Author name: Susan L. Brantley

Crossing Disciplines and Scales to Understand the Critical Zone

The Critical Zone (CZ) is the system of coupled chemical, biological, physical, and geological processes operating together to support life at the Earth’s surface. While our understanding of this zone has increased over the last hundred years, further advance requires scientists to cross disciplines and scales to integrate understanding of processes in the CZ, ranging in scale from the mineral–water interface to the globe. Despite the extreme heterogeneities manifest in the CZ, patterns are observed at all scales. Explanations require the use of new computational and analytical tools, inventive interdisciplinary approaches, and growing networks of sites and people.

This content is for Registered members only. To subscribe, please
join one of our participating societies or contact the Editorial Team.

Login
Already a member? Log in here

Crossing Disciplines and Scales to Understand the Critical Zone Read More »

Reactive Transport Models of Weathering

Continental rocks chemically weather when surficial waters and gases interact with the minerals and organisms that inhabit Earth’s critical zone. To understand and quantify this process, researchers use reactive transport models to track the kinetics and thermodynamics of weathering reactions and the transport of products and reactants. These models are powerful tools to explore how weathering sculpts the Earth’s surface from the scale of mineral grains to watersheds, and across temporal scales from seconds to millions of years. Reactive transport model simulations are now a vital tool for elucidating the complex links between climate, rock ­weathering, and biota.

This content is for Registered members only. To subscribe, please
join one of our participating societies or contact the Editorial Team.

Login
Already a member? Log in here

Reactive Transport Models of Weathering Read More »

Scroll to Top

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.