Auroral backscatter radar observations were made from Ithaca, New York, at 50 MHz during the early morning of April 1, 1976, a period of high magnetic disturbance (Kp ∼ 8). The backscattered power showed large rapid (time scale of a few minutes or less) variations, characteristic of discrete radar aurora, from L = 3.5–4. Doppler spectra of waves propagating in nearly the north-south direction from up to 28 different ranges were obtained simultaneously with good spatial (7.5 km) and temporal (2 s) resolution. Some unusual spectra with very narrow peaks at Doppler shifts between about 70 and 90 Hz were observed and were apparently associated with sheared flows of the auroral plasma. These echoes were observed at the southern edge of the scatt...
Incoherent scatter radars are powerful ground based instruments for ionospheric measurements. By ana...
The generation mechanism for naturally enhanced ion-acoustic echoes is still debated. One important ...
Fragmented aurora-like emissions (FAEs) are small (few kilometres) optical structures which have bee...
Radar observations have shown that the phase velocity of small scale (a few meters and smaller) auro...
We have observed 3-m auroral E region plasma waves with a high-resolution 50-MHz radar interferomete...
Multi-frequency observations of E-region coherent backscatter from decametre waves reveal that auror...
Simultaneous all-sky camera and HF radar observations of the visual and E-region radar aurora in t...
Broadband extremely low-frequency wave emissions below the ion plasma frequency have been observed b...
The radar interferometer technique first used at the magnetic equator in Peru is also a very powerfu...
Electromagnetic ion cyclotron (EMIC) waves, one of the possible origins of flickering aurora, have b...
Optical measurements of small-scale auroral structures are here combined with spectrographic data in...
Abstract. The generation mechanism for naturally enhanced ion-acoustic echoes is still debated. One ...
We present results from a coordinated camera and radar study of the auroral ionosphere conducted du...
International audienceBackscatter from E-region irregularities was observed at aspect angles close t...
The Fast Auroral Snapshot Explorer (FAST) satellite detected intense and coherent 5–20 m electric f...
Incoherent scatter radars are powerful ground based instruments for ionospheric measurements. By ana...
The generation mechanism for naturally enhanced ion-acoustic echoes is still debated. One important ...
Fragmented aurora-like emissions (FAEs) are small (few kilometres) optical structures which have bee...
Radar observations have shown that the phase velocity of small scale (a few meters and smaller) auro...
We have observed 3-m auroral E region plasma waves with a high-resolution 50-MHz radar interferomete...
Multi-frequency observations of E-region coherent backscatter from decametre waves reveal that auror...
Simultaneous all-sky camera and HF radar observations of the visual and E-region radar aurora in t...
Broadband extremely low-frequency wave emissions below the ion plasma frequency have been observed b...
The radar interferometer technique first used at the magnetic equator in Peru is also a very powerfu...
Electromagnetic ion cyclotron (EMIC) waves, one of the possible origins of flickering aurora, have b...
Optical measurements of small-scale auroral structures are here combined with spectrographic data in...
Abstract. The generation mechanism for naturally enhanced ion-acoustic echoes is still debated. One ...
We present results from a coordinated camera and radar study of the auroral ionosphere conducted du...
International audienceBackscatter from E-region irregularities was observed at aspect angles close t...
The Fast Auroral Snapshot Explorer (FAST) satellite detected intense and coherent 5–20 m electric f...
Incoherent scatter radars are powerful ground based instruments for ionospheric measurements. By ana...
The generation mechanism for naturally enhanced ion-acoustic echoes is still debated. One important ...
Fragmented aurora-like emissions (FAEs) are small (few kilometres) optical structures which have bee...