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  • Haldoupis, C.  (11)
  • 1
    Online Resource
    Online Resource
    Copernicus GmbH ; 2003
    In:  Annales Geophysicae Vol. 21, No. 7 ( 2003-07-31), p. 1589-1600
    In: Annales Geophysicae, Copernicus GmbH, Vol. 21, No. 7 ( 2003-07-31), p. 1589-1600
    Abstract: Abstract. In this paper we describe the conversion of SESCAT (Sporadic-E SCATter experiment), a bistatic 50 MHz continuous wave (CW) Doppler radar located on the island of Crete, Greece, to a single (east-west) baseline interferometer. The first results show that SESCAT, which provides high quality Doppler spectra and excellent temporal resolution, has its measurement capabilities enhanced significantly when operated as an interferometer, as it can also study short-term dynamics of localized scattering regions within mid-latitude sporadic E-layers. The interferometric observations reveal that the aspect sensitive area viewed by the radar often contains a few zonally located backscatter regions, presumably blobs or patches of unstable metallic ion plasma, which drift across the radar field-of-view with the neutral wind. On average, these active regions of backscatter have mean zonal scales ranging from a few kilometers to several tens of kilometers and drift with westward speeds from ~ 20 m/s to 100 m/s, and occasionally up to 150 m/s. The cross-spectral analysis shows that mid-latitude type 1 echoes occur much more frequently than has been previously assumed and they originate in single and rather localized areas of elevated electric fields. On the other hand, typical bursts of type 2 echoes are often found to result from two adjacent regions in azimuth undergoing the same bulk motion westwards but producing scatter of opposite Doppler polarity, a fact that contradicts the notion of isotropic turbulence to which type 2 echoes are attributed. Finally, quasi-periodic (QP) echoes are observed simply to be due to sequential unstable plasma patches or blobs which traverse across the radar field-of-view, sometimes in a wave-like fashion.Key words. Ionosphere (ionospheric irregularities; mid-latitude ionosphere; plasma waves and instabilities)
    Type of Medium: Online Resource
    ISSN: 1432-0576
    Language: English
    Publisher: Copernicus GmbH
    Publication Date: 2003
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  • 2
    Online Resource
    Online Resource
    Elsevier BV ; 2006
    In:  Journal of Atmospheric and Solar-Terrestrial Physics Vol. 68, No. 3-5 ( 2006-2), p. 539-557
    In: Journal of Atmospheric and Solar-Terrestrial Physics, Elsevier BV, Vol. 68, No. 3-5 ( 2006-2), p. 539-557
    Type of Medium: Online Resource
    ISSN: 1364-6826
    RVK:
    Language: English
    Publisher: Elsevier BV
    Publication Date: 2006
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  • 3
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 1999
    In:  Journal of Geophysical Research: Space Physics Vol. 104, No. A5 ( 1999-05-01), p. 10071-10080
    In: Journal of Geophysical Research: Space Physics, American Geophysical Union (AGU), Vol. 104, No. A5 ( 1999-05-01), p. 10071-10080
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 1999
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  • 4
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 1998
    In:  Journal of Geophysical Research: Space Physics Vol. 103, No. A6 ( 1998-06), p. 11605-11615
    In: Journal of Geophysical Research: Space Physics, American Geophysical Union (AGU), Vol. 103, No. A6 ( 1998-06), p. 11605-11615
    Abstract: We use observations from a high‐frequency Doppler radar experiment at midlatitudes to study the wavelength dependence of spectrum broadening of backscatter from field‐aligned E region irregularities. The radar made multifrequency measurements of high‐resolution Doppler spectra simultaneously at four frequencies, that is, 9.23, 11.03, 12.71, and 16.09 MHz, which correspond to backscatter from irregularities with wavelengths of 16.3, 13.6, 11.8, and 9.3 m, respectively. In the analysis we deal with secondary irregularities (type 2 echoes) characterized by small mean velocities that show no dependence on radar frequency and have mean spectrum width to velocity ratios well above unity. The spectrum width is found to increase monotonically with wavenumber k in the range from 0.38 to 0.67 m −1 covered in the experiment. By postulating that the width is determined mainly by the nonlinear growth rate of the secondary short‐scale plasma turbulence, we compare the results to the Sudan [1983] theory. Although there is some general agreement, on the average, the measured mean spectrum width follows approximately a k 4/3 power law dependence which is considerably stronger than the theoretical k 2/3 dependence. This discrepancy may be reduced somewhat but cannot be fully accounted for when additional spectrum broadening effects caused by the irregularity velocity distribution are also included.
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 1998
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  • 5
    Online Resource
    Online Resource
    Copernicus GmbH ; 2004
    In:  Annales Geophysicae Vol. 22, No. 11 ( 2004-11-29), p. 3789-3798
    In: Annales Geophysicae, Copernicus GmbH, Vol. 22, No. 11 ( 2004-11-29), p. 3789-3798
    Abstract: Abstract. In the mid-latitude E-region there is now evidence suggesting that neutral winds play a significant role in driving the local plasma instabilities and electrodynamics inside sporadicE layers. Neutral winds can be inferred from coherent radar backscatter measurements of the range-/azimuth-time-intensity (RTI/ATI) striations of quasi-periodic (QP) echoes, or from radar interferometer/imaging observations. In addition, neutral winds in the E-region can be estimated from angle-of-arrival ionosonde measurements of sporadic-E layers. In the present paper we analyse concurrent ionosonde and HF coherent backscatter observations obtained when a Canadian Advanced Digital Ionosonde (CADI) was operated under a portion of the field-of-view of the Valensole high frequency (HF) radar. The Valensole radar, a mid-latitude radar located in the south of France with a large azimuthal scanning capability of 82° (24° E to 58° W), was used to deduce zonal bulk motions of QP echoing regions using ATI analysis. The CADI was used to measure angle-of-arrival information in two orthogonal horizontal directions and thus derive the motion of sporadic-E patches drifting with the neutral wind. This paper compares the neutral wind drifts of the unstable sporadic-E patches as determined by the two instruments. The CADI measurements show a predominantly westward aligned motion, but the measured zonal drifts are underestimated relative to those observed with the Valensole radar.
    Type of Medium: Online Resource
    ISSN: 1432-0576
    Language: English
    Publisher: Copernicus GmbH
    Publication Date: 2004
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  • 6
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 1996
    In:  Journal of Geophysical Research: Space Physics Vol. 101, No. A4 ( 1996-04), p. 7961-7971
    In: Journal of Geophysical Research: Space Physics, American Geophysical Union (AGU), Vol. 101, No. A4 ( 1996-04), p. 7961-7971
    Abstract: We present results from a dual‐frequency ionospheric backscatter experiment carried out with the Valensole HF radar facility in the south of France. The radar was operated in a mode that allowed detailed Doppler spectrum recordings of coherent echoes from midlatitude E region irregularities simultaneously at 9.0 MHz and 12.4 MHz, corresponding to aspect‐sensitive backscatter from plasma waves with 16.7‐m and 12.1‐m wavelength, respectively. In this decameter wave band and in the presence of intense nighttime sporadic E s layers that contribute strong destabilizing density gradient components perpendicular to B, the E region is susceptible to direct plasma wave generation by the gradient drift instability even if electric fields are only a few mV/m. We observe that 9.0‐MHz echoes are stronger, more frequent, and more spatially extended than the 12.4‐MHz ones, which is in line with the threshold requirements of the gradient drift instability. Further, the data supports the notion of primary and secondary waves with spectral shapes similar to those seen, for example, at the equator. In one case, a situation analogous to the equatorial electrojet was clearly seen, in which the Doppler spectrum changed from a negatively shifted narrow peak (type I‐like) to a broad type II near zero shift and then to a positively shifted narrow type I‐like component, in the radar's azimuthal sector span from 22° east to 38° west of geomagnetic north. We have studied the ratio of the observed 12.4‐MHz versus 9.0‐MHz Doppler velocities in an attempt to test the widely used hypothesis that primary gradient drift waves have their phase velocity limited at instability threshold values. For simultaneous velocities in the range from 40 to 120 m/s, the V 12.1 m / V 16.7 m ratio was found on the average close to 1.1 and thus quite small compared to the anticipated value of 1.6 if the waves were to propagate at instability threshold values. Instead, the evidence is more supportive of the theory's dispersion relationship which requires that the wave phase velocity matches the relative electron‐ion drift along the direction of propagation.
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 1996
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  • 7
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 1995
    In:  Journal of Geophysical Research: Space Physics Vol. 100, No. A11 ( 1995-11), p. 21503-21521
    In: Journal of Geophysical Research: Space Physics, American Geophysical Union (AGU), Vol. 100, No. A11 ( 1995-11), p. 21503-21521
    Abstract: In this paper, an experiment designed for dual‐frequency azimuthal Doppler spectrum studies of decameter‐scale field‐aligned irregularities in the midlatitude E region ionosphere is introduced, and the first results are presented. The observations were made in July 1993 with a large HF radar facility near Valensole (43.8°N, 6.1°E), in the south of France. The radar system is an oblique ionospheric sounder that employes long antenna arrays of vertical monopole pairs and covers the HF frequency band from 4 to 30 MHz in 1‐kHz steps. A scheme of broad beam width transmission and narrow‐beam, phased‐array, multireceiver coverage was used to scan with 2° step an azimuthal sector from about 24° east to 60° west of geomagnetic north. The 15‐gate viewing region was confined in range between 100 and 370 km in order to cover an area of E region magnetic aspect sensitive backscatter near 37° invariant magnetic latitude ( L ≃ 1.7, magnetic dip, ∼60°). In this configuration, each azimuthal scan was completed in 80 s over a 15×42 spatial grid with the full Doppler spectrum at each grid point recorded in real time. The experiment provided observations simultaneously at two frequencies, 9.0 MHz and 14.8 MHz, that correspond to backscatter from plasma waves with wavelengths of 16.7 and 10.1 m, respectively. Here, we present an overview of the observations that include azimuthal and range‐time echo characteristics as well as mean Doppler shift and spectrum width properties. The first results show aspect sensitive decameter‐wavelength irregularities having mean phase velocities at least as large as 120 m/s to act as tracers of wavelike dynamic structures that drift westward with speeds in the 40‐ to 80‐m/s range and have characteristic times between 10 and 30 min and typical scale lenghts between 40 and 90 km. In our interpretation, we consider these structures to be sporadic E s ionization patches, possibly affected by the passage of atmospheric gravity waves, which are accompanied by intense horizontal electron density gradients and enhanced electric fields. Although secondary generation cannot be excluded entirely, the evidence supports the possibility that the gradient drift instability is the basic physical mechanism for direct generation of decameter aspect sensitive plasma waves in the midlatitude E region ionosphere.
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 1995
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  • 8
    Online Resource
    Online Resource
    Copernicus GmbH ; 1997
    In:  Annales Geophysicae Vol. 15, No. 7 ( 1997), p. 918-
    In: Annales Geophysicae, Copernicus GmbH, Vol. 15, No. 7 ( 1997), p. 918-
    Type of Medium: Online Resource
    ISSN: 0992-7689
    Language: Unknown
    Publisher: Copernicus GmbH
    Publication Date: 1997
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    SSG: 16,13
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  • 9
    Online Resource
    Online Resource
    Copernicus GmbH ; 1997
    In:  Annales Geophysicae Vol. 15, No. 7 ( 1997-07-31), p. 918-924
    In: Annales Geophysicae, Copernicus GmbH, Vol. 15, No. 7 ( 1997-07-31), p. 918-924
    Abstract: Abstract. In this paper an experiment designed for multifrequency azimuthal Doppler-spectrum investigations of decametre-scale plasma irregularities in the mid-latitude E region is introduced and some preliminary results are presented. The observations were made with the high-frequency Valensole radar in the south of France. The radar operated in a multifrequency mode that allowed simultaneous measurements of Doppler spectra at the four frequencies of 9.23, 11.03, 12.71 and 16.09 MHz, which correspond to scatter from field-aligned irregularities with wavelengths of 16.2, 13.6, 11.8 and 9.3 m, respectively. In addition, a digital ionosonde was operating beneath a small part of the radar viewing region. The data show that lower-frequency echoes are stronger, more frequent and more spatially extended than higher-frequency ones, in general agreement with theory and rocket measurements. On the other hand, the preliminary analysis shows no pronounced differences of the Doppler spectrum with radar frequency. Some trends in the spectral moments do exist, however, which can be understood as the result of temporal and/or spatial mixing of backscatter from directly generated (primary) plasma waves by the gradient drift instability and secondary low-velocity waves. Finally, a close relation of mid-latitude coherent backscatter with patchy sporadic E-layers is present in the data, but the details of this relation remain unresolved.
    Type of Medium: Online Resource
    ISSN: 1432-0576
    Language: English
    Publisher: Copernicus GmbH
    Publication Date: 1997
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  • 10
    Online Resource
    Online Resource
    Copernicus GmbH ; 1997
    In:  Annales Geophysicae Vol. 15, No. 7 ( 1997-07-31), p. 925-934
    In: Annales Geophysicae, Copernicus GmbH, Vol. 15, No. 7 ( 1997-07-31), p. 925-934
    Abstract: Abstract. HF radar observations of mid-latitude spo- radic-E irregularities carried out with the Valensole radar in South France are compared with simultaneous ionosonde measurements underneath the irregularity zones. In a previous study of Valensole radar data, it has been shown that HF backscatter from the night-time mid-latitude E region is usually associated with large- scale wave-like modulations. To obtain more informa- tion on the geophysical conditions prevailing during backscatter events, a new experiment was performed which also included a vertical ionosonde beneath the scattering region. The data to be presented here are from two periods when radar scattering appeared simulta- neously with large variations in the virtual height and the Doppler velocity of F-layer re¯ected echoes mea- sured with the vertical ionosonde, indicating very clearly the passage of atmospheric gravity waves (AGWs). The e.ect of the atmospheric waves on the sporadic-E layer is not always as marked as it is in the F region. In the ®rst event, the passage of the AGWs is accompanied by an upward followed by a downward movement of the Es-layer. The apparent descending movement of the Es-layer from 135 to 110 km in less than 10 min corresponded to a positive (downward) Doppler velocity of 35 m/s measured by the vertical ionosonde, and was accompanied by a range variation in the radar scattering region with a negative rate of about 90±110 m/s. In the second event, the Es-layer is not as strongly disturbed as in the previous one, but, nevertheless, the range varia- tions of the scattering region can still be associated with height ¯uctuations of the Es-layer.
    Type of Medium: Online Resource
    ISSN: 1432-0576
    Language: English
    Publisher: Copernicus GmbH
    Publication Date: 1997
    detail.hit.zdb_id: 1458425-6
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