Global model VenusLithoHeat2024

Resumen

Global model VenusLithoHeat2024 Reference: Ruiz, J., Jiménez-Díaz, A., Egea-González, I., Romeo, I., Kirby, J.F., Audet, P., 2024. Heat loss and internal dynamics of Venus from global surface heat flow estimates. arXiv:2401.06558. https://doi.org/10.48550/arXiv.2401.06558 Contact: Javier Ruiz (jaruiz@ucm.es) Description: Column 1: Longitude (°) Column 2: Latitude (°) Column 3: Crustal thickness, Tc (km) Column 4: Effective elastic thickness, Te (km) Column 5: Te error (km) Column 6: Surface heat flow, Fs (mW/m²) Column 7: Surface heat flow, 1-σ uncertainty (mW/m²) Column 8: Temperature at the base of the crust, Tcb (K) If you use the crustal thickness model in your work, please cite: Jiménez-Díaz, A., Ruiz, J., Kirby, J.F., Romeo, I., Tejero, R., Capote, R., 2015. Lithospheric structure of Venus from gravity and topography. Icarus 260, 215–231. https://doi.org/10.1016/j.icarus.2015.07.020 If you use the effective elastic thickness model in your work, please cite: Jiménez-Díaz, A., Ruiz, J., Kirby, J.F., Romeo, I., Tejero, R., Capote, R., 2015. Lithospheric structure of Venus from gravity and topography. Icarus 260, 215–231. https://doi.org/10.1016/j.icarus.2015.07.020 Ruiz, J., Jiménez-Díaz, A., Egea-González, I., Romeo, I., Kirby, J.F., Audet, P., 2024. Heat loss and internal dynamics of Venus from global surface heat flow estimates. arXiv:2401.06558. https://doi.org/10.48550/arXiv.2401.06558