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Combined model of topside ionosphere and plasmasphere derived from radio-occultation and Van Allen Probes data [PDF]

open access: yesScientific Reports, 2022
In the last years, electron density profile functions characterized by a linear dependence on the scale height showed good results when approximating the topside ionosphere. The performance above 800 km, however, is not yet well investigated.
Fabricio S. Prol   +3 more
doaj   +2 more sources

A novel neural network model of Earth’s topside ionosphere [PDF]

open access: yesScientific Reports, 2023
The Earth’s ionosphere affects the propagation of signals from the Global Navigation Satellite Systems (GNSS). Due to the non-uniform coverage of available observations and complicated dynamics of the region, developing accurate models of the ionosphere ...
Artem Smirnov   +6 more
doaj   +2 more sources

The Effects of Solar Wind Dynamic Pressure on the Structure of the Topside Ionosphere of Mars

open access: yesGeophysical Research Letters, 2019
We use Mars Atmosphere and Volatile EvolutioN observations of the upstream solar wind, and Mars Express observations of ionospheric electron densities and magnetic fields, to study how the topside ionosphere (>320 km) of Mars is affected by variations in
Z. Girazian   +5 more
doaj   +2 more sources

Dissipation of field-aligned currents in the topside ionosphere. [PDF]

open access: yesSci Rep, 2022
AbstractField-aligned currents (FACs) are electric currents parallel to the geomagnetic field and connecting the Earth’s magnetosphere to the high-latitude ionosphere. Part of the energy injected into the ionosphere by FACs is converted into kinetic energy of the surrounding plasma.
Giannattasio F   +6 more
europepmc   +4 more sources

TEC Enhancement due to Energetic Electrons Above Taiwan and the West Pacific

open access: yesTerrestrial, Atmospheric and Oceanic Sciences, 2013
The energetic electrons of the inner radiation belt during a geomagnetic disturbance can penetrate in the forbidden range of drift shells located at the heights of the topside equatorial ionosphere (< 1000 km).
Alla V. Suvorova   +2 more
doaj   +4 more sources

Enhanced variability in the topside ionosphere

open access: yesAnnals of Geophysics, 1995
Variability of total electron content (TEC) observed by the Faraday rotation method at Florence has been stud- ied with the same technique applied independently to the ionospheric parameters foF2 and M(3000)F2 of the ground-based vertical-incidence ...
P. Spalla, T. Gulyaeva
doaj   +3 more sources

The Analysis of the Topside Additional Layer of Martian Ionosphere Using MARSIS/Mars Express Data [PDF]

open access: yesJournal of Astronomy and Space Sciences, 2012
In this study, the transient second or third layer on the topside of the Martian ionosphere were investigated with the most recently released Mars advanced radar for subsurface and ionospheric sounding/Mars Express data obtained from January 2010 to ...
Eojin Kim   +6 more
doaj   +1 more source

Post-midnight irregularities in equator and its adjacent regions of topside ionosphere obtained by the CSES satellite

open access: yesFrontiers in Earth Science, 2023
The post-midnight irregularities in equator and its adjcent regions, which have remained least explored so far, are investigated using the in situ electron density (Ne) measurements from 2019 to 2021 obtained by the China Seismo-Electromagnetic Satellite
Xiuying Wang   +8 more
doaj   +1 more source

Modeling of Topside Ionosphere and Plasmasphere [PDF]

open access: yes, 2021
Abstract We developed a new topside ionosphere and plasmasphere model using a machine learning technique using approximately five million electron density datasets from the Japanese satellites, namely, Hinotori, Akebono, and Arase. The topside ionosphere and plasmasphere model (TIP-model) can estimate electron densities at altitudes ranging ...
Shigeto Watanabe   +6 more
openaire   +1 more source

A New Method for Retrieving Electron Density Profiles from the MARSIS Ionograms

open access: yesRemote Sensing, 2022
The Martian ionosphere was actively detected by Mars Advanced Radar for Subsurface and Ionosphere Sounding (MARSIS) aboard the Mars Express. The detected echo signal of the MARSIS at an epoch is presented as a function of frequency and time delay to form
Wendong Liu   +9 more
doaj   +1 more source

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