Topography on tidally locked M-dwarf planets induces stationary Rossby waves that strengthen cross-terminator jets, boost nightside moisture transport and cloud formation, and reduce the critical stellar flux for global deglaciation.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
fields
astro-ph.EP 2years
2026 2representative citing papers
citing papers explorer
-
Topography-Induced Stationary Waves and the Onset of Nightside Warming on Rocky Planets around M-dwarf Stars
Topography on tidally locked M-dwarf planets induces stationary Rossby waves that strengthen cross-terminator jets, boost nightside moisture transport and cloud formation, and reduce the critical stellar flux for global deglaciation.
- Modeling Volcanic Plume Heights Across Exoplanet Atmospheres: Insights from TRAPPIST-1