MANDALAS, YANTRAS, CHAKRAS, CROP CIRCLES.

MANDALAS, YANTRAS, CHAKRAS, CROP CIRCLES.
THE RAW MAGNETIC FORCE CAN BE ENCODED AND WHEN ENCODED, THE RESULTS ARE MAGNETIC DRIVER-MOTORS WHOSE OPTICAL LAYOUTS APPEAR AS MANDALAS, YANTRAS AND CHAKRAS.

quinta-feira, 18 de abril de 2019

SOLAR STORM: A RADIO, INTERNET AND CABLE BLACKOUT THIS EASTER WEEK-END AND SPECIALLY EASTER MONDAY MAY OCCUR.

Q!!mG7VJxZNCI
MUELLER BLOCKADE END.
Fake investigations by committee members will not delay what is about to be unleashed.
Q
If we are merely a LARP asking questions on the Chans, why are we being attacked daily by some of the world's biggest media co's, social media co's deliberately applying censorship/banning, shills paid/inserted to disrupt (media matters), blue checkmark coordinated attacks, etc.?
All for a 'conspiracy' on the Chans?
All for a 'LARP'?
Why is there a constant flow of disinformation being pushed re: Q?
Example:
Disinformation push re: Mueller is a white hat.
FAKE & FALSE narrative.
Think BLOCKADE.
When you can't attack the information directly, you attack the source, if that fails, you 'create false misleading information' to discredit knowing 'select' 'unaware' followers would not take the time to self-corroborate the claims (same vehicle/tactics used by FAKE NEWS media).
Logical thinking always wins.
Nothing can stop what is coming.
As the target(s) turn to the other side, the attacks will intensify.
We have the source.

CURRENT SPACE WEATHER CONDITIONS
 

SOLAR FLARES (RADIO BLACKOUTS)

Solar Flare Image
SOLAR FLARES (RADIO BLACKOUTS)
Solar flares are large eruptions of electromagnetic radiation from the Sun lasting from minutes to hours. The sudden outburst of electromagnetic energy travels at the speed of light, therefore any effect upon the sunlit side of Earth’s exposed outer atmosphere occurs at the same time the event is observed. The increased level of X-ray and extreme ultraviolet (EUV) radiation results in ionization in the lower layers of the ionosphere on the sunlit side of Earth. Under normal conditions, high frequency (HF) radio waves are able to support communication over long distances by refraction via the upper layers of the ionosphere. When a strong enough solar flare occurs, ionization is produced in the lower, more dense layers of the ionosphere (the D-layer), and radio waves that interact with electrons in layers lose energy due to the more frequent collisions that occur in the higher density environment of the D-layer. This can cause HF radio signals to become degraded or completely absorbed. This results in a radio blackout – the absence of HF communication, primarily impacting the 3 to 30 MHz band. The D-RAP (D-Region Absorption Prediction) product correlates flare intensity to D-layer absorption strength and spread.
Solar flares usually take place in active regions, which are areas on the Sun marked by the presence of strong magnetic fields; typically associated with sunspot groups. As these magnetic fields evolve, they can reach a point of instability and release energy in a variety of forms. These include electromagnetic radiation, which are observed as solar flares.
Solar flare intensities cover a large range and are classified in terms of peak emission in the 0.1 – 0.8 nm spectral band (soft x-rays) of the NOAA/GOES XRS. The X-ray flux levels start with the “A” level (nominally starting at 10-8 W/m2). The next level, ten times higher, is the “B” level (≥ 10-7 W/m2); followed by “C” flares (10-6 W/m2), “M” flares (10-5 W/m2), and finally “X” flares (10-4 W/m2).
Radio blackouts are classified using a five-level NOAA Space Weather Scale, directly related to the flare’s max peak in soft X-rays reached or expected. SWPC currently forecasts the probability of C, M, and X-class flares and relates it to the probability of an R1-R2, and R3 or greater events as part of our 3-day forecast and forecast discussion products. SWPC also issues an alert when an M5 (R2) flare occurs.
The table below provides the correlation between radio blackouts, solar flares, nominal energy flux (watts per square meter), and the designated severity event descriptor

Radio Blackout….. X-ray Flare….. Flux (W/m2)….. Severity Descriptor
R1                            M1                   0.00001               Minor
R2                            M5                   0.00005               Moderate
R3                            X1                     0.0001                 Strong
R4                            X10                   0.001                   Severe
R5                            X20                   0.002                   Extreme

*IMAGE courtesy of NASA
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