Mineralogy of interplanetary dust particles from the “olivine” infrared class
- 31 May 1986
- journal article
- Published by Elsevier in Earth and Planetary Science Letters
- Vol. 78 (1) , 53-66
- https://doi.org/10.1016/0012-821x(86)90172-x
Abstract
No abstract availableKeywords
This publication has 10 references indexed in Scilit:
- Ion microprobe isotopic measurements of individual interplanetary dust particlesGeochimica et Cosmochimica Acta, 1985
- Laboratory infrared transmission spectra of individual interplanetary dust particles from 2.5 to 25 micronsThe Astrophysical Journal, 1985
- Hydrated interplanetary dust particle linked with carbonaceous chondrites?Nature, 1985
- Discovery of Nuclear Tracks in Interplanetary DustScience, 1984
- Transmission electron microscopy of the “LOW-CA” hydrated interplanetary dust particleEarth and Planetary Science Letters, 1984
- Pyroxene whiskers and platelets in interplanetary dust: evidence of vapour phase growthNature, 1983
- The survival of solar flare tracks in interplanetary dust silicates on deceleration in the Earth's atmosphereJournal of Geophysical Research, 1982
- Interplanetary dust in the transmission electron microscope: diverse materials from the early solar systemGeochimica et Cosmochimica Acta, 1981
- The quantitative analysis of thin specimensJournal of Microscopy, 1975
- THE MINERALOGY OF METEORITESMeteoritics, 1972