S. Miller

Asymmetric Ionospheric Jets in Jupiter's Aurora

Saturn's Weather‐Driven Aurorae Modulate Oscillations in the Magnetic Field and Radio Emissions

ExoMol line lists – XL. Rovibrational molecular line list for the hydronium ion (H3O+)

The H ₃ ⁺ ionosphere of Uranus: decades-long cooling and local-time morphology

Local-time averaged maps of H ₃ ⁺ emission, temperature and ion winds

Observations of the chemical and thermal response of ‘ring rain’ on Saturn’s ionosphere

Identification of Jupiter’s magnetic equator through H3+ ionospheric emission

The Great Cold Spot in Jupiter's upper atmosphere

Ground-based observations of Saturn’s auroral ionosphere over three days: Trends in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si3.gif" overflow="scroll"><mml:mrow><mml:msubsup><mml:mrow><mml:mtext>H</mml:mtext></mml:mrow><mml:mrow><mml:mn>3</mml:mn></mml:mrow><mml:mrow><mml:mo>+</mml:mo></mml:mrow></mml:msubsup></mml:mrow></mml:math> temperature, density and emission with Saturn local time and planetary period oscillation

Magnetosphere–atmosphere coupling at Saturn: 1 – Response of thermosphere and ionosphere to steady state polar forcing

Peak emission altitude of Saturn's H₃⁺ aurora