Better characterization features borne from long-term crustal modification processes is essential for understanding the dynamics of large basin-forming impact structures on Earth. Within the deeply eroded 2.02 Ga Vredefort Impact Structure in South Africa, impact melt dikes are exposed at the surface. In this study, we utilized a combination of field, remote sensing, electrical resistivity, magnetic, petrographical, and geochemical techniques to characterize one such impact melt dike, namely, the Holfontein Granophyre Dike (HGD), along with the host granites. The HGD is split into two seemingly disconnected segments. Geophysical modeling of both segments sug-gests that the melt rock does not penetrate below the modern surface deeper than 5 ...
International audienceThis study investigates the origin of the 2.69 Ga-old Matok pluton, emplaced i...
Meteorite impacts produce shocked minerals in target rocks that record diagnostic high-pressure defo...
International audienceWhile most impact craters are characterised by negative magnetic anomalies ove...
Better characterization features borne from long-term crustal modification processes is essential fo...
The timescale of the modification stage of basin-sized impact structures is not well understood. Owi...
The timescale of the modification stage of basin-sized impact structures is not well understood. Owi...
The Vredefort Dome is located within and almost central to the Witwatersrand basin in its presently ...
The Vredefort impact structure in South Africa is deeply eroded to its lowermost levels. However, g...
A Dissertation submitted to the Faculty of Science, University of the Witwatersrand; in fulfilment o...
The structure of the older-than-3.2-Ga Archean basement and Archean-to-Precambrian sedimentary/volca...
The unique 2.05-Ga Bushveld and Vredefort complexes cover 100,000 sq km (diameter 400 km) on the oth...
Reconstructing the terrestrial impact cratering record is a fundamental goal of planetary science. H...
The Vredefort structure located in the center of the Witwatersrand basin in South Africa and the Sud...
Introduction: The Rochechouart structure is a deeply eroded impact crater formed ~ 207 Myr ago and t...
International audienceTwo populations of magnetite exist in the shocked basement rocks of the Vredef...
International audienceThis study investigates the origin of the 2.69 Ga-old Matok pluton, emplaced i...
Meteorite impacts produce shocked minerals in target rocks that record diagnostic high-pressure defo...
International audienceWhile most impact craters are characterised by negative magnetic anomalies ove...
Better characterization features borne from long-term crustal modification processes is essential fo...
The timescale of the modification stage of basin-sized impact structures is not well understood. Owi...
The timescale of the modification stage of basin-sized impact structures is not well understood. Owi...
The Vredefort Dome is located within and almost central to the Witwatersrand basin in its presently ...
The Vredefort impact structure in South Africa is deeply eroded to its lowermost levels. However, g...
A Dissertation submitted to the Faculty of Science, University of the Witwatersrand; in fulfilment o...
The structure of the older-than-3.2-Ga Archean basement and Archean-to-Precambrian sedimentary/volca...
The unique 2.05-Ga Bushveld and Vredefort complexes cover 100,000 sq km (diameter 400 km) on the oth...
Reconstructing the terrestrial impact cratering record is a fundamental goal of planetary science. H...
The Vredefort structure located in the center of the Witwatersrand basin in South Africa and the Sud...
Introduction: The Rochechouart structure is a deeply eroded impact crater formed ~ 207 Myr ago and t...
International audienceTwo populations of magnetite exist in the shocked basement rocks of the Vredef...
International audienceThis study investigates the origin of the 2.69 Ga-old Matok pluton, emplaced i...
Meteorite impacts produce shocked minerals in target rocks that record diagnostic high-pressure defo...
International audienceWhile most impact craters are characterised by negative magnetic anomalies ove...