Abstract The Juno Microwave Radiometer (MWR) is a six-frequency scientific instrument
designed and built to investigate the deep atmosphere of Jupiter. It is one of a suite of …

Abstract Before Cassini, scientists viewed Saturn's unique features only from Earth and from
three spacecraft flying by. During more than a decade orbiting the gas giant, Cassini studied …

The Cassini mission unveiled the intense and diverse activity in Saturn's atmosphere:
banded jets, waves, vortices, equatorial oscillations. To set the path towards a better …

We present observations of Neptune taken in H-(1.4–1.8 µm) and K'-(2.0–2.4 µm) bands on
the nights of July 3, 2013 and August 20, 2014 from the 10-m WM Keck II Telescope using …

The Latitudinal Dependence of Atmospheric Jet Scales and Macroturbulent Energy
Cascades in: Journal of the Atmospheric Sciences Volume 72 Issue 10 (2015) Jump to …

Why Eddy Momentum Fluxes are Concentrated in the Upper Troposphere in: Journal of the
Atmospheric Sciences Volume 72 Issue 4 (2015) Jump to Content Jump to Main Navigation …

An explanation of long-lived Saturn's North Polar hexagonal circumpolar jet in terms of
instability of the coupled system polar vortex-circumpolar jet is proposed in the framework of …

The weather layers of the gas giant planets, Jupiter and Saturn, comprise the shallow
atmospheric layers that are influenced energetically by a combination of incoming solar …

We conduct an in-depth analysis of statistical flow properties calculated from the reference
high-resolution Saturn simulation obtained by global climate modelling in Part II. In the …

Based on an assumption of strongly inhomogeneous potential vorticity mixing in quasi-
geostrophic-plane turbulence, a relation is obtained between the mean spacing of …