Ionospheric Radio
Abstract
This book is aimed at professional scientists, engineers and students who need an intermediate-level reference and/or text. Students of aeronomy and radio wave propagation are introduced to basic wave theory in absorbing, anisotropic and dispersive media and to the physics of production, loss, and movement of plasma in the ionosphere presence of the geomagnetic field.
Integrity signals
Registry
Cites
Statistics
Claims the paper makes
Claims other papers make about this one
Each is checked against this paper’s own text: does it say what the citing paper says it does?
Scintillation is more severe in equatorial and high latitude geomagnetic regions, particularly during solar maxima.
“Scintillation effects are more intense in geomagnetic equatorial and high latitude regions where the occurrences are mostly related respectively to the equatorial anomaly and geomagnetic storms.”
From Accuracy assessment of Precise Point Positioning with multi-constellation GNSS data under ionospheric scintillation effects (2018) · cites this paper as Davies, 1990
Scintillation is caused by small scale irregularities in the ionosphere and is characterized by rapid changes in amplitude and phase of the signal.
“Scintillation is caused by small scale irregularities in the ionosphere and is characterized by rapid changes in amplitude and phase of the signal, which are more severe in equatorial and high latitudes geomagnetic regions.”
From Accuracy assessment of Precise Point Positioning with multi-constellation GNSS data under ionospheric scintillation effects (2018) · cites this paper as Davies, 1990
In equatorial regions, scintillation occurrence is associated with the equatorial anomaly; in high latitude regions, it is associated with geomagnetic storms.
“Scintillation effects are more intense in geomagnetic equatorial and high latitude regions where the occurrences are mostly related respectively to the equatorial anomaly and geomagnetic storms.”
From Accuracy assessment of Precise Point Positioning with multi-constellation GNSS data under ionospheric scintillation effects (2018) · cites this paper as Davies, 1990
Cited by
Sorted by citations
Marques, H. A., Marques, H. A. S., Aquino, M., Veettil, S. V., & Monico, J. F. G. (2018) · Journal of Space Weather and Space Climate · doi:10.1051/swsc/2017043 · Cited by 57 · see citing works
- Authors
- Davies, K.
- Corresponding author
- Davies, Kenneth
- Venue
- Institution of Engineering and Technology eBooks
- Published
- 1990-01-01
- OpenAlex
- W4213019392
- Cited by
- 1,036
- References
- 0
- Citations by year
- 2026: 55 · 2025: 44 · 2024: 36 · 2023: 47 · 2022: 68 · 2021: 63 · 2020: 50 · 2019: 48 · 2018: 52 · 2017: 52 · 2016: 58 · 2015: 41 · 2014: 39 · 2013: 34 · 2012: 26
- FWCI
- 1.68
- Type
- book
- Language
- en
- Open access
- closed
- Locations
- Institution of Engineering and Technology eBooks (publishedVersion)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Ionosphere and magnetosphere dynamics
- Physical Sciences › Engineering › Aerospace Engineering › Radio Wave Propagation Studies
- Physical Sciences › Physics and Astronomy › Atomic and Molecular Physics, and Optics › Dust and Plasma Wave Phenomena
- Keywords
- ionosphere, radio wave propagation, aeronomy, plasma physics, anisotropic materials, absorbing media, geomagnetic field
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
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