View Selected Publications
- H. Hay, I. Matsuyama, and R. Pappalardo (2022). “The high-frequency tidal response of ocean
worlds: Application to Europa and Ganymede”. Journal of Geophysical Research: Planets. DOI: 10.1029/2021JE007064 - H. Hay, A. Trinh, and I. Matsuyama (2020). “Powering the Galilean Satellites with Moon-Moon
Tides”. Geophysical Research Letters 47.15, e2020GL088317. DOI: 10.1029/2020GL088317 - H. Hay and I. Matsuyama (2019b). “Tides Between the TRAPPIST1 Planets”. The Astrophysical Journal 875.1, p. 22. DOI: 10.3847/1538-4357/ab0c21
- H. Hay and I. Matsuyama (2019a). “Nonlinear tidal dissipation in the subsurface oceans of Enceladus and other icy satellites”. Icarus 319, pp. 68–85. DOI: 10.1016/j.icarus.2018.09.019
- I. Matsuyama, M. Beuthe, H. Hay, F. Nimmo, and S. Kamata (2018). “Ocean tidal heating in icy satellites with solid shells”. Icarus 312, pp. 208–230. DOI: 10.1016/j.icarus.2018.04.01
View Extended Publications
- E. Leonard, S. Howell, A. Mills, D. Senske, D. Patthoff, H. Hay, and R. Pappalardo (2022). “Finding
order in chaos: Quantitative predictors of chaos terrain morphology on Europa”. Geophysical
Research Letters. DOI: 10.1029/2021GL097309 - H. Hay and I. Matsuyama (2017). “Numerically modelling tidal dissipation with bottom drag in the
oceans of Titan and Enceladus”. Icarus 281, pp. 342–356. DOI: 10.1016/j.icarus.2016.09.022