The author attempts a brief summary of the history of ionospheric fadi
ng from sources beyond the upper atmosphere. The concentration is on t
he early studies of scintillation. The first sources used as transmitt
ers were radio stars with varying diameters. With the advent of satell
ite transmissions at altitudes varying from 300 km to several earth ra
dii, fading was studied as a function of various regions of the globe.
In years of high solar flux, trans-ionospheric propagation through po
lar and equatorial regions has experienced deep fading at frequencies
ranging from 54 MHz to 4 GHz. Fading of radio signals from satellites
still plays a role in evaluating operational and proposed system effec
tiveness. The relevance of these studies to Global Positioning System
reception and users of proposed systems at L band is discussed.