Results 111 to 120 of about 4,627 (227)

Ionosphere/microwave beam interaction study [PDF]

open access: yes
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.
core   +1 more source

Perpendicular Electrical Conductivity in the Topside Ionosphere Derived from Swarm Measurements

open access: yesRemote Sensing
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
doaj   +1 more source

Behavior of thermal plasma in the ionosphere and magnetosphere [PDF]

open access: yes
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.
core   +1 more source

Magnetosphere–Ionosphere Conjugate Harang Discontinuity and Sub-Auroral Polarization Streams (SAPS) Phenomena Observed by Multipoint Satellites

open access: yesAtmosphere
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
doaj   +1 more source

Ionospheric Plasma IRregularities - IPIR - Data Product Based on Data From the Swarm Satellites. [PDF]

open access: yesJ Geophys Res Space Phys, 2022
Jin Y   +7 more
europepmc   +1 more source

H2 Chemistry and Protonation in the Dayside Venusian Upper Atmosphere

open access: yesThe Astronomical Journal
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
doaj   +1 more source

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