HAARP |
Το πειραματικό πρόγραμμα HAARP (High frequency Active Auroral Research Project) έχει σκοπό τη μελέτη της ιονόσφαιρας για τη διέγερση και χρήση αυτής ως κεραίας ηλεκτρομαγνητικών κυμάτων, τη βελτίωση των επικοινωνιών (πχ HF, VHF, επικοινωνίες υποβρυχίων ELF, κτλ) αλλά ακόμη και για επιτήρηση (surveillance). Το HAARP χρηματοδοτείτο από την Αμερικάνικη Πολεμική Αεροπορία και το Ναυτικό, μετά δε την διακοπή αυτών των κονδυλίων το ανέλαβε η DARPA (Defense Advanced Research Projects Agency).
Η επίσημη πληροφορία... ...& εδώ the IHY Global AWESOME Network
Το πρόγραμμα έχει συνοδευτεί από συνωμοσιολογικές θεωρίες, σύμφωνα με τις οποίες, το HAARP αποτελεί αμερικανικό «υπερόπλο» μαζικής καταστροφής, το οποίο μέσω εσκεμμένης διέγερσης της ιονόσφαιρας επιτυγχάνει επιλεκτική διακοπή των επικοινωνιών σε συγκεκριμένες γεωγραφικές περιοχές, εξουδετέρωση των κατοίκων θέτοντάς τους σε κατάσταση λήθαργου/αδράνειας (ψυχοτρονικό όπλο), την πρόκληση καιρικών φαινομένων, σεισμών (περιβαλλοντικό/γεωφυσικό όπλο), κτλ. Παρόμοια με το HΑARP ιονοσφαιρικά συστήματα είναι το EISCAT (European Incoherent Scatter Scientific Association) με εγκαταστάσεις στο Τρόμσο της Νορβηγίας (μέλη Νορβηγία, Σουηδία, Φινλανδία, Ιαπωνία, Γαλλία, Μεγάλη Βρετανία, Γερμανία, Κίνα), καθώς επίσης και το Ρωσικό SURA. Παρόμοιο σύστημα υπάρχει και στο Ακρωτήρι της Κύπρου. *****************
HAARP is a scientific endeavor aimed at studying the properties and behavior of the ionosphere, with particular emphasis on being able to understand and use it to enhance communications and surveillance systems for both civilian and defense purposes. The HAARP program is committed to developing a world class ionospheric research facility consisting of:
Observation of the processes resulting from the use of the IRI in a controlled manner will allow scientists to better understand processes that occur continuously under the natural stimulation of the sun. Scientific instruments installed at the HAARP Observatory will be useful for a variety of continuing research efforts which do not involve the use of the IRI but are strictly passive. Among these studies include ionospheric characterization using satellite beacons, telescopic observation of the fine structure in the aurora, and documentation of long-term variations in the ozone layer. The induction magnetometer detects temporal variation of the geomagnetic field based on Faraday's law of magnetic induction. This instrument, which was provided by the University of Tokyo, is composed of three individual sensors. Each sensor is comprised of a large number of turns of fine copper wire wound around a rod with high magnetic permeability. The sensitivity of each sensor is determined by the effective area of the detection coil, that is, the cross sectional area of each winding, and the number of turns, and by magnetic flux density threading the coil. The magnetic flux density is enhanced by a factor of approximately 1,000 by the high-permeability metal core. The induction magnetometer installed at the HAARP site is designed to detect a signal level of a few picoTesla (pT) at 1 Hz. The overall frequency response of the magnetometer is shaped by Faraday's law at frequencies below 1 Hz and by active filters at frequencies above 1 Hz. Below 1 Hz the coil response is proportional to the time derivative of the magnetic field and thereby gives a response proportional to the frequency. Above 1 Hz, signals are suppressed by a low-pass filter with a corner frequency at 2.5 Hz. The filter response diminishes by 24 dB per octave above the corner frequency and thereby eliminates interference from 60 Hz radiation. The magnetometer sensors are aligned along the magnetic north, magnetic east and vertical directions to form an orthogonal measure of the derivative of the field. The sensor outputs are amplified by 40,000 and sampled at a 10 Hz rate with 16-bit resolution in a full scale of 10 Volts.
Typical signalsMagnetic field variations of interest in this program are those induced by electric currents in the ionosphere. The major signal categories detected by the induction magnetometer are short period magnetic pulsations such as Pc1, Pc2, Pc3, PiB, and PiC in a frequency range above a few tens of milliHertz. Among these, the induction magnetometer most efficiently detects Pc1 waves in the frequency range from 0.1 Hz to 3 Hz. Pc1 signals are the result of ion-cyclotron radiation generated near the equatorial plane of the outer-magnetosphere that make their way to the ionosphere guided by the magnetic lines of force. In addition, signals generated in the atmosphere that are caused by lightning discharges, the Schuman resonances, are also detected and sometimes become strong enough to mask signals from the ionosphere. ************************** ... και η συνωμοσιολογία HAARP in Japan?
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