The subject of this review is the atmospheric chemistry of the metals which ablate from
meteoroids in the Earth, s upper atmosphere. The major meteoric species are Fe, Mg, Si …

Gas‐phase experiments with state‐of‐the‐art techniques of mass spectrometry provide
detailed insights into numerous elementary processes. The focus of this Review is on …

This is the fifteenth in a series of evaluated sets of rate constants and photochemical cross
sections compiled by the NASA Panel for Data Evaluation. The data are used primarily to …

This review discusses the magnitude of the cosmic dust input into the earth's atmosphere,
and the resulting impacts from around 100 km to the earth's surface. Zodiacal cloud …

Shock waves and the associated phenomena generated by strongly ablating meteoroids
with sizes greater than a few millimeters in the lower transitional flow regime of the Earth's …

Most of the extraterrestrial dust entering the Earth's atmosphere ablates to produce metal
vapours, which have significant effects on the aeronomy of the upper mesosphere and lower …

Considerable progress has been made over the past years concerning the experimental
capabilities to observe mesospheric ice particles from space, from the ground, and in situ …

Micrometeorites that ablate in the lower thermosphere and upper mesosphere are thought to
recondense into nanometer‐sized smoke particles and then coagulate into larger dust …

On the basis of the Constellation Observing System for Meteorology, Ionosphere, and
Climate (COSMIC)‐measured fluctuations in the signal‐to‐noise ratio and excess phase of …

Dissecting the photochemical reactivity of metal ions is a significant contribution to
understanding secondary pollutant formation, as they have a role to be reckoned with …