The morphologies of the ultraviolet auroral emissions on the giant gas planets, Jupiter and
Saturn, have conveniently been described with combinations of a restricted number of basic …

Auroras are (generally) high‐latitude atmospheric emissions that result from the precipitation
of energetic charged particles from a planet's magnetosphere. Auroral emissions from the …

Ensemble recordings of 73 to 148 rat hippocampal neurons were used to predict accurately
the animals' movement through their environment, which confirms that the hippocampus …

Voyager 2 images of Neptune reveal a windy planet characterized by bright clouds of
methane ice suspended in an exceptionally clear atmosphere above a lower deck of …

This textbook was developed to provide seniors and first-year graduate students in physical
sciences with a general knowledge of electrodynamic phenomena in space. Since the …

On attending a conference on the Jovian satellites at UCLA, I heard Lou Lanze rotti
vigorously present the exciting data on the sputtering of water ice by Me V protons taken with …

The vertical structure of Neptune's atmosphere is studied on the basis of recordings of the
tracking signals received from Voyager 2 during its occultation by Neptune. The …

The present 15th volume of the ISSI Space Science Series is devoted to Auroral Plasma
Physics. The aurora is arguably the most intriguing phenomenon in space plasma physics …

Observations of the 1.4-to 2.4-micrometer spectrum of Pluto reveal absorptions of carbon
monoxide and nitrogen ices and confirm the presence of solid methane. Frozen nitrogen is …

The near-infrared spectrum of Triton reveals ices of nitrogen, methane, carbon monoxide,
and carbon dioxide, of which nitrogen is the dominant component. Carbon dioxide ice may …