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::To answer your last point first, I'd say your comments show good faith, and a helpful and entirely appropriate attempt to get to the core of the (potential) dispute.   
 
::To answer your last point first, I'd say your comments show good faith, and a helpful and entirely appropriate attempt to get to the core of the (potential) dispute.   
 
::On one level, we may just be talking past each other.  I say "delay" because excited molecules will eventually relax, and new photons (in a different spectrum) are emitted.  Your comments suggest that you mistakenly believe that all of the energy of a black body photon is permanently returned to the Earth as thermal energy just because it's absorbed by an atmospheric molecule.  But the molecules that are excited this way have much more of a tendency to shed the energy through re-radiation than mere black-body radiation.  These molecules shed energy through a couple of different mechanisms, including new photon emission directly radiated into space, as if the energy was never absorbed in the first place.  Other mechanisms are less direct, and therefore take longer; still others really do end up dumping the energy back into the Earth as thermal energy.  Thus, to fully describe the effect of the absorbtion of photons at a given quantum of energy, you need a graph over time that shows the expectation value of the fraction of that energy that ends up being radiated into space anyway.  It may be that a physical chemist's training is better suited to the task of calculating that curve from first principles, but, from my perspective as a physicist, I'd say that the curve needs to be measured empirically.  Worse, it needs to be calculated for each quantum of energy throughout the absorbtion spectrum, because the tendency of a molecule to want to relax through photon emission is a function of its quantum mechanical properties (and because the re-emitted photons are in a different spectrum, and, therefore, not likely to be absorbed by primary greenhouse molecules).  The shapes of these curves are the major unknown I'm pointing to. [[User:QBeam]]
 
::On one level, we may just be talking past each other.  I say "delay" because excited molecules will eventually relax, and new photons (in a different spectrum) are emitted.  Your comments suggest that you mistakenly believe that all of the energy of a black body photon is permanently returned to the Earth as thermal energy just because it's absorbed by an atmospheric molecule.  But the molecules that are excited this way have much more of a tendency to shed the energy through re-radiation than mere black-body radiation.  These molecules shed energy through a couple of different mechanisms, including new photon emission directly radiated into space, as if the energy was never absorbed in the first place.  Other mechanisms are less direct, and therefore take longer; still others really do end up dumping the energy back into the Earth as thermal energy.  Thus, to fully describe the effect of the absorbtion of photons at a given quantum of energy, you need a graph over time that shows the expectation value of the fraction of that energy that ends up being radiated into space anyway.  It may be that a physical chemist's training is better suited to the task of calculating that curve from first principles, but, from my perspective as a physicist, I'd say that the curve needs to be measured empirically.  Worse, it needs to be calculated for each quantum of energy throughout the absorbtion spectrum, because the tendency of a molecule to want to relax through photon emission is a function of its quantum mechanical properties (and because the re-emitted photons are in a different spectrum, and, therefore, not likely to be absorbed by primary greenhouse molecules).  The shapes of these curves are the major unknown I'm pointing to. [[User:QBeam]]
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:::I think you are right, we are just talking past each other. It seems that physicists and chemical engineers go about explaining things in different ways (for example the photon/wave difference)!
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:::As for the time vs. emission graph, I'm not sure it's necessary. The number of particles is large enough and close enough to uniform distribution that the effect can be modeled on the aggregate level. I don't think you need or want me to get into the specific calculations, but the radiation balance on the earth can be modeled the same way you would model any other system. It follows the same principle as figuring out the steady state temperature of a roof in full sunlight in the wintertime. [[User:HelpJazz|Help]][[User talk:HelpJazz|Jazz]] 19:39, 30 October 2007 (EDT)
    
::Now, regarding my third point, the logistical curve, let me try to reformulate.  There are a certain, relatively fixed number of ergs/year emitted by the Earth in CO2's absorbtion spectrum.  (Your point about the spectum being T dependent is correct, but of small effect, since T==300K and delta-T<~3.)  The maximum greenhouse effect would have every one of those ergs absorbed (and then a certain fraction of them would be re-emitted anyway in other spectra, and the rest "trapped").  Call that fraction, as a function of the amount of CO2, x(C).  For any incremental increase in CO2, delta-C, the number of ergs retained is proportional to (1-x(C)).  Logistical curves behave this way--logarithms do not.  In short, the horizontal asymptote of a logarithm is infinity, but the horizontal asymptote (and upper bound) on the greenhouse effect is finite.  [[User:QBeam]]
 
::Now, regarding my third point, the logistical curve, let me try to reformulate.  There are a certain, relatively fixed number of ergs/year emitted by the Earth in CO2's absorbtion spectrum.  (Your point about the spectum being T dependent is correct, but of small effect, since T==300K and delta-T<~3.)  The maximum greenhouse effect would have every one of those ergs absorbed (and then a certain fraction of them would be re-emitted anyway in other spectra, and the rest "trapped").  Call that fraction, as a function of the amount of CO2, x(C).  For any incremental increase in CO2, delta-C, the number of ergs retained is proportional to (1-x(C)).  Logistical curves behave this way--logarithms do not.  In short, the horizontal asymptote of a logarithm is infinity, but the horizontal asymptote (and upper bound) on the greenhouse effect is finite.  [[User:QBeam]]
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:*The problem is, you are assuming good faith.  Unfortunately on the Internet that is at the top of the charts for never happening.  QBeam was stringing together buzz words and silly science in the hope they would lend creditability to his/her post, a fact you just proved, HelpJazz.  --<font color="#1E90FF" face="Comic Sans MS">[[User:TK|şŷŝôρ-₮K]]</font><sup><font color="DC143C">[[User_Talk:TK|/Ṣρёаќǃ]]</font></sup> 01:01, 20 October 2007 (EDT)
 
:*The problem is, you are assuming good faith.  Unfortunately on the Internet that is at the top of the charts for never happening.  QBeam was stringing together buzz words and silly science in the hope they would lend creditability to his/her post, a fact you just proved, HelpJazz.  --<font color="#1E90FF" face="Comic Sans MS">[[User:TK|şŷŝôρ-₮K]]</font><sup><font color="DC143C">[[User_Talk:TK|/Ṣρёаќǃ]]</font></sup> 01:01, 20 October 2007 (EDT)
 
::If you believe you can identify an error in my (or anyone's) reasoning, then you should point that out.  Vacuous cheer-leading like this only serves to discredit whatever ideology it is you think you're representing.  Simply labeling something a "buzzword," even if it were accurate, is not a substantive response.  [[User:QBeam]]
 
::If you believe you can identify an error in my (or anyone's) reasoning, then you should point that out.  Vacuous cheer-leading like this only serves to discredit whatever ideology it is you think you're representing.  Simply labeling something a "buzzword," even if it were accurate, is not a substantive response.  [[User:QBeam]]
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:::I dunno, if it's buzzwords it sure fooled me (twice)! [[User:HelpJazz|Help]][[User talk:HelpJazz|Jazz]] 19:39, 30 October 2007 (EDT)
    
== Article is Thin ==
 
== Article is Thin ==
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