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H.A.A.R.P Sounds Haiti With Aurora Images

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Uploaded by on Jan 18, 2010

HAARP Sounds Haiti Quake With Aurora Images How events unfolded in the geomagnetic field , before & after the Haiti quake - with a magnitude of 7.0 Rs - struck at 1653 local time (2153 GMT) on Tuesday, 12 January.

If you wish to donate towards this disaster, please do so at ... http://www.dec.org.uk/

The HAARP Induction Magnetometer Jan 12th
From ... http://137.229.36.30/cgi-bin/scmag/disp-scmag.cgi?date=20100111&Bx=on

The images are a time-frequency spectrograms, which shows the frequency content of signals recorded by the HAARP Induction Magnetometer.

This instrument, provided by the University of Tokyo, measures temporal variations in the geomagnetic field in the ULF (ultra-low frequency) range of 0-5 Hz.

The spectrogram images are produced by computing the PSD (power spectral density) of successive 102.4-second segments of timeseries data, and plotting these spectra as colour/intensity slices along a 24-hour scale.

If the images below is not too interesting, you might want to look at 02 Sep 2004 for an example of narrowband PC1 pulsations, or 27 Jul 2004 for an example of wideband ULF noise during a magnetic substorm. Expanded plots of the last 12 hours, last 6 hours, last 3 hours, and last 1 hour are also available.

Click To View 27 July 2004 ... http://137.229.36.30/cgi-bin/scmag/disp-scmag.cgi?20040727 ... and follow links on page. for all years.

The induction magnetometer installed at the HAARP site is designed to detect a signal level of a few picoTesla (pT) at 1 Hz.

The over all 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. ... http://www.haarp.alaska.edu/haarp/magind.html

The aurora images in this video are intended for non-commercial, educational uses only & Copyrighted to: © Jan Curtis
Websites ... http://climate.gi.alaska.edu/Curtis/curtis.html

http://climate.gi.alaska.edu/Curtis/aurora/feb03/feb03.html

And ... http://latitude64photos.com

Music From Michel Dezanger ..
Thanks Mate.

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Education

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