I in this paragraph show the behavior of the speedy gravitational waves.
The gravitational waves here under received, comes produced
by two sensors installed in two separate boxes of iron tinned hermetic,
and feeds with electric contained piles to the inside of the same boxes.
I must have used these sagacity, for eliminate the interferences of the
electromagnetic waves that passed from the electric network, and radio,
and that they disturbed strongly the waves that I must reveal. With this
shielding, I could have amplified the gravitational waves, of 10000 times,
without any noise. The height of the signal in input to the amplifiers,
he is of about 200 microvolt, while the exit goes up to 2 volt. The two
signals that go out, they go in the entry of a audio card of a computer
(AVE_64 GOLD), and comes recorded on the computer. The card audio records
the waves with a sampling rate of 44 Khz in frequency, and with two ADC
to 16 bit of resolution. This one allows me of see the two waves very detailed.
Additionally, amplifying by computer of 100 times the signal I could see
the noise produced by the amplifier. Amplifying again 10 times the signal,
I arrive at to see the noise of the audio card. Recapitulate, I have: 200
microvolt pp, amplitude of the gravitational wave. 2 microvolt pp, amplitude
of the noise of the amplifier. 150 nanovolt pp, amplitude of the noise
of the audio card of the computer. The frequency of this last noise is
more a little of 10Khz. We see now the graphic inferior.
On these two graphic, is seen two piece of gravitational waves
left one of the two boxes. The total duration of each, he is of 160 milliseconds.
On the first wave, he could be seen in the central part, a decrease of
the signal, the waves are enough small. On the second diagram, always of
160 milliseconds of duration, the waves appear higher. That means. I premise
that the waves that appear, given the high frequency, (from 40 to 1000
hz) on the average, I have produced by nuclei of stars that to collapse
on the nuclei of supermassive quasar. The positive half-wave represents
the collapse, while the negative half-wave, the next burst. I repeat again,
that the inside of these quasar, it could not be observed, by different
instruments from those that I build, because they are wrapped by a dense
shell of gas at high temperature. If the quasar is not as made, we would
see an uninterrupted flashing, in the nocturnal sky. When a star falls
over the surface of one of these celestial bodies, the initial impact,
he is had with the external shell of the quasar in question. In this first
impact, the star loses whole the gaseous portion, he then continues the
run and his nucleus he breaks on the surface of one of the nuclei of the
quasar. For this reason waves of short duration are seen. (which they go
from about half millisecond, to about 10 milliseconds, on the average),
we see in fact the time of impact of the nucleus of the star, very small
nucleus. Also if waves of any about tens of milliseconds are observed,
these is composed waves by numerous simple waves.
The three graphics next they refer to spectrograms of: 1) Spectrogram
of the duration of 1.5 second. See the frequencies and the energies of
the waves. 2) three-dimensional Spectrogram of the duration of 2 minutes
of correspondent recording to an in single file of 10 Mbytes of data. 3)
three-dimensional Spectrogram of the duration of 2 minutes of recording
of the two instruments in stereo, and of 10 Mbytes of data. If they then
are listened to in audio and in directed these continual collapses, a terrifying
noise is listened to, equivalent to that of the fallen of an avalanche
and of a strong combined earthquake together. Makes fear. This noise doesn't
ever have end.
figure 1.available by file from test01
figure 2.available by file from test02
figure 3.available by file from test03
figure 4.available by file from test04
figure 5.available by file from test05
figure 6.available by file from test06
figu re 7.available by file from test07
figure 8.available by file from test08
figure 9.available by file from test09
figure 10.available by file from test10
figure 11.available by file from test11
figure 12.available by file from test12
figure 13.available by file from test13
figure 14.available by file from test14
figure 15.available by file from test15
figure 16.available by file from test16
figure 17.available by file from test17
figure 18.available by file from test18
figure 18b. Discussion file from test18b
figure 19.available by file from test19
figure 0.available by file from Homepage