[1] Following an earlier polarization study for a well-defined man-made very high frequency (VHF) signal by using the two orthogonally oriented, linear polarization antennas aboard the FORTE satellite, we report in this paper similar polarization observations for lightning-produced radiation. A selected group of 313 transionospheric pulse pairs (TIPPs) that were geolocated by the National Lightning Detection Network (NLDN) has been analyzed. The TIPPs have been examined with high time resolution so that the magnetoionic modes can be resolved. Most of the TIPPs have been found highly polarized, with 40 % of them far above the background polarization level. The polarization ellipticity and the orientation of the ellipse of the split modes hav...
We present polarization data for 32 mainly southern pulsars at 8.4 GHz. The observations show that t...
The Solar Corona is a teneous medium of magnetized plasma with an inherent distribution of number de...
It is now established that auroral emissions as measured from the ground are polarised. The question...
Very Low Frequency (VLF, 3-30 kHz) transmitter remote sensing has long been used as a simple yet use...
Plasma wave measurements from the DE 1 (Dynamics Explorer 1) spacecraft are used to determine the po...
The Radio Receiver Instrument (RRI) of the Swarm-E/e-POP satellite can determine the polarization st...
This work compares contemporaneous observations of lightning from two highly complementary systems. ...
Abstract Auroral medium frequency burst (MFB) is a radio emission of natural auroral origin associat...
Schumann resonance waveforms in the lower ELF band are produced by distant lightning discharges. T...
International audienceWe report here on the temporal and spatial evolution of the impact polarizatio...
Abstract—We show images of propagation spectrograms based on spacecraft observations of electromagne...
International audienceEarly in 2006 the RPWS (Radio and Plasma Wave Science) instrument and the ISS ...
International audience[1] We use a comprehensive analysis of 6-component ELF wave data from the DEME...
Polarization and direction of arrival of VLF emissions have been observed at Syowa Station in the An...
We present polarization data for 32 mainly southern pulsars at 8.4 GHz. The observations show that t...
The Solar Corona is a teneous medium of magnetized plasma with an inherent distribution of number de...
It is now established that auroral emissions as measured from the ground are polarised. The question...
Very Low Frequency (VLF, 3-30 kHz) transmitter remote sensing has long been used as a simple yet use...
Plasma wave measurements from the DE 1 (Dynamics Explorer 1) spacecraft are used to determine the po...
The Radio Receiver Instrument (RRI) of the Swarm-E/e-POP satellite can determine the polarization st...
This work compares contemporaneous observations of lightning from two highly complementary systems. ...
Abstract Auroral medium frequency burst (MFB) is a radio emission of natural auroral origin associat...
Schumann resonance waveforms in the lower ELF band are produced by distant lightning discharges. T...
International audienceWe report here on the temporal and spatial evolution of the impact polarizatio...
Abstract—We show images of propagation spectrograms based on spacecraft observations of electromagne...
International audienceEarly in 2006 the RPWS (Radio and Plasma Wave Science) instrument and the ISS ...
International audience[1] We use a comprehensive analysis of 6-component ELF wave data from the DEME...
Polarization and direction of arrival of VLF emissions have been observed at Syowa Station in the An...
We present polarization data for 32 mainly southern pulsars at 8.4 GHz. The observations show that t...
The Solar Corona is a teneous medium of magnetized plasma with an inherent distribution of number de...
It is now established that auroral emissions as measured from the ground are polarised. The question...