Search engine for discovering works of Art, research articles, and books related to Art and Culture
ShareThis
Javascript must be enabled to continue!

The ring-shaped thermal field of Stefanos crater, Nisyros Island: a conceptual model

View through CrossRef
Abstract. Fumarole fields related to hydrothermal processes release the heat of the underground through permeable pathways. Thermal changes, therefore, are likely to depend also on the variation of these pathways. As these paths may affect or even control the temperature field at the surface, their understanding is relevant to applied and basic science alike. A common difficulty, however, in surface temperature field studies at active volcanoes is that the parameters controlling the ascending routes of fluids are poorly constrained in general. Here we analyze the crater of Stefanos, Nisyros (Greece), and highlight complexities in the spatial pattern of the fumarole field related to permeability conditions. There may be different explanations for the observed permeability changes, such as structural control, lithology, weathering, and heterogeneous sediment accumulation and erosion. We combine high resolution infrared mosaics and grain-size analysis of soils, aiming to elaborate parameters controlling the appearance of the fumarole field. We find a ring-shaped thermal field located within the explosion crater, which is dependent on contrasts of the soil granulometry and volcanotectonic history. We develop a conceptual model of how the ring-shaped thermal field has formed at the Stefanos crater and similarly at other volcanic edifices, highlighting the importance of local permeability contrast that may increase or decrease the thermal fluid flux.
Title: The ring-shaped thermal field of Stefanos crater, Nisyros Island: a conceptual model
Description:
Abstract.
Fumarole fields related to hydrothermal processes release the heat of the underground through permeable pathways.
Thermal changes, therefore, are likely to depend also on the variation of these pathways.
As these paths may affect or even control the temperature field at the surface, their understanding is relevant to applied and basic science alike.
A common difficulty, however, in surface temperature field studies at active volcanoes is that the parameters controlling the ascending routes of fluids are poorly constrained in general.
Here we analyze the crater of Stefanos, Nisyros (Greece), and highlight complexities in the spatial pattern of the fumarole field related to permeability conditions.
There may be different explanations for the observed permeability changes, such as structural control, lithology, weathering, and heterogeneous sediment accumulation and erosion.
We combine high resolution infrared mosaics and grain-size analysis of soils, aiming to elaborate parameters controlling the appearance of the fumarole field.
We find a ring-shaped thermal field located within the explosion crater, which is dependent on contrasts of the soil granulometry and volcanotectonic history.
We develop a conceptual model of how the ring-shaped thermal field has formed at the Stefanos crater and similarly at other volcanic edifices, highlighting the importance of local permeability contrast that may increase or decrease the thermal fluid flux.

Related Results

Krupac crater in Sirenum Fossae, Mars: Understanding fresh impact cratering processes
Krupac crater in Sirenum Fossae, Mars: Understanding fresh impact cratering processes
Krupac crater in Sirenum Fossae, Mars: Understanding fresh impact cratering processesS. Vijayan, Harish and Bhalamurugan SivaramanPlanetary Science Division, Physical Research Labo...
Causes for the formation of cenotes (sinkholes) in post-impact strata of the Chicxulub crater, Yucatán Peninsula, Mexico
Causes for the formation of cenotes (sinkholes) in post-impact strata of the Chicxulub crater, Yucatán Peninsula, Mexico
The 66 Ma Chicxulub impact crater, Mexico, is obscured by hundreds of meters thick horizontal carbonate strata, which in age are as young as Pliocene. The spatial density of karst-...
Multiple superposed inverted landforms on Mars
Multiple superposed inverted landforms on Mars
<p><strong>Introduction:</strong> Inverted landforms are positive relief and well-preserved features; typically, their formation instigate...
Thermal Effects in High Compactness CEA Stack
Thermal Effects in High Compactness CEA Stack
Thermal management is a pivotal aspect of stack durability and system operability. Consequently, understanding the thermal mapping within a stack based on its operating conditions ...
Exploring the spectrophotometric properties of hollows from MESSENGER MIDS/WAC multiangular observations
Exploring the spectrophotometric properties of hollows from MESSENGER MIDS/WAC multiangular observations
Introduction: The origin and formation of Hollows, puzzling surface features identified on MESSENGER (MErcury Surface, Space ENvironment, GEochemistry, and Ranging, [1]) images [2]...
High‐Resolution Seismic Exploration of Xiuyan Impact Crater Structures
High‐Resolution Seismic Exploration of Xiuyan Impact Crater Structures
AbstractThe Xiuyan impact crater with a rim‐rim diameter of 1.8 km is located at northern hills in the Liaodong peninsula, Liaoning province, China, which is well reserved and conf...
A Tale of Two Moons: Global Crater Databases for Saturn’s Moons Dione and Tethys
A Tale of Two Moons: Global Crater Databases for Saturn’s Moons Dione and Tethys
USGS SIM geologic maps are being produced for Saturn’s moons Dione and Tethys (Martin et al., 2023; White et al., 2024) at 1:5M scale. As part of these mapping efforts, two global ...
Haleakala Crater, Maui, Hawaii
Haleakala Crater, Maui, Hawaii
Abstracr Haleakala Crater occupies the summit region of east Maui, Hawaii (Fig, 1). The crater is the center piece of Haleakala National Park and access is via Hawai...

Back to Top