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Old 19-10-2010, 08:24 PM
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CraigS
Unpredictable

CraigS is offline
 
Join Date: Jul 2010
Location: Australia
Posts: 3,023
Alex;

So, from the PU ‘Plasma Scaling’ link you sent the other day, it says:

Quote:
The first thing to notice is that many cosmic phenomena cannot be reproduced in the laboratory because the necessary magnetic field strength is beyond the technological limits. Of the phenomena listed, (Ionosphere, Exosphere, Interplanetary space, Interstellar space, Intergalactic space, Solar Chromosphere & Corona), only the ionosphere and the exosphere can be scaled to laboratory size. Another problem is the ionization fraction. When the size is varied over many orders of magnitude, the assumption of a partially ionized plasma may be violated in the simulation.
So, according to PU, there are many, many aspects of Plasma laboratory modeling/testing which cannot be demonstrated in the lab.

From this, it would seem unlikely that you could demonstrate your pulsar model in a ‘scaled down’ version in the lab. The only option I can see for the Relaxation Oscillator hypothesis, is a purely theoretical approach, using physics and mathematical models …

Quote:
Originally Posted by Jarvamundo
Double layers *do* store vast amounts of electrical energy, this has been empirically verified from lab to solar scales, so i have no concern there with cosmic scales of plasma double layers.
These two pieces of information seem to be at odds with each other when discussing Relaxation Oscillators emitting pulsar levels of radiation and exhibiting stabilities in the order of the magnitudes mentioned by Bojan. The leap between lab models and real-life pulsar phenomena would seem far from trivial.

Can you explain the discrepancy and fill in the blanks ?

Cheers

Last edited by CraigS; 20-10-2010 at 06:33 AM.
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