From the 2 of 23 papers with an AI index.
4 citations
- University of Colorado BoulderUS14 papers
- Goddard Space Flight CenterUS7 papers
- Centre National de la Recherche ScientifiqueFR6 papers
- University of ChicagoUS5 papers
- Yale UniversityUS5 papers
- Carnegie Institution for ScienceUS4 papers
- Durham UniversityGB4 papers
- Jet Propulsion LaboratoryUS4 papers
- Lowell ObservatoryUS4 papers
- National Solar ObservatoryUS4 papers
- NSF NOIRLabUS4 papers
- Simons FoundationUS4 papers
6 papers · 1 filter
Upper Limits on Planet-Induced GHz Radio Emission from Inactive M Dwarfs
Jackie Villadsen, Carter Russell, Luna Guerrero +9
Nearby short-period exoplanet systems may produce detectable stellar radio emission due to sub-Alfvénic star-planet interaction (SPI), but there are no confirmed cases yet. We tar…
Maximum Lifetime of the Vegetative Biosphere
Jacob Haqq-Misra, Eric Wolf
We use a three-dimensional model to calculate steady-state climates at various intervals in Earth's future, across a parameter space of increasing insolation and decreasing CO…
Stellar flare-driven evolution of primordial early exo-Earth atmospheres: Insights from a Young M Dwarf Flare model
E. Mamonova, K. Herbst, V. Kofman +4
Context. M dwarfs are key targets for terrestrial exoplanet studies, with prospects for atmospheric spectroscopy. However, strong stellar magnetic activity and frequent flaring req…
Thermal Segregation and Reddening in Europa's Double Ridges
Kya C. Sorli, Paul O. Hayne, Lucas Lange +1
Europa's double ridges often display lower albedo and redder color than their surroundings. Their unique topography may cause sublimation-driven darkening due to illumination and s…
Disentangling auroral, cloud and magnetic spot driven variability in three early L-dwarfs with HST/WFC3
C. O'Toole, J. M. Vos, E. N. Nasedkin +5
Variability monitoring provides an unparalleled insight into the atmospheric processes of brown dwarfs and directly imaged exo-planets. Inhomogeneous clouds, aurorae and magnetic s…
The Effect of Planetary Rotation Period on Clouds in a Global Climate Model with a Bin Microphysics Scheme
Huanzhou Yang, Eric T. Wolf, Cheng-Cheng Liu +3
Clouds are the largest source of uncertainty in climate simulations. For exoplanets, cloud simulation is particularly challenging because of the lack of observational data to tune…