Results 61 to 70 of about 84 (83)
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Solar System Research, 2002
We consider the mechanisms of the formation of dust ejected from craters produced by large-meteoroid impacts on the Martian surface, as well as the mechanisms of the elevation of dust that already existed on the surface, due to impulsed aeolian processes.
I. B. Kosarev +4 more
openaire +1 more source
We consider the mechanisms of the formation of dust ejected from craters produced by large-meteoroid impacts on the Martian surface, as well as the mechanisms of the elevation of dust that already existed on the surface, due to impulsed aeolian processes.
I. B. Kosarev +4 more
openaire +1 more source
The meteoroid influx and the maintenance of the solar system dust cloud
Planetary and Space Science, 1972Abstract The total mass influx onto the Earth's surface has been calculated over the mass range 10−13–1010 g by using cumulative influx rate data. Interpolation formulae have been fitted to this data and the resulting influx is found to vary between 3 × 108 and 5 × 1013 g. (Earth surface)−1 yr−1 depending on which data are used to obtain the formulae.
openaire +1 more source
Cometary Dust Loss, Meteoroid Streams and the Inner Solar System Dust Cloud
1996This paper reviews the way in which the dust cloud in the inner solar system is fed by the decay of comets and by interasteroidal collisions. Both these mechanisms lead to the formation of streams of meteoroid particles that can be observed on Earth as meteor showers.
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Mineral dust aerosol impacts on global climate and climate change
Nature Reviews Earth & Environment, 2023Jasper F Kok +2 more
exaly
Detecting meteoroid streams with an in-situ dust detector above an airless body
Icarus, 2016Jamey R Szalay, Mihaly Horanyi
exaly
Ignition hazard of non-metallic dust clouds exposed to hotspots versus electrical sparks
Journal of Hazardous Materials, 2019Chunmiao Yuan, Paul R Amyotte
exaly