132-134Electron concentration profiles during sunrise and sunset periods, observed with the Arecibo incoherent scatter radar, are presented. The measurements are made in the height range of 100-500 km, using short pulses resulting in a height resolution of 15 km. Electron concentrations are observed to change by more than an order of magnitude during these periods in the height range of 120-200 km. The changes are rather small in the Es and in the F2 region and thus a large valley is developed between 100 and 200 km, with a minimum of electron concentration at about 140 km. The fast decay of electron concentration during sunset is used to estimate the effective recombination coefficient which is then compared with the experimental values
The daytime measurements of electron temperature (Te) and concentration (Ne) from incoherent scatter...
159-161Incoherent scatter radar measurements of electron temperature (Te) and electron concentration...
193-194The variation of the effective collision frequency of electrons veff with solar zenith angle ...
Results of continuous measurements of nighttime electron concentration profiles, using short pulses ...
The topside electron density profiles for sunrise and sunset conditions measured with incoherent sca...
Earth’s lower ionosphere is the region where terrestrial weather and space weather come together. He...
Results of electron content and equivalent slab thickness obtained from radar backscatter measuremen...
In the years 1974 to 1977 the incoherent-scatter radar at Arecibo made high resolution measurements ...
The size and shape of the valley region between E and F layers is studied for nighttime conditions b...
High resolution electron density profiles, measured with the Arecibo incoherent scatter radar have b...
Incoherent scatter radar data from Arecibo, for high solar activity (HSA) (1989-1990) as well as for...
Incoherent backscatter measurements of the F-region electron concentrations and electron and ion tem...
Observations by incoherent-scatter radar have been applied to explore relationships between the flu...
251-256The daytime measurements of electron temperature (Te) and concentration (Ne) from incoherent ...
About 1500 electron density (Ne) profiles observed with the Arecibo incoherent scatter (I.S.) radar ...
The daytime measurements of electron temperature (Te) and concentration (Ne) from incoherent scatter...
159-161Incoherent scatter radar measurements of electron temperature (Te) and electron concentration...
193-194The variation of the effective collision frequency of electrons veff with solar zenith angle ...
Results of continuous measurements of nighttime electron concentration profiles, using short pulses ...
The topside electron density profiles for sunrise and sunset conditions measured with incoherent sca...
Earth’s lower ionosphere is the region where terrestrial weather and space weather come together. He...
Results of electron content and equivalent slab thickness obtained from radar backscatter measuremen...
In the years 1974 to 1977 the incoherent-scatter radar at Arecibo made high resolution measurements ...
The size and shape of the valley region between E and F layers is studied for nighttime conditions b...
High resolution electron density profiles, measured with the Arecibo incoherent scatter radar have b...
Incoherent scatter radar data from Arecibo, for high solar activity (HSA) (1989-1990) as well as for...
Incoherent backscatter measurements of the F-region electron concentrations and electron and ion tem...
Observations by incoherent-scatter radar have been applied to explore relationships between the flu...
251-256The daytime measurements of electron temperature (Te) and concentration (Ne) from incoherent ...
About 1500 electron density (Ne) profiles observed with the Arecibo incoherent scatter (I.S.) radar ...
The daytime measurements of electron temperature (Te) and concentration (Ne) from incoherent scatter...
159-161Incoherent scatter radar measurements of electron temperature (Te) and electron concentration...
193-194The variation of the effective collision frequency of electrons veff with solar zenith angle ...