Innovative Dose Rate Determinations for Luminescence Dating

Luminescence dating relies on the fact that mineral grains (crystals) are exposed to sources of natural radiation, which causes charge to be stored in electron traps within the crystal lattice. The radiation dose rate from the grain’s local environment, which ideally should be homogeneous, is what is routinely measured for luminescence dating. However, there are often local, sub-millimetre, sources of radiation heterogeneity that adversely affect a desired luminescence age. For the past 15 years, researchers have been developing Monte Carlo simulations and computer software that can correct for these heterogeneities. These new computer modelling techniques, and concomitant advances in statistics, allow more accurate luminescence dates to be obtained and also allow researchers access to a wider range of samples for an even greater number of dating applications.

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December 2025 --The Variscan Orogeny in Europe – Understanding Supercontinent Formation

The Variscan orogen formed between 380 and 300 million years ago through several accretionary and collisional cycles, culminating with the construction of the Pangea supercontinent. This process occurred via sequential opening and closure of oceanic basins, synchronous detachment of Gondwana derived continental ribbons, and their outboard amalgamation onto the Laurussia margin. The Variscan orogen is rather unique compared with other orogenic belts on Earth: its overthickened and dominantly magmatic crust in the central belt, surprisingly minor mantle involvement in the magmatic and geodynamic processes, coherent and pulsed magmatism along the collision suture, and its complex accretionary history. Because its final product, Pangea, is the youngest and best-understood supercontinent on Earth, the Variscan orogeny offers clues for understanding the mechanisms of supercontinent formation.