
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PHYSICS OF INTERPLANETARY PLASMA AND LABORATORY EXPERIMENTS

Soviet Physics Uspekhi, 1970
I M Podgornyĭ, Renad Z Sagdeev
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Emerging exciton physics in transition metal dichalcogenide heterobilayers

Nature Reviews Materials, 2022
Emma C Regan, Yongxin Zeng, Long Zhang
exaly  

Interplanetary Physics Research in China:2006—2008

, 2008
Wang Chi, Feng Xueshang
semanticscholar   +1 more source