Ionosphere/microwave beam interaction study [PDF]
A solar power satellite microwave power density of 20mw sq cm was confirmed as the level where nonlinear interactions may occur in the ionosphere, particularly at 100 km altitude.
Duncan, L. M., Gordon, W. E.
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Perpendicular Electrical Conductivity in the Topside Ionosphere Derived from Swarm Measurements
The study of the physical properties of the topside ionosphere is fundamental to investigating the energy balance of the ionosphere and developing accurate models to predict relevant phenomena, which are often at the root of Space Weather effects in the ...
Fabio Giannattasio +7 more
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Day-to-Day Variability of the Semidiurnal Tide in the F-Region Ionosphere During the January 2021 SSW From COSMIC-2 and ICON. [PDF]
Oberheide J.
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Behavior of thermal plasma in the ionosphere and magnetosphere [PDF]
Models of ion flow in the topside ionosphere were developed. These models took both H(+) and O(+) into account and permitted various parameter studies to be made affecting H(+) escape in polar winds.
Banks, P. M., Doupnik, J. R.
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It is well understood that near midnight, the Harang Discontinuity separates the auroral duskside eastward electrojet (EEJ) and dawnside westward electrojet (WEJ) and associated plasma flows driven by enhanced magnetospheric convections via Magnetosphere–
Ildiko Horvath, Brian C. Lovell
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Performance evaluation of IRI-Plas 2017 model with ionosonde data measurements of ionospheric parameters. [PDF]
Endeshaw L, Seyoum A.
europepmc +1 more source
Neustrelitz Total Electron Content Model for Galileo Performance: A Position Domain Analysis. [PDF]
Gioia C, Angrisano A, Gaglione S.
europepmc +1 more source
Ionospheric Plasma IRregularities - IPIR - Data Product Based on Data From the Swarm Satellites. [PDF]
Jin Y +7 more
europepmc +1 more source
Middle latitude changes in topside electron density through a magnetic storm technical note no. 1, 24.- 28 jun. 1963 [PDF]
Middle latitude changes in topside electron density during magnetic ...
Milic, P. L.
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H2 Chemistry and Protonation in the Dayside Venusian Upper Atmosphere
Although H _2 is present in low concentrations, it critically controls the structure and composition of planetary upper atmospheres through protonation under solar extreme-ultraviolet and soft X-ray irradiation. Recent studies highlight the importance of
Shiqi Wu +3 more
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