Added: Jul 20, 2008
From: BackwardsFuture
Duration: 9:46
HAARP(High Frequency Active Auroral Research Program) The project site ( [show location on an interactive map] 62°23'30?N, 145°09'03?W) is north of Gakona, Alaska, just West of the Wrangell-Saint Elias National Park. An environmental impact statement led to permission for an array of up to 180 antennas to be erected. The HAARP has been constructed at the previous site of an over-the-horizon radar installation. A large structure, built to house the OTH now houses the HAARP control room, kitchen, and offices. Several other small structures house various instruments. The Ionospheric Research Instrument (IRI) is the primary instrument at HAARP, which is a high-frequency (HF) transmitter system used to temporarily modify the ionosphere. Study of this modified volume yields important information for understanding natural ionospheric processes. During active ionospheric research, the signal generated by the transmitter system is delivered to the antenna array, transmitted in an upward direction, and is partially absorbed, at an altitude between 100 to 350 km (depending on operating frequency), in a small volume a few hundred meters thick and a few tens of kilometers in diameter over the site. The intensity of the HF signal in the ionosphere is less than 3 µW/cm², tens of thousands of times less than the Sun's natural electromagnetic radiation reaching the earth and hundreds of times less than even the normal random variations in intensity of the Sun's natural ultraviolet (UV) energy which creates the ionosphere. The small effects that are produced, however, can be observed with the sensitive scientific instruments installed at the HAARP facility and these observations can provide new information about the dynamics of plasmas and new insight into the processes of solar-terrestrial interactions. The HAARP site has been constructed in three distinct phases. The Developmental Prototype (DP) had 18 antenna elements, organized in three columns by six rows. It was fed with a total of 360 kilowatts (kW) combined transmitter output power. The DP transmitted just enough power for the most basic of ionospheric testing. The Filled Developmental Prototype (FDP) had 48 antenna units arrayed in six columns by eight rows, with 960 kW of transmitter power. It was fairly comparable to other ionospheric heating facilities. This was used for a number of successful scientific experiments and ionospheric exploration campaigns over the years. The Final IRI (FIRI) will be the final build of the IRI. It has 180 antenna units, organized in 15 columns by 12 rows, yielding a theoretical maximum gain of 31 dB. A total of 3600 kW (3.6 MW) of transmitter power will feed it. The total effective radiated power (ERP) will be 3,981 MW (96 dBW). As of the summer of 2005, all the antennas were in place, but the final quota of transmitters had not yet been installed. As of March 2007, the final phase was completed and the antenna array was undergoing testing aimed at fine-tuning its performance to comply with safety requirements required by regulatory agencies. Each antenna element consists of a crossed dipole that can be polarized for linear, ordinary mode (O-mode), or extraordinary mode (X-mode) transmission and reception. Each part of the two section crossed dipoles are individually fed from a custom built transmitter, that has been specially designed with very low distortion. The ERP of the IRI is limited by more than a factor of 10 at its lower operating frequencies. Much of this is due to higher antenna losses and a less efficient antenna pattern. HAARP can transmit between 2.8 and 10 MHz. This frequency range lies above the AM radio broadcast band and well below Citizens' Band frequency allocations. The HAARP is only licensed to transmit in certain segments of this frequency range, however. When the IRI is transmitting, the bandwidth of the transmitted signal is 100 kHz or less. The IRI can transmit continuously (CW) or pulses as short as 100 microseconds (µs). CW transmission is generally used for ionospheric modification, while short pulses are frequently repeated, and the IRI is used as a radar system. Researchers can run experiments that use both modes of transmission, modifying the ionosphere for a predetermined amount of time, then measuring the decay of modification effects with pulsed transmissions.
Channel: Tech
Tags: active auroral energy frequency haarp heaven high holes illuminati in new nikola nwo order program research tesla world
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