Results 91 to 100 of about 2,463,485 (172)

Photoelectron Flux in the Topside Ionosphere Measured by Retarding Potential Analyzers [PDF]

open access: yes, 1968
Photoelectron flux measurements in topside ionosphere using retarding potential ...
Donley, J. L., Rao, B. C. N.
core  

Atmosphere-Ionosphere (A-I) Coupling as Viewed by ICON: Day-to-Day Variability Due to Planetary Wave (PW)-Tide Interactions. [PDF]

open access: yesJ Geophys Res Space Phys, 2021
Forbes JM   +9 more
europepmc   +1 more source

Radio-induced incoherent scatter ion line enhancements with wide altitude extents in the high-latitude ionosphere [PDF]

open access: yes, 2013
[1] Apparent large electron density enhancements deduced from incoherent scatter radar observations during recent high power radio wave injection experiments at the European Incoherent Scatter Scientific Association (EISCAT) facility near Tromsø, Norway ...
Rietveld, M. T.   +3 more
core  

Q2DW-Tide and -Ionosphere Interactions as Observed From ICON and Ground-Based Radars. [PDF]

open access: yesJ Geophys Res Space Phys, 2021
Forbes JM   +11 more
europepmc   +1 more source

Neutral Composition Information in ICON EUV Dayglow Observations. [PDF]

open access: yesJ Geophys Res Space Phys, 2022
Tuminello RM   +8 more
europepmc   +1 more source

3DI: A novel ion composition and three-dimensional velocity analyzer for the topside ionosphere. [PDF]

open access: yesSci Rep, 2020
Ogasawara K   +6 more
europepmc   +1 more source

Capabilities of GNSS based topside reconstructions of the ionosphere

open access: yes, 2009
GPS navigation measurements onboard Low Earth Orbiting (LEO) satellites may be used to reconstruct the ionospheric electron density distribution from the LEO satellite orbit height up to GPS orbit heights.
Mayer, Christoph, Jakowski, Norbert
core  

On the relationship between energy input to the ionosphere and the ion outflow flux under different solar zenith angles. [PDF]

open access: yesEarth Planets Space, 2021
Kitamura N   +8 more
europepmc   +1 more source

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