Results 61 to 70 of about 87 (79)
Abstracts of the 2008 ISSOL Meeting. August 24-29, 2008. Florence, Italy. [PDF]
Orig Life Evol Biosph, 2009 europepmc +1 more source
Impact structures in Africa: A review.
J Afr Earth Sci, 2014 Reimold WU, Koeberl C.
europepmc +1 more source
Some of the next articles are maybe not open access.
Related searches:
Related searches:
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.
V V Shuvalov, I B Kosarev, T V Losseva
exaly +2 more sources
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.
V V Shuvalov, I B Kosarev, T V Losseva
exaly +2 more sources
Impacts of Fast Meteoroids and a Plasma–Dust Cloud Over the Lunar Surface
JETP Letters, 2017The possibility of the formation of a plasma–dust cloud in the exosphere of the Moon owing to impacts of meteoroids on the lunar surface is discussed. Attention is focused on dust particles at large altitudes of ~10–100 km at which measurements were performed within the NASA LADEE mission. It has been shown that a melted material ejected from the lunar
Lev M Zelenyi, Sergey I. Popel
exaly +2 more sources
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.
David W Hughes
exaly +2 more sources
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.
David W Hughes
exaly +2 more sources
Linking Studies of Tiny Meteoroids, Zodiacal Dust, Cometary Dust and Circumstellar Disks
Planetary and Space Science, 2020Jeremie Lasue, Julien Milli, J -B Renard
exaly
Atmospheric Effects of the Gas–Dust Plume of the Chelyabinsk Meteoroid of 2013
Izvestiya - Atmospheric and Oceanic Physics, 2017L F Chernogor
exaly