Area of research
Astronomy and Astrophysics · Atmospheric Science
Research interest
Research interests include Astro and Planetary Science, Stellar, planetary, and galactic studies, Climate variability and models, and Geology and Paleoclimatology Research.
Can AI weather models predict out-of-distribution gray swan tropical cyclones?
Revealing the Statistics of Extreme Events Hidden in Short Weather Forecast Data
The Effect of Ocean Salinity on Climate and Its Implications for Earth's Habitability
Probing the Capability of Future Direct-imaging Missions to Spectrally Constrain the Frequency of Earth-like Planets
Rare Event Sampling Improves Mercury Instability Statistics
The Effect of Substellar Continent Size on Ocean Dynamics of Proxima Centauri b
Spatial Radiative Feedbacks from Internal Variability Using Multiple Regression
The Atmospheric Circulation and Climate of Terrestrial Planets Orbiting Sun-like and M Dwarf Stars over a Broad Range of Planetary Parameters
Simple Rules Govern the Patterns of Arctic Sea Ice Melt Ponds
Snowball Earth climate dynamics and Cryogenian geology-geobiology
Persistence of a freshwater surface ocean after a snowball Earth
No Snowball on Habitable Tidally Locked Planets
DIFFERENCES IN WATER VAPOR RADIATIVE TRANSFER AMONG 1D MODELS CAN SIGNIFICANTLY AFFECT THE INNER EDGE OF THE HABITABLE ZONE
EFFECT OF SURFACE-MANTLE WATER EXCHANGE PARAMETERIZATIONS ON EXOPLANET OCEAN DEPTHS
Feedback temperature dependence determines the risk of high warming
DECIPHERING THERMAL PHASE CURVES OF DRY, TIDALLY LOCKED TERRESTRIAL PLANETS
STRONG DEPENDENCE OF THE INNER EDGE OF THE HABITABLE ZONE ON PLANETARY ROTATION RATE
WATER TRAPPING ON TIDALLY LOCKED TERRESTRIAL PLANETS REQUIRES SPECIAL CONDITIONS
Resolved Snowball Earth Clouds
Effects of explicit atmospheric convection at high CO <sub>2</sub>
Intra-surface radiative transfer limits the geographic extent of snow penitents on horizontal snowfields
STABILIZING CLOUD FEEDBACK DRAMATICALLY EXPANDS THE HABITABLE ZONE OF TIDALLY LOCKED PLANETS
Robust elements of Snowball Earth atmospheric circulation and oases for life
THERMAL PHASES OF EARTH-LIKE PLANETS: ESTIMATING THERMAL INERTIA FROM ECCENTRICITY, OBLIQUITY, AND DIURNAL FORCING
Sea-ice dynamics strongly promote Snowball Earth initiation and destabilize tropical sea-ice margins
Clouds and Snowball Earth deglaciation
Continental constriction and oceanic ice‐cover thickness in a Snowball‐Earth scenario
A FALSE POSITIVE FOR OCEAN GLINT ON EXOPLANETS: THE LATITUDE-ALBEDO EFFECT