GD
Geodynamics

edited by Constanza Rodriguez Piceda

She is a postdoctoral researcher at University of Plymouth (UK). Her research interests span from the role of fault networks with complex geometries in earthquake processes to the link of the lithospheric structure with observed seismic deformation. She is co-editor-in-chief of the GD blog team.

Dirty Poppy and the Research Tournament of Arcane Mysteries.

Representative Cup for the winner of the Research Tournament of Arcane Mysteries. Figure generated by PromeAI.

In this week’s post, Dr. Katherine Villavicencio (University G. d’Annunzio, Italy) looks into the flaws of the academic system that enables abusive supervisors to hold excessive power.  In the form of a wizardly tale, she sheds light on the negative experiences of students subjected to the oppressive control of this kind of supervisors. In an alternate universe, the magical world is governed by ac ...[Read More]

Between the Volcano and the Deep Blue Sea: Tales from Montserrat (Part 1)

Between the Volcano and the Deep Blue Sea: Tales from Montserrat (Part 1)

In 1995, the Caribbean Island of Montserrat was shaken by the beginning of one of the most significant volcanic eruptions in recent history: one that profoundly changed the natural, social and economical landscape of the country. Three decades later, Soufrière Hills Volcano and its legacy of destruction still shape the lives of Montserrat’s people. Join us on the first part of our reportage and fi ...[Read More]

What’s the role of hotspot and oceanic transform faults at ultraslow spreading ridge?

What’s the role of hotspot and oceanic transform faults at ultraslow spreading ridge?

  Mid-ocean ridges (MOR) and hotspots are two types of magmatic activity occurring in the ocean. The MORs are typically associated with another tectonic feature—oceanic transform faults. While numerous studies have focused on the interactions within MORs, hotspots, and transform faults, there has been limited research on cases where a hotspot and a transform fault are located at the same end ...[Read More]

Ice Ice Baby! Modelling the thermal evolution within the ice shell of Ganymede, Jupiter’s moon.

Ice Ice Baby! Modelling the thermal evolution within the ice shell of Ganymede, Jupiter’s moon.

Ganymede, one of the Galilean moons of Jupiter and the largest in the Solar System, has caught the scientists’ attention due to its potential for hosting life. The JUICE mission, launched from the Guiana Space Centre in French Guiana on 14 April 2023, is on its way to orbit and conduct experiments on the Galilean moons (Ganymede, Europa, and Callisto), with  particular emphasis on characterizing G ...[Read More]