Results 41 to 50 of about 1,807 (203)

Modeling the effects of equatorial plasma bubbles on the oblique propagation of high-frequency electromagnetic waves

Frontiers in Astronomy and Space Sciences
The ionosphere, as an essential component of the Earth’s space environment, contains free electrons that influence the amplitude and phase of radio signals.
Ziyi Zhao, Lingyun Zhu, Chunhua Jiang, Tongxin Liu, Guobin Yang, Zhengyu Zhao, Zhengyu Zhao   +6 more
doaj   +1 more source

Modeling z-shaped disturbance along the Pedersen ray of oblique sounding ionogram using adaptation of IRI to experimental data

Solar-Terrestrial Physics, 2016
We present the results of numerical modeling of a traveling ionospheric disturbance that causes z-shaped bends at the Pedersen ray of oblique incidence ionograms.
Kim A.G., Ponomarchuk S.N., Kotovich G.V., Romanova E.B.   +3 more
doaj   +1 more source

Optimization Algorithms for Retrieving the Bottomside Ionospheric B0 and B1 Parameters

Radio Science, Volume 61, Issue 10, October 2026.
Abstract The bottomside morphological parameters of the ionospheric F2 layer, the thickness parameter B0 and the shape parameter B1, are crucial for describing electron density profiles and monitoring space weather. However, existing climatological models and indirect ionosonde approaches have limitations in real‐time applicability and direct ...
Cheng Wang, Xiaoyu Zhu, Zhen Li
wiley   +1 more source

Computation of topside ionograms from N/h/ profiles [PDF]

, 1969
Computation of topside ionograms from electron concentration ...
Colin, L., Lee, J. G. K., Chan, K.-L.
core  

Application of Autoscala to ionograms recorded by the VIPIR ionosonde

, 2010
In November 2008, the ionosonde station at Boulder, Colorado, USA (40.0°N; 105.3°W) became the host of a new ionosonde (VIPIR, Vertical Incidence Pulsed Ionospheric Radar) developed and built by Scion Associates.
Scotto, C., Bullett, T., Malagnini, A., Pezzopane, M., M. Pezzopane, C. Scotto, T. Bullett, A. Malagnini   +7 more
core   +1 more source

Compatible analysis of vertical and oblique ionospheric sounding data

Annals of Geophysics, 1996
Examples are presented of the ray-tracing synthesis of multifrequency Oblique Sounding (OS) data on the Dourbes (Belgium) í Roquetes (Spain) path using electron density height profiles derived from Vertical Sounding (VS) measurements at both terminals ...
J. C. Jodogne, L. F. Alberca, I. V. Krasheninnikov   +2 more
doaj   +1 more source

Ionospheric Mechanisms Leading to Plasma‐Bubble Zonal Drift Reversal and Deformation During the 12 November 2025 Geomagnetic Storm

Space Weather, Volume 24, Issue 10, October 2026.
Abstract We present a multi‐instrument analysis of the ionospheric response to the intense geomagnetic storm of 12 November 2025 over the American sector, with emphasis on the longitudinally asymmetric deformation, latitudinal expansion, and zonal drift reversal of equatorial plasma bubbles (EPBs).
G. A. S. Picanço, I. Galkin, P. Song, E. Astafyeva, L. C. A. Resende, J. P. Marchezi, L. A. da Silva, P. R. Fagundes, C. M. Denardini, C. Martinis, A. M. Santos, V. G. Pillat, A. J. Coster, A. L. Christovam, S. R. Laranja, M. A. M. Lopes   +15 more
wiley   +1 more source

The reduction of topside ionograms to electron density profiles [PDF]

, 1969
Satellite ionosonde techniques and method for reducing topside ionograms to electron density ...
Jackson, J. E.
core  

Technical Possibilities and Limitations of the DPS-4D Type of Digisonde in Individual Meteor Detections

Remote Sensing
During the peak days of the 2019 Leonids and Geminids (16–19 November and 10–16 December), two ionograms/minute and one Skymap/minute campaign measurements were carried out at the Sopron (47.63°N, 16.72°E) and Průhonice (50.00°N, 14.60°E) Digisonde ...
Csilla Szárnya, Zbyšek Mošna, Antal Igaz, Daniel Kouba, Tobias G. W. Verhulst, Petra Koucká Knížová, Kateřina Podolská, Veronika Barta   +7 more
doaj   +1 more source

Type‐III Solar Radio Bursts at Mars: A 16.5‐Year Catalog From Mars Express‐MARSIS at 0.1–5.5 MHz

Space Weather, Volume 24, Issue 10, October 2026.
Abstract The most intense radio feature in the Solar System are the solar Type‐III radio bursts, which are associated with electron beams that propagate along open magnetic field lines. Although solar radio bursts have been studied since the 1940s, observations remain mainly restricted within 1 AU.
Beatriz Sánchez‐Cano, Samuel Carter, Mark Lester, Olivier Witasse, Caitriona M. Jackman, Sophie Musset, Baptiste Cecconi, Louis Siebenaler, Simon Joyce, Luis Alberto Cañizares, Andrea Cicchetti, Alexandra R. Fogg, Peter Gallagher, Christopher Gerekos, Yuki Harada, Alessandro Ippolito, Immanuel Jebaraj, Dikshita Meggi, Roberto Orosei, Hermann Opgenoorth, Jeff Plaut, Catherine Regan, Katerina Stergiopoulou   +22 more
wiley   +1 more source