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 …

Liquid water oceans are now predicted to exist beneath the icy shells of numerous worlds in
the outer solar system. These ocean worlds are prime targets in our search for evidence of …

NASA's Dragonfly mission will send a rotorcraft lander to the surface of Titan in the mid-
2030s. Dragonfly's science themes include investigation of Titan's prebiotic chemistry …

In this introductory chapter we describe general properties of the Earth–ionosphere cavity,
outline the relationship of the global electromagnetic resonance to other natural low …

The Cassini-Huygens mission that explored the Saturn system during the period 2004–2017
revolutionized our understanding of Titan, the only known moon with a dense atmosphere …

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 …

We present new experimental data on the liquidus of ice polymorphs in the H 2 O–NH 3
system under pressure, and use all available data to develop a new thermodynamic model …

Using electric field measurements gathered on the C/NOFS satellite, we report, Schumann
resonance signatures detected in space, well beyond the upper boundary of the resonant …

This study illuminates scenarios whereby the heat produced by the dissipation of ocean
tides is significant in the heat budgets maintaining liquid oceans on icy satellites in the outer …

The historical development of terrestrial atmospheric electricity is described, from its
beginnings with the first observations of the potential gradient to the global electric circuit …