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= CO2 Spectrum = | = CO₂ Spectrum = |
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I don't understand cycles/cm very well. The speed of light is 3e10 cm/s, so multipliy 600 to 800 cycles/cm to get 18 to 24 THz. | I don't understand cycles/cm very well. The speed of light is 3e10 cm/s, so multiply 600 to 800 cycles/cm to get 18 to 24 THz. |
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------ Here's the CO₂ absorption spectrum from NIST: ( http://webbook.nist.gov/cgi/cbook.cgi?ID=C124389&Type=IR-SPEC&Index=1#IR-SPEC ) {{attachment:NIST2.png | | width=800 }} This first graph shows absorption out to 3700 cycles/cm ( about 110 THz ). The strongest and broadest peak is at 2300 cycles/cm (about 70 THz), but this peak is irrelevant; The Earth is 220K to 300K (depending on where you look) so this is well above the earth's black body emission peaks (400 to 600 cycles/cm), in the quantum-limited exponential rolloff region. It is also well below the sun's black body emission peak of 11,300 cycles/cm at 5780 K. The peak that matters to us is within the 100 to 1500 cycles/cm window, shown below. ---- {{attachment:NIST5.png | | width=800 }} The interesting aspect of this peak is that it is broad, not sharp, with long tapering tails to the side. MoreLater |
CO₂ Spectrum
From Global Warming, Understanding The Forecast by David Archer, Blackwell 2007, without permission. Buy the book for a lucid explanation of the science; perhaps the author and publisher might forgive me for posting the excerpt below.
I don't understand cycles/cm very well. The speed of light is 3e10 cm/s, so multiply 600 to 800 cycles/cm to get 18 to 24 THz.
Here's the CO₂ absorption spectrum from NIST: ( http://webbook.nist.gov/cgi/cbook.cgi?ID=C124389&Type=IR-SPEC&Index=1#IR-SPEC )
This first graph shows absorption out to 3700 cycles/cm ( about 110 THz ).
The strongest and broadest peak is at 2300 cycles/cm (about 70 THz), but this peak is irrelevant; The Earth is 220K to 300K (depending on where you look) so this is well above the earth's black body emission peaks (400 to 600 cycles/cm), in the quantum-limited exponential rolloff region. It is also well below the sun's black body emission peak of 11,300 cycles/cm at 5780 K. The peak that matters to us is within the 100 to 1500 cycles/cm window, shown below.
The interesting aspect of this peak is that it is broad, not sharp, with long tapering tails to the side.