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.