 | « on: June 14, 2010, 02:24:03 PM » |  Quote |
The European Incoherent Scatter Scientific Association (EISCAT) operates an ionospheric heating facility, capable of transmitting over 1 GW effective radiated power (ERP), near Tromsø in Norway.
EISCAT is an acronym for the European Incoherent Scatter Scientific Association. It operates three incoherent scatter radar systems, at 224 MHz, 931 MHz in Northern Scandinavia and one at 500 MHz on Svalbard, used to study the interaction between the Sun and the Earth as revealed by disturbances in the ionosphere and magnetosphere. At the Ramfjordmoen facility (near Tromsø, Norway) it also operates an ionospheric heater facility, similar to HAARP. Additional receiver stations are located in Sodankylä, Finland, and Kiruna, Sweden. The EISCAT Headquarters are also located in Kiruna.
An ionospheric heater is an array of antennas which are used for heating the ionosphere, and which can create artificial aurora.
According to Yahoo News this anomaly was seen by many people
From Trondelog to Finnmark 500 miles to the North. Maybe they fired up the old EISCAT
to have a little fun with the climate conference...G:
http://electricregime.blogspot.com/2009/12/ramfjordmoen-eiscat-spiral-anolamies-in.html
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EISCAT Organisation and Administration
EISCAT is an acronym of European Incoherent SCATter. The Association operates two powerful radar systems (using 224 MHz and 933 MHz); the transmitting site is in Tromsø (Norway) and the scattered signals are received at Tromsø and at additional receiving sites at Sodankylä (Finland) and Kiruna (Sweden). The Association's Headquarters are also in Kiruna.
EISCAT exists as a scientific and educational organization to conduct high latitude upper atmosphere research by the Incoherent Scatter technique and it provides instrumentation and observational opportunities for the scientific community to pursue these goals. It also uses its own staff resources to make long term synoptic observations of the ionosphere and upper atmosphere, to develop new signal processing and radar control hardware and software and to conduct its own research.
The EISCAT Scientific Association is governed by a Council, with members from each of the seven Associate countries (Germany, Finland, France, Japan, Norway, Sweden and the United Kingdom). The Council is supported by two advisory committees, also with representatives from each Associate. These two committees consider scientific and administrative/financial matters respectively. The executive consists of a Directorate and support staff at the Headquarters, and further scientific and technical staff are located at each of the three experimental sites. The total staff of EISCAT numbers about thirtyfive.
The total capital investment and accumulated operating costs now amount to some 275 million Swedish Crowns (MSEK) distributed between the Associates. Almost three-quarters of the original investment was allocated to the provision of the major hardware components - particularly the transmitters and antennas. The annual operating budget is about 33 MSEK.
EISCAT regularly achieves more than 2000 experiment-hours of operation each year and the accumulated total now exceeds 20000 hours. This time is distributed equally between Common and Special Programmes;
Special Programmes are usually combined into larger campaigns allowing many experiments to be conducted efficiently by groups of visiting scientists, assisted by EISCAT staff. EISCAT provides working space and accommodation for visiting scientists at each of its three sites.
The large number of publications (to the end of 1989), about 250 in the scientific literature, 50 doctoral and master's theses and innumerable presentations at international scientific meetings, all dealing with EISCAT science, makes the EISCAT radar facilities some of the most cost effective of the World's geophysical research projects.
Information about the EISCAT systems and operations can be found in various EISCAT reports; in particular, regular Annual Reports contain detailed summaries of operations, scientific results and reference lists. The latest, covering the years 1998-2001, is available on-line in high (11 Mb) or low (2 Mb) resolutions as well as the submissions (13 Mb - gzipped) to it.
http://www.eiscat.se:8080/organisation.html
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Three-dimensional simulations show the ELF (extremely low frequency) radiation generated by heating the high-latitude D region and modulating the polar electrojet. The simulations use a time-varying current perturbation in the D region. The ELF radiation is calculated in the Earth-ionospheric waveguide to a radial distance of 2400 km. The angular and radial dependence and the polarization of the horizontal, ground-level magnetic field are determined. The radiation pattern is a combination of a linear dipole antenna and a right-hand circular antenna. At ELF frequencies because of low D region absorption the dipole is dominant. The polarization and field strength in the near-field can predict the orientation of the radiation pattern and the wave amplitude in the far-field. The near-field polarization indicates the direction and strength of the electrojet. As the electromagnetic wave propagates in the waveguide, it drives whistlers waves into the D region. Because of reflection from the D region the mode inside the waveguide is not purely transverse. This gives a counterclockwise rotation to the polarization. Directly above the heated region, waves are also launched along the Earth’s magnetic field. The near-field polarization shows good agreement with observations from the high-power auroral stimulation array (HIPAS) and Tromsø. © 1999 American Geophysical Union
http://www.chemtrails911.com/docs/-%202006_june-december/Simulations%20of%20ELF%20radiation%20generated%20by%20heating%20the%20high-latitude%20D%20region.htm
EISCAT graphs ...
http://www.dcs.lancs.ac.uk/~kavanaaj/campaign.html
...and thank u Phasma again for this ... ;¥
TEQUILAsunrise (Transient Effects Quantification Under Ionospheric Low Angle sunrise). The idea is to look at the polar wintertime mesophere through the transient caused by (scattered) sunrise around 8 UT. Interestingly, this happens to
be the maximum occurence time of the Polar Mesosphere Winter Echoes (PMWE).
After reading up on this stuff I figured out they were performing an experiment on a layer of the atmosphere called the mesosphere, coincidentally, during the maximum time of PMWE (which is a time that the mesosphere reflects signals very well due to charged aerosols in it, as said in the title... Meteor dust). They used the sun coming in at a low angle to cause it to light up the area of the mesosphere they were hitting with VHF (Very High Frequencies). Basically, the overall goal of the test was to see it light up... like a "Tequilla Sunrise" And record the temperature, plasma density,etc in the effected area.
http://disclosure2009.blogspot.com/2009/12/norway-lights-actually-scientific.html
http://wwwppd.nrl.navy.mil/whatsnew/haarp/haarpabsez.gif
" ... in near future, the current EISCAT IS radars will be replaced by a new radar system consisting of multiple phased array antennas in northern Scandinavia will also be upgraded making it possible to design new heating experiments and therefore providing a 3D view of the ionosphere at high latitudes. The EISCAT Heating [emphasis added] ...."
In other words, with these upgrades the EISCAT facility -- in cooperation with other parts of "the northern Scandinavian HAARP antenna network" (below) -- could combine its beams ... and also project them (via their "phased array" technoloogy) considerably off-axis ... towards the horizon.
Which, of course, is exactly the direction from which the Norway Spiral initially appeared ... southeast of EISCAT, just over that pre-dawn horizon ... as viewed from the geometric center of this (now operational) "northern Scandinavian HAARP Interferometer (above) ...."
The same direction that our own analysis has strongly indicated an EISCAT experiment could, indeed, have caused such a spectacular phenomenon -- that another, totally independent geographic analysis has also now confirmed.
Over the eastern end of Russia's Kola Peninsula -- just north of the White Sea (below)--
http://fgportugal.blogspot.com/2010/02/feb-4-nobel-torsion-message-over-norway.html
...
EISCAT Radar School 2010
30th August - 4th September 2010
Sodankylä Geophysical Observatory
In the near future the EISCAT Scientific Association will face a major instrumental upgrade with the ESFRI Roadmap project "EISCAT_3D: A European Three-Dimensional Imaging Radar for Atmospheric and Geospace Research."
EISCAT, in co-operation with the Sodankylä Geophysical Observatory, will run a training course for new users of the EISCAT radars, from 30th August to 4th September, 2010 (Monday to Saturday). The training course will be held at Sodankylä, where one of the EISCAT UHF remote sites is located.
http://www.sgo.fi/Events/RS2010/
...
EISCAT_3D is a project led by EISCAT Scientific Association.
The planned radar facility consists of several large active phased-array antenna transmitter/receiver sites and multiple passive sites located in Norway, Finland and Sweden and comprising tens of thousands individual antenna elements. When it has been built, EISCAT_3D will be capable of making measurements from the upper stratosphere to the magnetosphere and beyond, contributing to basic, environmental and applied science that underpins the use of space by contemporary society.
http://www.eiscat3d.se/
!!!...like I've said the code of this technology has been join or compromised regardless of patents or any other complication, like 'international treaties' to not harm this planet!!!
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