Ultraviolet Sensing of Volcanic Sulfur Emissions

While other volcanic gas species are more abundant than sulfur, it is the measurement of sulfur dioxide emissions that has played the key geochemical role in volcano monitoring for decades. Recently, this sphere of volcano surveillance has undergone a revolution: the instruments suitable for the task have become cheaper, more compact, less power hungry, and more capable than their predecessors. It is now possible to measure multiple gas species simultaneously, at high time resolution, and even to image volcanic clouds remotely. This technological explosion is leading to the installation of a global network of volcanic-emission sensors. This network will underpin the geochemical surveillance and hazard assessment at volcano observatories worldwide and will yield new insights into the degassing and eruptive style of volcanoes and the impact of volcanic clouds on the atmosphere.

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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.