The New Horizons (NH) flyby of the Pluto–Charon binary planet and its system of four small
surrounding satellites in mid-2015 revolutionized our knowledge of this distant planet and its …

We present the first application of a bin-scheme microphysical and vertical transport model
to determine the size distribution of titanium and silicate cloud particles in the atmospheres …

We determine the observability in transmission of inhomogeneous cloud cover on the limbs
of hot Jupiters through post-processing a general circulation model to include cloud …

New Horizons data provide a snapshot of the current state of Pluto's atmosphere. Winds are
slow and mostly controlled by sublimation of surface ices. Molecular nitrogen is the primary …

A planetary atmosphere is the outer gas layer of a planet. Besides its scientific significance
among the first and most accessible planetary layers observed from space, it is closely …

The observed mass–radius relationship of low-mass planets informs our understanding of
their composition and evolution. Recent discoveries of low-mass, large-radius objects (" …

Global Chemistry and Thermal Structure Models for the Hot Jupiter WASP-43b and Predictions
for JWST - IOPscience This site uses cookies. By continuing to use this site you agree to our …

Condensation clouds in substellar atmospheres have been widely inferred from spectra and
photometric variability. Up until now, their horizontally averaged vertical distribution and …

The Alice instrument on NASA's New Horizons spacecraft observed an ultraviolet solar
occultation by Pluto's atmosphere on 2015 July 14. The transmission vs. altitude was …

Most chemistry and cloud formation models for planetary atmospheres adopt a one-
dimensional (1D) diffusion approach to approximate the global-mean vertical tracer …