Observations made using the LOw-Frequency ARray (LOFAR) between 10:15 and 11:48 UT on the 15th of September 2018 over a bandwidth of approximately 25–65 MHz contain discrete pseudo-periodic features of ionospheric origin. These features occur within a period of approximately 10 min and collectively last roughly an hour. They are strongly frequency dependent, broadening significantly in time towards the lower frequencies, and show an overlaid pattern of diffraction fringes. By modelling the ionosphere as a thin phase screen containing a wave-like disturbance, we are able to replicate the observations, suggesting that they are associated with small-scale travelling ionospheric disturbances (TIDs). This modelling indicates that the features ob...
Context. There are a number of hardware upgrades for the Low-Frequency Array (LOFAR) currently under...
In this article we present results from very low frequency (VLF) observations of transient and inter...
To obtain high quality images with the Lofar low frequency radio telescope, accurate ionospheric cha...
Observations made using the LOw-Frequency ARray (LOFAR) between 10:15 and 11:48 UT on the 15th of Se...
LOFAR is the LOw-Frequency Radio interferometer ARray located at midlatitude (52°53'N). Here we pres...
The Earth’s ionosphere is a highly variable medium on a wide range of spatio-temporal scales. The re...
This paper presents the results from one of the first observations of ionospheric scintillation take...
The Low Frequency Array (LOFAR) is designed to observe the early universe at radio wavelengths. When...
LOFAR is the LOw-Frequency Radio interferometer ARray located at midlatitude (52°53′N). Here we pres...
Context. The ionosphere is the main driver of a series of systematic effects that limit our ability ...
Ionospheric scintillations of radio waves at low-latitudes are associated with electron density ...
Inhomogeneities within the ionospheric plasma density affect trans-ionospheric radio signals, causin...
Context. There are a number of hardware upgrades for the Low-Frequency Array (LOFAR) currently under...
In this article we present results from very low frequency (VLF) observations of transient and inter...
To obtain high quality images with the Lofar low frequency radio telescope, accurate ionospheric cha...
Observations made using the LOw-Frequency ARray (LOFAR) between 10:15 and 11:48 UT on the 15th of Se...
LOFAR is the LOw-Frequency Radio interferometer ARray located at midlatitude (52°53'N). Here we pres...
The Earth’s ionosphere is a highly variable medium on a wide range of spatio-temporal scales. The re...
This paper presents the results from one of the first observations of ionospheric scintillation take...
The Low Frequency Array (LOFAR) is designed to observe the early universe at radio wavelengths. When...
LOFAR is the LOw-Frequency Radio interferometer ARray located at midlatitude (52°53′N). Here we pres...
Context. The ionosphere is the main driver of a series of systematic effects that limit our ability ...
Ionospheric scintillations of radio waves at low-latitudes are associated with electron density ...
Inhomogeneities within the ionospheric plasma density affect trans-ionospheric radio signals, causin...
Context. There are a number of hardware upgrades for the Low-Frequency Array (LOFAR) currently under...
In this article we present results from very low frequency (VLF) observations of transient and inter...
To obtain high quality images with the Lofar low frequency radio telescope, accurate ionospheric cha...