Category Archives: Science

DPRK: N-Test, Take X

The UN Security Council has unanimously condemned North Korea’s latest nuclear firing test, which everyone seems to be assuming is their second such detonation, though that might not be the case.

The precise yield of the explosion is difficult to gauge for the following reasons: 

  1. Given the DPRK’s proficiency at digging shafts, tunnels and underground facilities, they may be successfully shielding and shaping their blasts in order to minimise their seismic signatures. If different device placement configurations are used for each test, this will help to confound those attempting to ‘profile’ the device in question — and, over a series, it will tell the North Koreans which configurations work best.
  2. The seismic waves generated by the most recent test are distinctly different from their first known test on October 9, 2006, which could mean that a different device type may have been employed this time, in which case, the previous data will be somewhat less useful in determining the energy output of the test at hand.
  3. Russian seismographs have been off-line for quite some time, limiting the number of high quality data points when interpreting the test’s meaning and ultimate implications. The Chinese ones have been running off-and-on for a good part of the past few months, which has proved less than helpful to seismic monitoring efforts focused on that part of the world. 

INCN_24hr
As compared to the first test, the blast barely registered a blip at China’s QIZ seismograph located at Guangzhou, Guangdong Province, which responded quite emphatically to the October 9th test. (See last story this topic.)

QIZ_24hr
Russian sources estimate the test’s yield to be in the range of 10 to 20 kilotons — which are the same figures they proposed for the first test, which turned out only to have generated a blast force of less than one kiloton. It makes you wonder about the value of Russian contributions on these matters. 

I’m still digesting the news (and the data), but I’ll take a stab at guessing the yield on this newest test — which could be anything from the country’s second to tenth nuclear test.

Best guesstimate at this time: 5 – 10 kT.
 
Note: There is also a possibility that two tests could have been conducted in almost immediate sequence (about 15 minutes apart) — with the second test of the day yielding roughly double the energy of the first. In other words: two tests registering 5 kT and 10 kT, respectively. (I can’t find a quake to match up with that second, slightly larger, blip. Maybe you can.)

INCN_24hr_2 

Did North Korea score a 2-for-1 deal once again?

Now, I guess we just wait to see what happens next.

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An Order of Pi on the (dark)Side

dE : dM = π : 1

dE = darkEnergy; dM = darkMatter

NASA Pi Chart?

NASA Pie Chart (dE, dM, m)

Note: This is seemingly true only because of the widespread misperception that the universe is expanding, and because of our failure to see galactic field integrity as a critical factor in the system’s rotational momentum, with the poles of the field being defined by the orientation of its Hawking ex-vortices and its “dark” mass being distributed according to each galaxy’s interaction with its neighbours.

Current NASA data tallies roughly 73%/23%/4%, respectively (see “pi” chart).

As data collection, comparison and amalgamation grow ever more precise, the numbers should shake out like this (rounded to 0.0000):

dE = 72.7131…%

dM = 23.1453…%

m = 4.1416…%

(Given as % of all gravitationally-affective materials/forces.)
Note that mass totals [π+1]% of the sum of itself, dE & dM.

If dE and dM really existed, this would actually be cool!

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When You’re Just Not Crazy Enough

“We in the back are convinced your theory is crazy. But what divides us is whether it is crazy enough to have a chance of being correct. My own feeling is that it is not crazy enough.” 
Niels Bohr to Wolfgang Pauli, on behalf of the “gang at the back” –
Columbia University, 1958. The remark was made by Bohr at the
conclusion of Pauli’s presentation of a non-linear field theory
of elementary particles developed by Werner Heisenberg and
himself. Pauli may have unintentionally invited the comment
when he allowed that the idea “might look” crazy.
.

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What’s in Einstein’s Refrigerator?

einstein refrigeratorMost people have no idea that Albert Einstein and Leo Szilárd invented a refrigeration mechanism with no moving parts, requiring no mechanical compressor. The range of designs (conceived between 1926 and 1933) were an alternative to the those devised by Baltzar von Platen and Carl Munters in 1922. A number of the ‘Einstein Refrigerator’ designs were subsequently purchased by Electrolux (assignees of the Platen-Munters designs) in order to secure their market position. 

Szilárd, Einstein’s former student, went on to work in many other significant collaborations, most notably, the Manhattan Project.

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Which Weighs More?

 


 

weight2

 

© 2009
 

 

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