Miller, S and Stallard, T and Smith, C and Millward, G and Melin, H and Lystrup, M and Aylward, A (2006) H-3(+): the driver of giant planet atmospheres. PHILOS T R SOC A , 364 (1848) 3121 - 3137. 10.1098/rsta.2006.1877.
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We present a review of recent developments in the use of H-3(+) molecular ion as a probe of physics and chemistry of the upper atmospheres of giant planets. This ion is shown to be a good tracer of energy inputs into Jupiter (J), Saturn (S) and Uranus (U). It also acts as a 'thermostat', offsetting increases in the energy inputs owing to particle precipitation via cooling to space (J and U). Computer models have established that H-3(+) is also the main contributor to ionospheric conductivity. The coupling of electric and magnetic fields in the auroral polar regions leads to ion winds, which, in turn, drive neutral circulation systems (J and S). These latter two effects, dependent on H-3(+), also result in very large heating terms, approximately 5 X 10(12) W for Saturn and greater than 10(14) W for Jupiter, planet-wide; these terms compare with approximately 2.5 X 10(11) W of solar extreme UV absorbed at Saturn and 10(12) W at Jupiter. Thus, H-3(+) is shown to play a major role in explaining why the temperatures of the giant planets are much greater (by hundreds of kelvin) at the top of the atmosphere than solar inputs alone can account for.
|Title:||H-3(+): the driver of giant planet atmospheres|
|Keywords:||planetary atmospheres, ionospheres, thermospheres, magnetospheres, infrared, MAIN AURORAL OVAL, IO FLUX TUBE, JOVIAN IONOSPHERE, SOLAR-WIND, MAGNETIC-FIELD, X-RAY, THERMOSPHERE, JUPITER, EMISSION, DYNAMICS|
|UCL classification:||UCL > School of BEAMS > Faculty of Maths and Physical Sciences > Physics and Astronomy|
UCL > School of BEAMS > Faculty of Maths and Physical Sciences > Science and Technology Studies
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