Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
5487576 | Journal of Atmospheric and Solar-Terrestrial Physics | 2017 | 37 Pages |
Abstract
Analogues have been developed and characterised for both interplanetary dust and meteoric smoke particles. These include amorphous materials with elemental compositions similar to the olivine mineral solid solution series, a variety of iron oxides, undifferentiated meteorites (chondrites) and minerals which can be considered good terrestrial proxies to some phases present in meteorites. The products have been subjected to a suite of analytical techniques to demonstrate their suitability as analogues for the target materials.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Geophysics
Authors
Alexander D. James, Victoria L.F. Frankland, Josep M. Trigo-RodrÃguez, Jacinto Alonso-Azcárate, Juan Carlos Gómez MartÃn, John M.C. Plane,