Page 31 - Elana Freeland - Under an Ionized Sky

But then, there may be blowback chalked up to “climate change”:

It’s as if global warming were ringing the Earth’s atmosphere like some great, cacophonous alarm bell. The upper
level zonal winds are swinging wildly from record high positive anomalies to record low negative anomalies. . .And
the Jet Stream now has redefined all boundaries—flowing at times from the East Siberian Sea in the Arctic across the
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Equator and all the way south to West Antarctica.

Today, we can count more than 260 SDI-inspired installations around the world, all engaged,
to one degree or another, in ULF/ELF modulation and manipulation of the ionospheric
fluctuation known as the auroral jet (electrojet), where the Van Allen Radiation Belts—the shell
of our magnetosphere—intersect our atmosphere. Even before Project Cloverleaf was activated
and HAARP built, a network of ionospheric heaters already existed.
The first ionospheric heaters like the Arecibo Radio Telescope (“The Pit”) in Puerto Rico
(1963), the Platteville Atmospheric Observatory in Platteville, Colorado, and EISCAT (European
Incoherent Scatter Scientific Association) in Tromsø, Norway (1981) initially concentrated on
interfering high-frequency radio waves for earth-penetrating tomography. The Pit is still the
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largest dish antenna in the world with three radar transmitters with an ERP of 20 TW at
2380MHz, 2.5 TW (pulse peak) at 430MHz, and 300MW at 47MHz.
Just before HAARP was shut down in summer 2013, the Pit ionospheric heater was
upgraded:

“It is basically the same as HAARP for the science, except that HAARP was in the Auroral Region, where the physics
of the ionosphere is quite different with all the energetic particles and magnetic fields,” Penn State Electrical
Engineering Professor Jim Breakall, WA3FET, told ARRL. . .The National Science Foundation and Cornell
University, which previously operated Arecibo Observatory, contracted with Penn State’s Electrical Engineering
Department to construct the “new and enhanced” HF ionospheric instrument. It will be used to study the interaction
between HF radio energy and ionospheric plasma. 11

The Platteville Observatory supposedly shut down in 1984 and is now being used for “wind
profiling.” EISCAT oversees three incoherent scatter radar systems at 224MHz and 931MHz in
Northern Scandinavia, and one at 500MHz at EISCAT Space Centre in Svalbard. Additional
receiver stations are located in Sodankylä, Finland and Kiruna, Sweden, transmitting 10MW
with an antenna gain of 35 decibels (dB) producing an ERP of 32 billion watts. EISCAT is
funded and operated by research institutes and councils of Norway, Sweden, Finland, Japan,
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China, the UK, France, and Germany, and has recently been recalibrated to serve lower-earth
orbit (LEO) Space Fence surveillance.
As for how ionospheric heaters work, picture focused radio waves generated by phased-array
radar units striking a targeted area in the ionosphere to ionize (heat) electrons. HAARP’s
ionospheric research instrument (IRI) was constructed with 180 antenna towers in a grid of
fifteen columns and twelve rows, with two dipole antennas atop each tower. Beneath the array
are transmitter shelters, each housing twelve diesel-powered transmitters capable of generating
10,000 watts of RF power each with an ability to focus 3.6 billion watts on a single point.
Steering this focus and its pulse transmission agility constitutes the secret power of HAARP,
according to Eastlund.
Once the electrons in the ionosphere are ionized, they twirl down the magnetic lines of force
conjoining with Birkeland currents, ready to be steered by various radar instruments for a variety
of military-industrial-intelligence C4 operations (command, control, communications, and
cyberwarfare), including moving and enhancing weather systems, stimulating seismic plates to