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- W110260019 abstract "The Martian ionosphere has been studied by space missions since the beginning of the space age. Recently, the orbiters Mars Global Surveyor, Mars Odyssey and Mars Express have included instruments to study this component of the Martian atmosphere, which has triggered a renovated interest in this atmospheric region. The data from these instruments have allowed the study, among others, of the morphology of the ionosphere in the terminators (Fox and Yeager, 2006), of ionospheric structures associated with crustal magnetic fields (Gurnett et al., 2005), of the presence of meteoric layers (Withers et al., 2008), and of the effects of the EUV solar flux on the Total Electron Content (Lillis et al., 2010). From a global perspective, these measurements show that the ionosphere is influenced by external forcings (e.g. the solar flux) and also by the 3-D structure and variability of the underlying neutral atmosphere (Bougher et al., 2004). A General Circulation Model is a very useful tool for to study the ionosphere and its couplings, since predicted variations (spatial and temporal) in the temperature and composition of the neutral atmosphere are calculated and their effects on the ionosphere straightforwardly taken into account, so that no assumptions have to be made regarding these parameters" @default.
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- W110260019 date "2011-02-01" @default.
- W110260019 modified "2023-09-27" @default.
- W110260019 title "Study of the Martian Ionosphere with A General Circulation Model" @default.
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