Axil,
                How about a very dynamic isotropy?  while C MUST appear 
constant throughout our macro frame adhering to the rules of SR, acceleration 
and gravitational fields, what if….. the rate of virtual particles passing 
through our plane had a certain dynamic flow. By the rules of SR we could never 
be aware of this flow at the macro scale  since this rate reflects in the clock 
rate for all physical matter.. but these anomalous radioactive decay rates and 
relativistic like forms of hydrogen with exotic ground states make me ask the 
question, what if quantum geometries at the nano scale can accumulate an 
opposition to this flow into the physical scale–segregating it into faster and 
slower regions inside and outside the suppression zones where longer vacuum 
wavelengths  have to  dilate to pass thru our plane? The solar activity you 
cite wrt change in nuclear decay could be the SAME normal percentage of 
suppression in the radioactive geometry illuminating a change in isotropy that 
we as macro participants in the isotropy are unable to detect - our inertial 
frame is unchanged relative to macroverse – I am not talking about a change 
from any spatial direction that would be detectable but rather variation in the 
pressure of the Dirac sea  or along the temporal axis.
Fran

From: Axil Axil [mailto:[email protected]]
Sent: Saturday, August 23, 2014 2:18 AM
To: vortex-l
Subject: EXTERNAL: [Vo]:It must be magnetism


On Dec 13, 2006, the sun itself provided a crucial clue, when a solar flare 
sent a stream of particles and radiation toward Earth. Purdue nuclear engineer 
Jere Jenkins, while measuring the decay rate of manganese-54, a short-lived 
isotope used in medical diagnostics, noticed that the rate dropped slightly 
during the flare, a decrease that started about a day and a half before the 
flare.

Read more at: http://phys.org/news201795438.html#jCp

The unknown force from the sun must not only increase nuclear decay rates but 
reduce them. This is an important clue to the nature of this unknown factor. 
Radioactive decay rates must be embedded in an environment that defines its 
nature. That environment can be increased or decreased based on solar activity 
and in fact is defined by solar activity.

The sun must provide an average background flux that directly affects the rates 
of decay. Various parts of the sun contribute to this background. This 
background comes from the core of the sun, but it can also be effected by 
localized regions on the sun’s surface.

It must be magnetism. Here is why…

The high magnetic fields in the sunspot-producing active regions also give rise 
to explosions known as solar flares. When the twisted field lines cross and 
reconnect, energy explodes outward with a force exceeding that of millions of 
hydrogen bombs.

Temperatures in the outer layer of the sun, known as the corona, typically fall 
around a few million kelvins. As solar flares push through the corona, they 
heat its gas to anywhere from 10 to 20 million K, occasionally reaching as high 
as a hundred million.

Because solar flares form in the same active regions as sunspots, they are 
connected to these smaller, less violent events. Flares tend to follow the same 
11-year cycle. At the peak of the cycle, several flares may occur each day, 
with an average lifetime of only 10 minutes.

Solar flares vary in size and power. The largest, X-class flares have the most 
significant effect on Earth. They can cause long-lasting radiation storms in 
the upper atmosphere, and trigger radio blackouts. Medium-size M-class flares 
can cause brief radio blackouts in the Polar Regions and the occasional minor 
radiation storms. C-class flares have few noticeable consequences.

Absorbing X-rays affects the atmosphere. The increase in heat and energy result 
in an expansion of the Earth's ionosphere. Man-made radio waves travel through 
this portion of the upper atmosphere, so radio communications can be disturbed 
by its sudden unpredictable growth. Similarly, satellites previously circling 
through vacuum-free space can find themselves caught in the expanded sphere. 
The resulting friction slows down their orbit, and can bring them back to Earth 
sooner than intended.

Despite their size and high energy, solar flares are almost never visible 
optically. The bright emission of the surrounding photosphere, where the sun's 
light originates, tends to overshadow even these explosive phenomena. Radio and 
optical emissions can be observed on Earth.

What I am saying in so many words is that solar flares are very powerful.

Clearly, a tremendous amount of magnetic energy is converted in an instant to 
all the aforementioned energetic phenomena at the expense of the magnetic 
output of the sun. The sun stores vast amounts of energy in its magnetic 
fields. A sudden release and conversion of that energy will reduce that 
magnetic energy storehouse and consequentially reduce the magnetic background 
around earth that defines the rate of radioactive decay.

Reply via email to