Titan is the only moon with a substantial atmosphere, the only other thick N2 atmosphere
besides Earth's, the site of extraordinarily complex atmospheric chemistry that far surpasses …

This review presents an insight into our current knowledge of the atmospheres of the planets
Venus, Mars, Jupiter, Saturn, Uranus and Neptune, the satellite Titan, and those of …

A new planetary atmospheric numerical model,“planetWRF,” has been developed by
modifying the Weather Research and Forecasting (WRF) model. The model has generalized …

Thousands of longitudinal dunes have recently been discovered by the Titan Radar Mapper
on the surface of Titan. These are found mainly within±30° of the equator in optically-, near …

We have developed a new 3-dimensional climate model for Titan's atmosphere, using the
physics of the IPSL Titan 2-dimensional climate model with the current version of the LMDZ …

This book describes how sand dunes work, why they are the way they are in different
settings, and how they are being studied. Particular attention is paid to their formation and …

The Composite Infrared Radiometer–Spectrometer (CIRS) instrument, on the NASA Cassini
Saturn orbiter, has been acquiring thermal emission spectra from the atmosphere of Titan …

This paper describes new oscillator and atomic clock technologies that, when combined,
create a master oscillator for use in deep-space navigation and science measurements. This …

TitanWRF general circulation model simulations performed without sub-grid-scale horizontal
diffusion of momentum produce roughly the observed amount of superrotation in Titan's …

This study presents an approximate model for the atypical Schumann resonance in Titan's
atmosphere that accounts for the observations of electromagnetic waves and the …