The electron thermal structure in the dayside Martian ionosphere implied by the MGS radio occultation data
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Title
The electron thermal structure in the dayside Martian ionosphere implied by the MGS radio occultation data
Authors
Keywords
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Journal
JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS
Volume 120, Issue 2, Pages 278-286
Publisher
American Geophysical Union (AGU)
Online
2015-01-20
DOI
10.1002/2014je004726
References
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Related references
Note: Only part of the references are listed.- Predictions of electron temperatures in the Mars ionosphere and their effects on electron densities
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- Suprathermal electron spectra in the Venus ionosphere
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- Dayside ionosphere of Mars: Empirical model based on data from the MARSIS instrument
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- Observations of thermal tides in the middle atmosphere of Mars by the SPICAM instrument
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- Three-dimensional structure of the Martian nightside ionosphere: Predicted rates of impact ionization from Mars Global Surveyor magnetometer and electron reflectometer measurements of precipitating electrons
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- A review of observed variability in the dayside ionosphere of Mars
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- Simulating the density and thermal structure of the middle atmosphere (∼80–130km) of Mars using the MGCM–MTGCM: A comparison with MEX/SPICAM observations
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- A comparison of global models for the solar wind interaction with Mars
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- Density and temperatures of the upper Martian atmosphere measured by stellar occultations with Mars Express SPICAM
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