The parent impact crater of Australasian tektites has not been discovered so far, but a
consensus has been accepted on its location in a wider area of Indochina. Recently, an …

Résumé We propose a probabilistic approach to gauge the plausibility of a genetic link
between a distal ejecta and a known impact structure, considering the only possible …

Tektite and microtektite formation have important implications on our understanding of
impacts both on Earth, the Moon and on other bodies within our solar system. Here, we …

South China, the northern part of the Australasian strewn field (AASF) of tektites and
microtektites is located at the uprange of the hypothesized source crater that is still …

Abstract Tektites are reduced (Fe 2+) glasses formed by the quenching of molten material
ejected from Earth's surface as a result of a hypervelocity impact. The vast majority of tektites …

地外天体物质的高速撞击深刻地影响着地球系统各个圈层的协同演化. 撞击过程产生了广泛分布
的气化, 熔融和冲击变质物质, 其中, 一部分飞行距离超过母坑半径五倍的气化和熔融物快速冷却 …

Abstract In situ LA‐ICP‐MS/MS U‐Pb and Rb‐Sr geochronology combined with
geochemical analysis and electron microscopy have been performed on ejecta components …

Tektites are a rare type of impact glass; they are found in only four distinct and
geographically extended strewn fields, ranging from 0.8 to 35 million years in age. For three …

This thesis explores the gravity and magnetic aspects (functionals) derived from the gravity
gradient tensor (GGT) and magnetic gradient tensor (MGT). These functionals include …

We propose a probabilistic approach to gauge the plausibility of a genetic link between a
distal ejecta and a known impact structure, considering the only possible alternative that the …