From the mid-Ordovician into the Late Silurian: Changes in the micrometeorite flux after the L chondrite parent breakup
Author:
Affiliation:
1. Astrogeobiology Laboratory; Department of Physics; Lund University; Box 118 SE-221 00 Lund Sweden
2. Center for Geosciences; Austrian Academy of Sciences; Dr. Ignaz Seipel-Platz 2 A-1010 Vienna Austria
Funder
H2020 European Research Council
Publisher
Wiley
Subject
Space and Planetary Science,Geophysics
Link
http://onlinelibrary.wiley.com/wol1/doi/10.1111/maps.13174/fullpdf
Reference57 articles.
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3. Numerical simulation of high-velocity impact ejecta following falls of comets and asteroids onto the Moon;Artemieva;Solar System Research,2008
4. The range of spinel compositions in terrestrial mafic and ultramafic rocks;Barnes;Journal of Petrology,2001
5. Sedimentary pyrite formation: An update;Berner;Geochimica et Cosmochimica Acta,1984
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