A method of extrapolating electron densities (N-e) from Incoherent Scatter
Radar (ISR) data to high altitudes is presented, and is used to estimate th
e vertical Total Electron Content (TEC) over Arecibo, Although primarily in
tended for use on the N-e profiles obtained using the new topside frequency
hopping mode at Arecibo which provides measurements to over 2000 km altitu
de, we show that if the O+-H+ transition altitude is low enough to be obser
ved, then the method may also be applied to the data taken using the standa
rd World Day multi-radar mode, and thus to a great fraction of the World Da
y data from low solar flux conditions. This method is applied to Arecibo IS
R data taken during the January 6-11 1997 CEDAR storm period, and compared
with measured TEC from the Global Positioning System (GPS) satellite networ
k. In addition, the TEC is compared to TEC calculated from the Sheffield Un
iversity Plasmasphere Ionosphere Model (SUPIM) as part of an ongoing projec
t of model validation.