Atmospheric deposition of cosmic dust studied by moss analysisстатья
Информация о цитировании статьи получена из
Web of Science
Статья опубликована в журнале из списка Web of Science и/или Scopus
Дата последнего поиска статьи во внешних источниках: 4 сентября 2019 г.
Аннотация:The majority of particles undergo melting during their passage through the atmosphere.
Most abundantly, particularly at large sizes, cosmic spherules, i.e. completely melted droplets, were observed. These
spherical particles provide a useful proxy for the total flux of dust because they are relatively easy to identify. They
are the background magnetic component of cosmic dust, mainly microspheres and particles of native metals. Most
often, it was possible to detect native Fe, Fe-Ni and Fe-Cr minerals.