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Journal ArticleDOI

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

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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Journal ArticleDOI

Cusp and LLBL as sources of the isolated dayside auroral feature during northward IMF

TL;DR: An intense dayside proton aurora was observed by Imager for Magnetopause-to-Aurora Global Exploration Far Ultra-Violet imager (IMAGE FUV) for an extensive period of northward interplanetary magnetic field (IMF) on 17 and 18 September 2000.
Journal ArticleDOI

Do the dayside cusps blink

TL;DR: The polar cusp is a region of the ionosphere for which magnetosheath plasma can be observed as mentioned in this paper, and the low-altitude particle cusp region is the region of ionosphere that can be seen from the Earth's magnetic field.
Dissertation

Les échelles de la turbulence dans l'ionosphère des hautes latitudes et leurs signatures sur les échos des radars HF du réseau SuperDARN

Abstract: SuperDARN est un reseau de radars HF coherents dedie a l'etude de la convection du plasma ionospherique a haute latitude qui trouve ses principales applications dans l'etude des relations Soleil/Terre. On s'interesse ici aux effets des interactions entre l'onde radar emise et les gradients d'ionisation de differentes echelles et a leur impact sur la mesure. Des etudes sont menees pour detecter la signature du mouvement cyclotron des ions, superpose aux mouvements turbulents, dans les spectres mesures. Ensuite, l'effet des moyennes echelles (100 m a 10 km) est mis en evidence sur la mesure des largeurs spectrales. Des etudes statistiques montrent que la determination des parametres est affectee par le rapport entre la frequence emise et la frequence plasma et par la distance de l'echo. Nous proposons une interpretation en terme de decorrelation du front d'onde au cours de la propagation, validee par la mise en place de simulations s'appuyant sur des parametres realistes de l'ionosphere.
Journal ArticleDOI

Initial development of HF radar polar patch caused by azimuthal flow burst in the cusp

TL;DR: In this article, the authors investigated the relationship between the initial development of a poleward propagating feature of the radar backscatter and a fast azimuthal flow in the cusp.
Journal ArticleDOI

Transient production of F-region irregularities associated with TCV passage

TL;DR: In this paper, the authors investigated the transient production of F-region plasma irregularities due to traveling convection vortices (TCVs) using the Super Dual Auroral Radar Network (SuperDARN) combined with ground magnetometer networks and the POLAR ultraviolet imager.
References
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Journal ArticleDOI

DARN/SUPERDARN : A global view of the dynamics of high-latitude convection

TL;DR: The Dual Auroral Radar Network (DARN) is a global-scale network of HF and VHF radars capable of sensing backscatter from ionospheric irregularities in the E and F-regions of the high-latitude ionosphere as mentioned in this paper.
Journal ArticleDOI

A new magnetic coordinate system for conjugate studies at high latitudes

TL;DR: In this article, the authors presented a variation on the corrected geomagnetic coordinate system that is well defined and smooth over the entire globe, and provided an analytic expression relating geographic coordinates, including altitude, to the magnetic coordinates.
Journal ArticleDOI

The frontside boundary layer of the magnetosphere and the problem of reconnection

TL;DR: In this article, Heos 2 plasma and magnetic field data obtained in the frontside boundary layers of the magnetosphere are presented, revealing that the low-latitude extension of the entry layer is of a somewhat different nature.
Journal ArticleDOI

The cusp and the cleft/boundary layer: Low-altitude identification and statistical local time variation

TL;DR: In this paper, the authors investigated the distinction between the low-altitude cusp and the cleft (with the latter identified as the ionospheric signature of low-latitude boundary layer (LLBL)) on both a statistical and a case study basis.
Journal ArticleDOI

Mapping the dayside ionosphere to the magnetosphere according to particle precipitation characteristics

TL;DR: In this article, a complementary approach is tried: regions are identified based on the plasma characteristics as observed by low-altitude satellites using an automated identification scheme applied to approximately 60,000 individual satellite passes through the dayside oval, probability maps are computed for observing various types of plasma precipitating into the ionosphere.
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