There are multiple weirdnesses about Rossi's January presentation of the SK, but the weirdest of all involves his treatment of the SK spectrum. Of course lots of people have noted that the spectrum doesn't look very blackbody - ish, but probably many don't understand how out-of-bound it is.
So ... below I show a plot comparing the SK spectrum that Rossi showed in his presentation (blue) and a the theoretical spectrum (orange) for a blackbody at 8111 degrees K (note: the SK spectrum is based on a compilation of 17 screen grabs provided at http://www.electric-sailing.fi/other/EcatSK/ by Pekka Janhunen and the theoretiical curve is from a nice online calculator available athttps://astrogeology.usgs.gov/tools/thermal-radiance-calculator/ ).
I have done my best to fit the theoretical curve to the measured SK spectral data. Given a temperature of 8111 K, the only parameter available for fitting is the overall magnitude of the orange calculated spectrum -- the location of its peak and the existence of the long tail on the right are invariant. So I might be a little off with my fitting but I am confident that this is pretty much the best fit achievable as long as you ignore the isolated peaks at short wavelengths that appear to be individual emission lines.
What is glaringly obvious in the plot is that the SK spectrum is missing a huge amount of power at wavelengths longer than about 420. Here is a closeup of the region where the SK spectrum just gives out bu the theoretical blackbody spectrum just keeps on rolling.
Rossi claims he sees a peak in the SK spectrum at 357 nm. I don't really see that in the SK spectrum here although I guess you could argue that the data are at least sort of consistent with this. But the sudden collapse of the SK spectrum above about 415 nm is remarkable when compared with an actual blackbody curve. I originally wondered if this was due to a limitation of the response of the spectrometer or due to filtering of the light, but why would Rossi introduce these limitations when at the same time he is so intent on showing people the 437.2 nm peak he predicted in his recent paper.
Perhaps we should ask Mr Rossi about all this! Well thank goodness someone has done just that. Of the more than 400 messages on Rossi's blog in the last 3 weeks since the SK production, 3 have asked where the longer wavelength have gone. The first time he was asked, by Steven Karels at 8:24 on Feb 9, Rossi's full response is ...
A “Black Body” is a hypothetical absorber and radiator of energy, with no reflecting power. It radiates at all frequencies with a spectral energy distribution dependent on its temperature in Kelvin. Our calculation is focused only in 1 cm^2 where the plasma has the max density, while the plasma has a surface of about 330 cm^2, so to measure the power we consider only 1/330 of the plasma surface focusing conservatively only where there is the max density and the max absolute temperature. As you can see, the spectrum is more complex.
Obviously it radiates only at the frequencies with a spectral energy distribution corresponding to the temperature in K.
Only the final sentence of this attempts to answer Karel's question and that is not very satisfactory.
Other answers on the same topic are ...
- To Lotr Milekosky at 2:10AM on Feb 20 who asks if the lack of long wavelength is due to a filter ...
No. The absence of lambda>500 nm is due to the fact that we pointed the focus only where the plasma had the highest density, in coherence with the theoretical hypothesis wrote in https://researchgate.net/publi…nge_particle_interactions"
- To Stephen at 5:22 on Feb 20 ...
We want not to compute also the energy of longer waves, to be conservative and focus only where the density of the plasma is highest: in https://www.researchgate.net/p…nge_particle_interactions
In sum, Rossi's answers on this topic are either just plain wrong, or vague or misleading. The whole thing is a mess even though the spectral stuff is one of his main arguments for COP > 1
.