The Quasi-periodic pulsing hiss emissions observed during daytime in the frequency range of 50 Hz – 15 kHz at low latitude station Jammu (geomag. Lat. = 220 26 / N; L = 1.17) has been reported. It is noted that pulsing VLF emissions is a rare phenomena at low latitudes. The spectrograms clearly show band limited spectrum regularly pulsing with almost equal period of the order of a fraction of a second in the frequency band 2.6 to 6.8 kHz. Generation and propagation mechanism of these emissions are briefly discussed. 1
133-135Intensity calculations are done in a realistic ionospheric model for ground-observed low lati...
During the analysis of archived VLF data from Indian low latitude ground stations, some discrete VLF...
Abstract Using numerical filtering techniques allowing us to reduce noise from sferics, we are able...
This paper reports quasi-periodic pulsing hiss emissions recorded during daytime in the frequency ra...
Abstract The new type of daytime natural very low frequency (VLF) whistler mode emissions of the ma...
209-210Successful recording of different types of whistlers as also the VLF hiss at a low latitude g...
Abstract Very low frequency (VLF) emissions of natural origin were identified for the first time by...
Abstract. A detailed analysis of the VLF emissions data obtained during occasional whistler campaign...
70-74The ground based VLF database from Indian Antarctic station Maitri (70o 46ʹ S, 11o 44ʹ E, L ~ ...
Recent topics of VLF observations at Syowa Station, Antarctica, are summarized. In the frequency-tim...
VLF emissions were observed at Syowa Station by the 11th wintering party of the Japanese Antarctic R...
The characteristic features of VLF hiss emissions during quiet and disturbed conditions observed at ...
36-37By assuming source location at low altitudes in the equatorial plane, ray-tracing computations ...
International audienceDEMETER was a low-altitude satellite in operation between 2004 and 2010 in a c...
24-30The morphological features of VLF hiss observed at the auroral and low latitude stations are ...
133-135Intensity calculations are done in a realistic ionospheric model for ground-observed low lati...
During the analysis of archived VLF data from Indian low latitude ground stations, some discrete VLF...
Abstract Using numerical filtering techniques allowing us to reduce noise from sferics, we are able...
This paper reports quasi-periodic pulsing hiss emissions recorded during daytime in the frequency ra...
Abstract The new type of daytime natural very low frequency (VLF) whistler mode emissions of the ma...
209-210Successful recording of different types of whistlers as also the VLF hiss at a low latitude g...
Abstract Very low frequency (VLF) emissions of natural origin were identified for the first time by...
Abstract. A detailed analysis of the VLF emissions data obtained during occasional whistler campaign...
70-74The ground based VLF database from Indian Antarctic station Maitri (70o 46ʹ S, 11o 44ʹ E, L ~ ...
Recent topics of VLF observations at Syowa Station, Antarctica, are summarized. In the frequency-tim...
VLF emissions were observed at Syowa Station by the 11th wintering party of the Japanese Antarctic R...
The characteristic features of VLF hiss emissions during quiet and disturbed conditions observed at ...
36-37By assuming source location at low altitudes in the equatorial plane, ray-tracing computations ...
International audienceDEMETER was a low-altitude satellite in operation between 2004 and 2010 in a c...
24-30The morphological features of VLF hiss observed at the auroral and low latitude stations are ...
133-135Intensity calculations are done in a realistic ionospheric model for ground-observed low lati...
During the analysis of archived VLF data from Indian low latitude ground stations, some discrete VLF...
Abstract Using numerical filtering techniques allowing us to reduce noise from sferics, we are able...