Heat Flow and Near‐Seafloor Magnetic Anomalies Highlight Hydrothermal Circulation at Brothers Volcano Caldera, Southern Kermadec Arc, New Zealand
Key Points First systematic, integrated heat flow and magnetic study of a submarine arc volcano highlights multiscale convection cells Deep circulation structurally controlled, with recharge through the caldera floor and discharge at the caldera walls and postcollapse cones Shallow circulation is ch...
Gespeichert in:
Veröffentlicht in: | Geophysical research letters 2019-07, Vol.46 (14), p.8252-8260 |
---|---|
Hauptverfasser: | , , , |
Format: | Artikel |
Sprache: | eng |
Schlagworte: | |
Online-Zugang: | Volltext |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
Zusammenfassung: | Key Points
First systematic, integrated heat flow and magnetic study of a submarine arc volcano highlights multiscale convection cells
Deep circulation structurally controlled, with recharge through the caldera floor and discharge at the caldera walls and postcollapse cones
Shallow circulation is characterized by recharge zones in close proximity to the sites of present‐day diffuse and focused discharge
Brothers volcano is the most hydrothermally active volcano along the Kermadec arc, with distinct hydrothermal fields located on the caldera walls and on the postcollapse volcanic cones. These sites display very different styles of hydrothermal activity in terms of temperature, gas content, fluid chemistry, and associated mineralization. Here we show the results of a systematic heat flow survey integrated with near‐seafloor magnetic data acquired using remotely operated vehicles and autonomous underwater vehicles. Large‐scale circulation is structurally controlled, with a deep (~1‐ to 2‐km depth) central recharge through the caldera floor and lateral discharge along the caldera walls and at the summits of the postcollapse cones. Shallow (~ 0.1‐0.2 km depth) circulation is characterized by small‐scale recharge zones located at a distance of ~ 0.1–0.2 km from the active vent sites. |
---|---|
ISSN: | 0094-8276 1944-8007 |
DOI: | 10.1029/2019GL083517 |