to: Ames Research Station-Kepler system

[viragons]

Kusari Naval Forces
Exploration Wing
Nensei Research Station

from: kaigun Chusa Daiso Takata
to: Ames Research Station-
Comm ID : Edward Malrone, Co Admistrator

Kuryo Anomaly

Konnichiwa mr. Edward Malrone

After several days of research in our library, and documents of the great scientist Ichi Matsuo, deliver you for review the theory of Kuryo Anomaly
I should point out right from the start, that on this theory works several of our skilled experts from the Nansei Research Complex, and works years to permanently monitors the status of anomalies and movement of unstable pulsars, dark matter within it.

This is a clip from one document ...

How to notice dr.Matsuo followed the movement through two prisms tracking. It was noted that Kuryo cloud has so far static anomaly that is within the solar magnetic and ionosferic winds. This directly impacts on the wrong level of the ionic, proton and neutron radiation.differences of opinion between Dr. Matsuo and our scientists now is that Dr. Matsuo observed anomaly and the appearance of dark matter through dynamic movement of.
Is it some random x-rays, or perhaps the influence of proton winds, the position of the anomaly is now to become stable, while the dark matter particles within the cloud reduced the movement and become centered.
Use a form formulas
E2 = p2c2 + m2c4

Where p is momentum. Which has been used to justify the Existence of very high energy particles with negligible mass. Like neutrinos that after traveling through space pass straight through the planet or systems. However they should be detectable from the bluelight they emit as they loose momentum.What Dr. Matsuo not had the opportunity to discover, right technology was not as widespread as now, this is what is left of our scientists in awe. Using 4 clusters and compacting the particles of the atom cloud came to chart sterilization of one particle of dark matter with nanosfericnim cloud the water.

occurrence of water in its original form and not the appearance of Sirius in some parts, but as far as Kepler sector has remained a small mystery. especially that its part which refers to binding molecules of oxygen.

On average, density at the surface and at cloud base is smaller, and the rate of distribution greater, than measured. Including pressure fronts in the simulations reduces convective intensity, increases boundary layer stratification, and decreases DMP for nearly all models. Including pressure fronts substantially decreases entrainment, decreases convective intensity, and increases DMP for most models. In nearly all cases, DMP responds more strongly to cloud matter sedimentation than to density. The omission of cloud matter sedimentation in simulations is strongly discouraged, regardless of whether or not sediment is present at cloud base.
Monitoring the work of Dr. Matsuo is coming to a constant that is repeated in every observations concerning dark matter. His studying proton compaction of particles and gamma rays within the dark matter gives us an indication that the variability of the constant changes in the basis of TGA compaction of the particles of dark matter that is moving along the edge of the center of dark matter.
Starting from the fact that the compaction of clouds of dark matter its dynamic force moves outward, reaches the value of conjunctive force acting at a point directions, and it prints to send a huge force of energy

using gamma radiation leads to such imagery of action

In TGD framework both dark energy and dark matter are assumed to correspond to dark matter but with widely different values of dr Matsuo constant. The point is that very large value of dr Matsuo constant for dark matter implies that its density is in an excellent approximation constant as is also the density of dark energy. dr Matsuo constant is indeed predicted to be gigantic at the space-time sheets mediating gravitational interaction.

The appearance of number five as a ratio of mass densities sounds mysterious. Why the average mass in a large volume should be proportional to hbar at least if hbar is not too large? Intriguingly, number five appears also in the Bohr model for planetary orbits. The value of the gravitational Matsuo constant GMm/v0 assignable to the space-time sheets mediating gravitational interaction between planet and star is gigantic: v0/c ∼2-11 holds true inner planes. For outer planets v0/c is by a factor 1/5 smaller so that coresponding gravitational Matsuo constant is 5 times larger. Do these two fives represent a mere coincidence?

In accordance with TGD inspired cosmology suppose that visible matter and also the matter which is conventionally called dark matter has emerged from the decay and widening of cosmic strings to magnetic flux tubes. Assume that the string tension can be written as k×hbar/G, k a numerical constant.
Suppose that the values of hbar come as pairs hbar=n× hbar0 and 5×hbar. Suppose also that for a given value of hbar the length of the cosmic string (if present at all) inside a sphere or radius R is given by L=x(n)R, x(n) a numerical constant which can depend on the pair but is same for the members of the pair (hbar,5×hbar). This assumption is supported by the velocity curves of distant stars around galaxies.
These assumptions imply that the masses of matter for a pair (hbar,5×hbar) corresponding to a given value of hbar in a volume of size R are given by M(hbar)= k× x(hbar)× hbar×R/G and M(5×hbar)= 5×M(hbar). This would explain the finding if visible matter corresponds to hbar0, and x(n) is much smaller for pairs (n>1,5×n) than for the pair (1,5).

One can explain the pairing in TGD framework. Let us accept the earlier hypothesis that the preferred values of hbar correspond to number theoretically maximally simple quantum phases q= exp(i2π/n) emerging first in the number theoretical evolution having a nice formulation in terms of algebraic extensions of rationals and p-adics and the gradual migration of matter to the pages of the book like structure labelled by large values of Planck constant. These number theoretically simple quantum phases correspond to n-polygons drawable by ruler and compass construction. This predicts that the preferred values of hbar correspond to a power of 2 multiplied by a product of Fermat primes Fk=22k+1. The list of known Fermat primes is short and given by Fk, k=0,1,2,3,4 giving the Fermat primes 3,5,17,257, 216+1. This hypothesis indeed predicts that Matsuo constants hbar and 5×hbar appear as pairs.

This picture supports the view that ordinary matter and what is usually called dark matter are characterized by Matsuo costants hbar0 and 5×hbar0, and that the space-time sheets mediating gravitational interaction correspond to dark energy because the density of matter at these space-time sheets must be constant in an excellent approximation since Compton lengths are so gigantic.

Using the fact that 4 per cent of matter is visible this means that n=5 corresponds to 20 per cent of dark matter in standard sense. Pairs (n>1,5×n) should contribute the remaining 2 per cent of dark matter. The fractal scaling law

x(n) proportional to 1/nr

allowing pairs defined by all Fermat integers not divisible by 5 would give for the mass fraction of conventional dark matter with n>1 the expression

p = 6× ∑k 2-kr×[2-r+ ∑ nF-r]× (4/100)= (24/100)× (1-2-r)-1×[2-r+ ∑ nF-r] .

Here nF denotes a Fermat integer which is product of some Fermat primes in the set {3,17,257, 216+1}. The contribution from n=2k, k>0, gives the term not included to the sum over nF. r=4.945 predicts p=2.0035 and that the mass density of dark matter should scale down as 1/hbarr-1= 1/hbar3.945.

The prediction brings in mind the scaling 1/ar-1 for the cosmological mass density. a-4 scaling for the radiation dominated cosmology is very near to this scaling. r=5 would predict p=1.9164 which is of course consistent with the data. This inspires the working hypothesis that the density of dark matter as function of hbar scales just like the density of matter as function of cosmic time at particular epoch. In matter dominated cosmology with mass density behaving as 1/a3 one would have r=4 and p=4.45. In asymptotic cosmology with mass density behaving as 1/a2 (according to TGD) one would have r=3 and p=11.68.
Living systems would represent a deviation from the "fractal thermodynamics" for hbar since for the typical values of hbar associated with the magnetic bodies in living systems (say hbar= 244hbar0 for EEG to guarantee the the energies of EEG photons are above the thermal threshold) the density of the dark matter would be extremely small. Bio-rhythms are assumed to come as powers of 2 in the simplest model for the bio-system: the above considerations raise the question whether these rhythms could be accompanied by 5-multiples and perhaps also by Fermat integer multiples. For instance, the fundamental 10 Hz alpha frequency could be accompanied by 2 Hz frequency and the 40 Hz thalamocortical resonance frequency by 8 Hz frequency.

Detecting the appearance of water molecules, which facilitated greatly the formation of the picture size of the anomaly and the measuring points in which the arrangements observed the presence of dark matter particles.percent of the Doppler effect on the Kuryo, it has no effect, three-dimensional display using laser action of gamma particles, and with the help of four clusters gave us this picture of the position of anomalies in the clouds.This three-dimensional map, and ls Xray XMM-Matsuo data, offers a first look at the web-like large-scale distribution of dark matter, an invisible form of matter that accounts for the majority of the mass in the your system.

Mr Malrone, these are for now the data with which we work with .. we sent a couple of automated probes in the center of the cloud, the place for us to dispose with the largest molecules of dark matter, but because of certain technical irregularities in the construction of the probe, there was a leak, and their destruction. Command KNF-Exploration wing over Kishiro Corporation, currently in phase of making new probes that will be directed towards the same place in the monitoring of the anomaly.
I hope that you find these few information provided to assist in your further study.
[color=#000000]
<div align="right]kaigun Chusa
Daiso Takata

---

[Ames Research Station]

COMM ID : Edward Malrone, Co Admistrator
Topic: Historical Data


To : Kusari Naval Forces

Greetings,

Your Data are very precious. That will update some of ours. The map you send me, will be very helpful.
I hope to have result in a few month.

Concerning the probe, we have designed a new polymer which one act as a sponge, once a layer is 'full', it's automatically evaporating in space. Each layer can sustain the radiation for 2-3 month. Each layer is 1 mm thick. However the polymer very rigid. So for each mobile part we currently use a basic hull. And the manufacturing is pretty costly. If you are interested in.

Thanks for your time.

Sincerely Edward Malrone.

---

[viragons]

Kusari Naval Forces
Exploration Wing
Nensei Research Station

[color=#000000]from: kaigun Chusa Daiso Takata
to: Ames Research Station-
Comm ID : Edward Malrone, Co Admistrator

Mr.Malrone
would not want to sound overbearing, but perhaps should think of change in material you use. Polymer molecules in too large and consist of several chains of mono and nucleoid monomers.
Strength of a single chain monomer is general enough to gamma radiation, which is found in Kuryo cloud. With 100% polymer, which is otherwise very difficult to find in Sirius, may be endured about 17 minutes.
By Matsuo-Hirogato theory, which is used to protect against gamma radiation, and according to some sources in the old documents which were found in the archives from the era of planet Earth,"Shielding from gamma rays requires large amounts of mass. They are better absorbed by materials with high atomic numbers and high density, although neither effect is important compared to the total mass per area in the path of the gamma ray. For this reason, a lead shield is only modestly better (20'€“30%) as a gamma shield than an equal mass of another shielding material such as aluminium, concrete, or soil; lead's major advantage is its density.

The higher the energy of the gamma rays, the thicker the shielding required. Materials for shielding gamma rays are typically measured by the thickness required to reduce the intensity of the gamma rays by one half (the half value layer or HVL). For example gamma rays that require 1 cm (0.4″) of lead to reduce their intensity by 50% will also have their intensity reduced in half by 4.1 cm of granite rock, 6 cm (2½″) of concrete, or 9 cm (3½″) of packed soil. However, the mass of this much concrete or soil is only 20'€“30% larger than that of lead with the same absorption capability. Depleted uranium is used for shielding in portable gamma ray sources, but again the savings in weight over lead is modest, and the main effect is to reduce shielding bulk."

Our scientists were based on the comparability between the four materials: Boron, Beryllium, Cobalt and Diamond.But, for example, Boron, in his state isotope Boron-10 is excellent in protection against nuclear, radiation more precisely, while the other components that are a byproduct, acid Boron and Borates are slightly toxic to the human body.Beryllium on the other hand absorbs neutron radiation in the 93% effective, but for its material condition is very fragile.Cobalt alloys, in its unalloyed condition, serving a large compression and abnormally high temperatures and is also resistant to corrosion, while on the other hand, cobalt alloy C60, is intense gamma ray emitter, which can infrequently cause serious body damage and death.As you can conclude how much of good and poor is the selection of materials. But for now, an intensive search for a best solution.


[color=#000000]

Sincerely

[color=#000000]<div align="right]kaigun Chusa
Daiso Takata

---

[Ames Research Station]

COMM ID : Edward Malrone, Co Admistrator
Topic: Historical Data


To : Kusari Naval Forces

Very well, then I hope you will find what you want in your way. We live near a dark matter cloud everyday, we know what we do. The Kuryo Anomaly have still lot of secret.

Thanks for your time.

Sincerely Edward Malrone.

---