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HF radar signatures of the cusp and low-latitude boundary layer

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TLDR
In this article, an intercalibration study made using the Polar Anglo-American Conjugate Radar Experiment radars located at Goose Bay, Labrador, and Halley Station, Antarctica, and the Defense Meteorological Satellite Program (DMSP) satellites is used to provide clear identifications of the ionospheric cusp and the low-latitude boundary layer (LLBL).
Abstract
Continuous ground-based observations of ionospheric and magnetospheric regions are critical to the Geospace Environment Modeling (GEM) program. It is therefore important to establish clear intercalibrations between different ground-based instruments and satellites in order to clearly place the ground-based observations in context with the corresponding in situ satellite measurements. HF-radars operating at high latitudes are capable of observing very large spatial regions of the ionosphere on a nearly continuous basis. In this paper we report on an intercalibration study made using the Polar Anglo-American Conjugate Radar Experiment radars located at Goose Bay, Labrador, and Halley Station, Antarctica, and the Defense Meteorological Satellite Program (DMSP) satellites. The DMSP satellite data are used to provide clear identifications of the ionospheric cusp and the low-latitude boundary layer (LLBL). The radar data for eight cusp events and eight LLBL events have been examined in order to determine a radar signature of these ionospheric regions. This intercalibration indicates that the cusp is always characterized by wide, complex Doppler power spectra, whereas the LLBL is usually found to have spectra dominated by a single component. The distribution of spectral widths in the cusp is of a generally Gaussian form with a peak at about 220 m/s. The distribution of spectral widths in the LLBL is more like an exponential distribution, with the peak of the distribution occurring at about 50 m/s. There are a few cases in the LLBL where the Doppler power spectra are strikingly similar to those observed in the cusp.

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Citations
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Variations in the polar cap area during two substorm cycles

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GPS TEC, scintillation and cycle slips observed at high latitudes during solar minimum

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CUTLASS Finland radar observations of the ionospheric signatures of flux transfer events and the resulting plasma flows

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Characteristics of plasma structuring in the cusp/cleft region at Svalbard

TL;DR: In this article, a study of the distribution and dynamics of mesoscale (tens of kilometers to tens of meters) electron density irregularities in the dayside auroral region was performed at Ny Alesund, Svalbard, by measuring the effects of these irregularities on the amplitude scintillation of 250-MHz transmissions from a quasi-stationary polar satellite as well as the amplitude and phase scintillations of 1.6-GHz signals from Global Positioning System (GPS) satellites.
References
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Journal ArticleDOI

Identification of the magnetospheric cusp and cleft using Pc1–2 ULF pulsations

TL;DR: In this paper, the spatial and temporal distribution of spectral characteristics of the magnetospheric cusp and boundary layer were analyzed using ground riometer, magnetometer and ionosonde measurements.
Journal ArticleDOI

Polar Anglo-American Conjugate Experiment

TL;DR: In this article, a global view of the interactions and coupling between different regions of the magnetosphere and ionosphere is taken, and an important aspect o f this global approach is coordinated investigation of ionospheric processes in both polar regions.
Journal Article

Acceleration/heating of plasma on auroral field lines: preliminary results from the Viking satellite

TL;DR: On presente quelques exemples de populations de plasma accelere ainsi que leurs energies and distributions angulaires as mentioned in this paper, comparees aux theories existantes de chauffage de plasma auroral and de processus d'acceleration.
Journal ArticleDOI

Low‐altitude observations of the conjugate polar cusps

TL;DR: In this article, a set of 118 pairs of nearly simultaneous polar cusp observations over opposite hemispheres, taken by two identically instrumented satellites on orbits that are very close to each other, is used to determine the morphology of the conjugate polar cusps.
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