>From what I took away from the Mills demo, Mills says that he uses fluorescence to convert and downshift the XUV and X-ray EMF into the visible spectrum. I don't recall exactly, but Mills says that he is using some sulfate to do this light frequency downshifting. He must do this to get the EMF into the frequency range needed to allow a solar cell to convert the visible EMF into electric current. He cannot find a solar cell now that can work with XUV and x-rays but he is working on this direct conversion as a side project.
On Fri, Feb 5, 2016 at 1:49 PM, Bob Higgins <[email protected]> wrote: > My take on the curves shown after slide 49 is that they were showing > evolution of the spectrum. As the machine and Ag vapor gets hotter and > hotter, the spectrum will begin to be dominated/overwhelmed by blackbody > radiation. What is heated to those temperatures is Ag vapor. I am not > sure exactly what you mean by "lasts very long at that temperature" (I > presume you mean doesn't melt), but I think the answer is that we are > talking about a vapor (gas) of Ag. Plasmas are commonly at that > temperature. > > I said that the 10V source has a capability of generating up to 10eV > effects which correspond to 124nm minimum wavelength photons. In the chart > 49 you can see the spectrum from the photons cut-off before reaching down > to 124nm. This spectrum is from the emissions of the silver+H2O in the arc > before being overwhelmed by the vapor around it that is very hot. A 10eV > electron or a 124nm photon is not enough to ionize the inner shells of Ag, > even if it is a vapor. Another thing to consider is drawing a > Stephan-Boltzmann curve over the UV portion of the radiation below that > cuts off just before reaching down to 124nm. The temperature for such a > curve would be about 6000K. Even at 6000K, you don't produce blackbody > photons at 124nm. My point here being that the soft x-ray spectra are not > explained by the temperature (even of 6000K) or 10eV possible excitations > from the 10V. > > OTOH, Karabut has published papers about the generation of laser-like > x-ray photons in systems capable only of lower energy transitions. It > could be a hydrino signature, but that was not Karabut's conclusion, nor > that of Peter Hagelstein who has a theory for what is happening in > Karabut's experiments. > > On Fri, Feb 5, 2016 at 10:30 AM, Bob Cook <[email protected]> wrote: > >> Bob-- >> >> Look at slides that follow #49—like about 57 and 60 or so. The first >> is a multi-colored spectrum of some different runs I believe in Nano meters >> up to about 500. And the second is a calculated spectrum for a black body >> for 5000 D Kelvin. Note that the multi-colored graph shows each run of the >> colored lines turning into a black body spectrum for about 5000 D K. >> >> If some material stands 5000 D K for any length of time, I would like to >> know what it is. May Iridium oxide or some heavy trans-uranium oxide. I >> do not think thoria lasts very long at that temperature? Maybe it is a >> metal hydrino compound [image: Smile] >> >> Bob Cook >> >> *From:* Bob Higgins <[email protected]> >> *Sent:* Friday, February 05, 2016 8:03 AM >> *To:* [email protected] >> *Subject:* Re: [Vo]:BLP demo video >> >> Thank you, Axil, for this link. It is slide 49, in particular to which I >> am making reference. In this slide you can see the soft x-ray set of lines >> around 20-60nm, and another set of deep UV lines from 120-300nm. What I >> was saying is that the band from 120-300nm is explain-able from the 10V >> source, capable of providing 10eV direct excitation, while the lines from >> 20-60nm are harder to explain. In fact, it is hard to measure this >> spectrum ... I wonder what he used to measure it. >> >> [image: Inline image 1] >> >> On Fri, Feb 5, 2016 at 8:31 AM, Axil Axil <[email protected]> wrote: >> >>> Dear Dave, >>> >>> This may help >>> >>> >>> http://brilliantlightpower.com/wp-content/uploads/pdf/TechnicalPresentation1.8.16.pdf >>> >>> These are the slides used in the demo >>> >>> Slide 53 and/or 57 are what you might need to see what you want. >>> >> >
