Preprints
https://doi.org/10.5194/egusphere-2025-3036
https://doi.org/10.5194/egusphere-2025-3036
07 Jul 2025
 | 07 Jul 2025

Numerical simulation of magma-rock interaction at Krafla volcano using OpenFOAM software and a simplified thermal model

Muriel Gerbault, Oleg Melnik, and Anastassia Borisova

Abstract. We present a 2D numerical modelling study aimed at exploring magma-rock interaction following the emplacement of a magmatic sill into cold shallow crust. An interface-tracking solver was developed, based on the open-source OpenFOAM package that enables simulation of heat and momentum transfer between magmas of different compositions, with contrasting densities, thermal properties, temperatures, crystal contents, and strain-rate dependent viscosities. Two scenarios are considered to reconstruct sharp temperature gradients and explain the presence of fresh rhyolitic fragments excavated from approximately 2 km depth during IDDP-1 drilling at Krafla caldera in 2009: partial melting of felsic crust triggered by either (1) a 300 m thick rhyolite intrusion or (2) a 100 m thick basalt sill. We also assume two possible magma emplacement periods: during the Krafla Fires (1975–1984, ~35 years before drilling) and the Myvatn Fires (1724–1729, ~300 years before drilling). In scenario (1), vigorously convective molten rhyolite produces a temperature jump (400 °C) over approximately 25 meters (~16 °C/m) 35 years after emplacement. After 300 years, the thickness of these molten rocks reaches approximately 75 m, however, the thermal gradient becomes too small (less than 5 °C/m) to explain the IDDP-1 observations. In scenario (2), because of large density contrasts between the injected basaltic magma and molten rhyolite, two separate convective layers are formed. The thickness of molten rocks exceeds 30 m after 30 years. The rapid melting front propagation causes a sharp temperature gradient in the undisturbed rocks (28 °C/m). We conclude that the second scenario provides a more reliable explanation for the existing data and is well supported by previous petrological studies. By comparing with a simplified 1D thermal model and performing parametric tests, we argue that our numerical approach is suitable for studying magmatic convection at such extremely high Rayleigh and Prandtl numbers.

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Muriel Gerbault, Oleg Melnik, and Anastassia Borisova

Status: final response (author comments only)

Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor | : Report abuse
  • RC1: 'Comment on egusphere-2025-3036', Catherine Annen, 25 Jul 2025
    • CC1: 'AC reply on RC1', Oleg Melnik, 13 Aug 2025
      • AC2: 'Reply on CC1', Oleg Melnik, 10 Sep 2025
  • RC2: 'Comment on egusphere-2025-3036', Alain Burgisser, 20 Aug 2025
    • AC1: 'Reply on RC2', Oleg Melnik, 01 Sep 2025
  • EC1: 'Comment on egusphere-2025-3036', Virginie Pinel, 08 Sep 2025
Muriel Gerbault, Oleg Melnik, and Anastassia Borisova
Muriel Gerbault, Oleg Melnik, and Anastassia Borisova

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Short summary
Intrusion of a hot basaltic magma into produces melting of host rocks. We simulate this process by means of 2D thermo-hydrodynamical model with account for variable magma properties. The melting front rapidly propagates into intact rocks, leading to a formation of a sharp temperature gradient on magma-rock interface. Our modelling proposes that a basaltic sill was injected during Krafla Fires, leading to formation of ~30 m of molten felsic magma that was penetrated by IDDP-1 drilling.
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