Clouds Archives - Page 3 of 3 - Astrobiology

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Spatial Variations of Jovian Tropospheric Ammonia via Ground-Based Imaging

Jupiter

Spatial Variations of Jovian Tropospheric Ammonia via Ground-Based Imaging

Simulation-based Inference for Exoplanet Atmospheric Retrieval: Insights from winning the Ariel Data Challenge 2023 using Normalizing Flows

Exoplanets, -moons, -comets

Simulation-based Inference for Exoplanet Atmospheric Retrieval: Insights from winning the Ariel Data Challenge 2023 using Normalizing Flows

Mapping Water Clouds On Jupiter With Ultraviolet Data From Hubble

Gas Giants

Mapping Water Clouds On Jupiter With Ultraviolet Data From Hubble

Detecting Molecules In Ariel Low Resolution Transmission Spectra

Astrochemistry

Detecting Molecules In Ariel Low Resolution Transmission Spectra

Exoplanet Surveyor Ariel Passes Major Milestone

Ariel Mission

Exoplanet Surveyor Ariel Passes Major Milestone

Where Are The Water Worlds?: Self-Consistent Models of Water-Rich Exoplanet Atmospheres

Water/Hycean Worlds & Oceanography

Where Are The Water Worlds?: Self-Consistent Models of Water-Rich Exoplanet Atmospheres

Scattering Transparency of Clouds in Exoplanet Transit Spectra

Exoplanets, -moons, -comets

Scattering Transparency of Clouds in Exoplanet Transit Spectra

Cloud Behaviour On Tidally Locked Rocky Planets From Global High-resolution Modeling

Imaging & Spectroscopy

Cloud Behaviour On Tidally Locked Rocky Planets From Global High-resolution Modeling

The Earth-sized Exoplanet Next Door: The Venus Cloud Discontinuity in 2022

Venus

The Earth-sized Exoplanet Next Door: The Venus Cloud Discontinuity in 2022

YunMa: Enabling Spectral Retrievals of Exoplanetary Clouds

Imaging & Spectroscopy

YunMa: Enabling Spectral Retrievals of Exoplanetary Clouds

A JWST NIRSpec Phase Curve for WASP-121b: Dayside Emission Strongest Eastward of the Substellar Point and Nightside Conditions Conducive to Cloud Formation

Imaging & Spectroscopy

A JWST NIRSpec Phase Curve for WASP-121b: Dayside Emission Strongest Eastward of the Substellar Point and Nightside Conditions Conducive to Cloud Formation

Martian Dust Storms Churn Up Earth-like Clouds

Mars

Martian Dust Storms Churn Up Earth-like Clouds

Hubble WFC3 Spectroscopy of the Rocky Planet L 98-59 b: No Evidence for a Cloud-Free Primordial Atmosphere

Imaging & Spectroscopy

Hubble WFC3 Spectroscopy of the Rocky Planet L 98-59 b: No Evidence for a Cloud-Free Primordial Atmosphere

A Radiative-Convective Model For Terrestrial Planets With Self-Consistent Patchy Clouds

Exoplanets, -moons, -comets

A Radiative-Convective Model For Terrestrial Planets With Self-Consistent Patchy Clouds

Climate Of High Obliquity Exo-terrestrial Planets With A Three-dimensional Cloud System Resolving Climate Model

Atmospheres, Climate, Weather

Climate Of High Obliquity Exo-terrestrial Planets With A Three-dimensional Cloud System Resolving Climate Model

The Ariel Target List: The Impact of TESS and the Potential for Characterising Multiple Planets Within a System

Ariel Mission

The Ariel Target List: The Impact of TESS and the Potential for Characterising Multiple Planets Within a System

Ariel: Enabling Planetary Science Across Light-years

Ariel Mission

Ariel: Enabling Planetary Science Across Light-years

The Role of Clouds on the Depletion of Methane and Water Dominance in the Transmission Spectra of Irradiated Exoplanets

Exoplanets, -moons, -comets

The Role of Clouds on the Depletion of Methane and Water Dominance in the Transmission Spectra of Irradiated Exoplanets