ANGELS DON‘T PLAY THIS HAARP Advances in Tesla Technology

Chapter Five
HIGH ON THE SKY
Countless suns in other galaxies spray cosmic rays in all directions continuously. Closer
to home, our own sun radiates gamma rays, X-rays and shorter wavelengths of ultraviolet
light. When they hit the outer layers of earth‘s atmosphere, these cosmic rays are absorbed
by atoms, but in the process electrons are knocked off the atoms. Thus there is a constant
flux (flow) of electrons at this altitude, and the atoms are changed to positively charged ions.
This process gave the ionosphere its name. Although ionization happens at heights as
high above the earth as 1,000 kilometers and as low as 50, the positively charged ions and
negative electrons are most dense at altitudes of 80 to 400 kilometers. In non-metric terms,
the ionosphere begins at an altitude of about 30 miles and goes up to about 300 miles or
more.
This natural electrically charged shield around the earth filters harmful wavelengths of
solar radiation, protecting the surface of Earth from significant bombardment.
Blown toward Earth on the solar wind, electrically charged particles follow Earth‘s
magnetic field lines. Along such paths of least resistance, high energy particles funnel toward
the magnetic poles of Earth, squeeze into a pole-ward current called the electrojet, and are
dumped toward the earth. Sometimes the electrojet dwindles, but at other times a solar flare
floods the system with high energy particles and the sky lights up into the dancing, shifting
curtains of an auroral display. At the south pole it is called the aurora australis, and the
northern lights is the aurora borealis.
For eons the electrojet has flowed in the form of a direct current into the polar regions of
Earth. Who would want to change the electrojet?
THE PATH TO A GIGA PROJECT
In a way it began with a few puzzled radio listeners. In 1933 a man in Eindhoven, Holland
tried to listen to a radio station in Beromunster, Switzerland. Suddenly he was hearing two
stations. The powerful Radio Luxembourg was not supposed to tune in at this frequency; it
broadcast at a frequency far apart on the dial, but here it was superimposed on the Swiss
station.
The Luxembourg Effect, as it was later called, did not remain a mystery long. The Dutch
scientist named Tellegen figured out that the cross modulation of the radio signals was a
wave interaction caused by nonlinear characteristics of the ionosphere. What this means to
non-scientists is that reactions of the ionosphere are unpredictable.
Then other scientists also realized that high power radio waves changed the temperature
and density of electrons in the ionosphere and that other radio signals passing through the
―modified‖ region were influenced. They experimented with wave interaction for thirty years
and eventually were certain that directing high power waves into the ionosphere produced
instabilities.
Their tool was a transmitter – array of antennae - called an ionospheric heater. (Press
releases now refer to it as an Ionospheric Research Instrument, but this book will call a
heater a heater.) For the most part, ionospheric heaters were operated by universities and
research institutes. Stanford Research Institute (SRI) International developed much of the
high frequency transmitting programs with money from the Defense Nuclear Agency.
The newest, multi-purpose, tool being built for HAARP, however, is directed from
Phillips Air Force Base.