On Tue, Jun 24, 2014 at 04:31:00PM -0400, John Mikes wrote:
> Russell:
> you wrote:
> 
> 
> *Not really - the peak of the solar spectrum is yellow light. The IR and UV*
> *portions are relatively small components, and what little there is is
> further absorbed by water vapour and the ozone layer respectively.*
> 
> Is ALL you do mean the SOLAR (!) spectrum we can detect with our
> instruments?
> Are you sure there is nothing else? Liz mentioned EM spectrum *total*. What
> is included in it beyond the above (as part of our unknowables)?
> John M
> 

Nothing. We can measure everything in the EM spectrum from sub 1Hz up
to high energy gamma rays. Different instruments are used for
different bands, but they all overlap and are cailbrated against each
other. I understand that the gamma ray spectrum is unbounded, since
any photon with sufficient energy to knock an electron out of an atom
(ionising radiation) will be detected by a photomultiplier, regardless
of whether it is the photoelectric effect, the Comptom effect or pair
production that is involved. The sub 1Hz spectrum really is
unimportant, as there is no useful energy in a photon whose wavelength
is bigger than the Earth.

We also have a well established theory called "blackbody radiation"
that gives a distribution of photon energies being emitted from a body
at a given temperature. The sun's distribution fits that perfectly, so
we have sound theoretical reasons why it is not emitting anything
appreciable outside that spectrum.

Obviously, the name "blackbody radiator" is a misnomer, as it needn't
be black, as in the Sun's case. Another example of a blackbody
radiator is the incandescent lightglobe (when turned on!).

-- 

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Prof Russell Standish                  Phone 0425 253119 (mobile)
Principal, High Performance Coders
Visiting Professor of Mathematics      hpco...@hpcoders.com.au
University of New South Wales          http://www.hpcoders.com.au

 Latest project: The Amoeba's Secret 
         (http://www.hpcoders.com.au/AmoebasSecret.html)
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