Published 2025 | Version v1
Dataset Open

The Surface Heat Flow of Mars at the Noachian–Hesperian Boundary

  • 1. ROR icon Universidad Complutense de Madrid
  • 2. ROR icon University of Alicante
  • 3. ROR icon Universidad de Cádiz
  • 4. ROR icon Universidad Rey Juan Carlos

Description

This archive contains supplemental data for the manuscript

Ruiz, J., Parro, L.M., Egea-Gonzalez, I., Romeo, I., Alvarez-Lozano, J., Jiménez-Díaz, A. (2025). The Surface Heat Flow of Mars at the Noachian–Hesperian Boundary.

Format: 
# Pixel node registration used [Geographic grid]
# longitude latitude surface heat flow (mW/m²)

Global Heat Flow Model

Mars_N-H_SHF.xyz
N = 10800    <-179/179>    <-59/59>    <19.5/61>

Global Heat Flow Model with Large Plumes

Mars_N-H_SHF_Plumes.xyz
N = 10800    <-179/179>    <-59/59>    <19.5/119.2>

Files

Mars_N-H_SHF_Models.zip

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