Ok. Presumably they would have caught their error had they succeeded
in attaching a thermocouple to the surface
of the reactor right over the reaction chamber.

Harry

On Wed, Feb 24, 2016 at 3:40 PM, Bob Higgins <rj.bob.higg...@gmail.com> wrote:
> AFAIK, the Lugano team never publicly commented on the errors found in their
> analyses.  Tom Clarke makes a good case for some portions of the surface
> envelope to be at 780C.  If this were the whole story, the reactor would
> have been seen as a barely detectable red glow.  MFMP found in its replica
> that the roots of the ridges were 50C hotter than the tips of the ridges.
> But, even this doesn't explain the appearance.  Alumina is well known to
> transmit a lot of light in the visible, and we see that in the visible light
> pictures.  I think this is a case like the incandescent light bulb, where
> you cannot use the 1 surface temperature to characterize anything but the
> convection which was a small part of the overall output power.
>
> On Wed, Feb 24, 2016 at 1:31 PM, H LV <hveeder...@gmail.com> wrote:
>>
>> If I remember correctly, the Lugano team did not provide any internal
>> temperatures. They only reported the surface temperatures which were
>> high enough that the reactor should have glowed white hot if it
>> behaved like an incandescent body. However, as Jed pointed out, the
>> pictures they provided were more consistent with an incandescent body
>> at a lower surface lower temperature. Most people decided this was a
>> consequence of their camera's settings. Did the Lugano team say this
>> was reason?
>>
>> Harry
>>
>> On Wed, Feb 24, 2016 at 2:54 PM, Bob Higgins <rj.bob.higg...@gmail.com>
>> wrote:
>> > I don't think that is the reason for the Lugano appearance.  The Lugano
>> > reactor was like an incandescent light bulb and it was not analyzed that
>> > way.  If you analyzed an incandescent light bulb, the appearance and its
>> > radiated power would not be represented by the temperature of the glass
>> > envelope.  Yes, the glass envelope temperature will be what you want to
>> > use
>> > for the envelope convection power and envelope contribution to the
>> > radiation
>> > power.  However, you must use the temperature of the filament and the
>> > transmission response of the glass envelope to determine the radiated
>> > power.
>> > At the Lugano temperatures, radiated power dominated and the
>> > transparency of
>> > the alumina was unknown and not factored into the equation.
>> >
>> > Back to the light bulb, the glass envelope temperature may only be 80C,
>> > but
>> > you would hardly ascribe its heat + light energy output or visual
>> > appearance
>> > to be that of a blackbody radiator at 80C.
>> >
>> > On Wed, Feb 24, 2016 at 12:47 PM, H LV <hveeder...@gmail.com> wrote:
>> >>
>> >> An energy distribution whose peak becomes higher at lower temperatures
>> >> might help to explain
>> >> why the Lugano reactor's surface temperature appeared to be too high
>> >> for how it looked visually.
>> >>
>> >> Harry
>> >>
>
>

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