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  1. 5 sie 2011 · Abstract. Neutral density shows complicated temporal and spatial variations driven by external forcing of the thermosphere/ionosphere system, internal dynamics, and thermosphere and ionosphere coupling. Temporal variations include abrupt changes with a time scale of minutes to hours, diurnal variation, multi-day variation, solar-rotational ...

  2. 13 gru 2019 · The thermosphere of Mars is the interface through which the planet is continuously losing its reservoir of atmospheric volatiles to space. The structure and dynamics of the thermosphere is driven by a global circulation that redistributes the incident energy from the Sun.

  3. 16 mar 2022 · In this paper, we show that a simple arithmetic sum of the solar and geomagnetic indices can explain a large part of the day-to-day Texo variability. Also, Texo has good (poor) correlation with thermospheric parameters such as temperature and density above ∼130 km (at ∼100 km).

  4. 6 kwi 2023 · The design, principles of operation, calibration, and data analysis approaches of the Michelson Interferometer for Global High-resolution Thermospheric Imaging (MIGHTI) on the NASA Ionospheric Connection (ICON) satellite have been documented prior to the ICON launch.

  5. 13 maj 2019 · The scientific goals of the WACCM-X model include studying solar impacts on the Earth atmosphere, couplings between atmosphere layers through chemical, physical and dynamical processes, and the implications of the coupling for the climate and for the near-space environment.

  6. 28 lis 2022 · New, comprehensive, thermospheric composition and temperature (and wind) measurements in this altitude region, would significantly advance T-I system science, space weather modeling and prediction, and provide a means for more collaboration between the ground and space-based observation communities of the 100–200 km region.

  7. 12 cze 2024 · The thermospheric density and its variations are crucial to aerospace activities as well as space weather research and operation. However, due to the difficulties in observing the thermosphere, there has been a lack of effective descriptions for the general characteristics of thermospheric density.

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