Start with section 4.2 in the multi megabyte chapter I'd referred to before:
Read carefully forward from there to the two-stream equations (4.8) on page 143, which are an important key, then proceed on towards a paragraph that just follows equation (4.37) on page 154, where the author writes, "For constant k, most gases would produce a deep stratosphere in the optically thick limit. This conclusion is greatly altered by pressure broadening." Then proceed a little further on.
I think John's problem on this subject is that he won't actually seriously engage himself to _read_ anything on the subject unless perhaps he already expects it to support his essentially ignorant (and I don't mean the term itself in a cruel way, just a factual one about what he actually _knows_ about the subject), preconceived notions. It turns out that there are very good theory confirmed by extensive and broad-reaching experiments, as fully quantitative as anyone has any business caring about -- at least, as an outsider looking in. There are very detailed discussions John _could_ read, if he'd a mind to inform himself instead of just speaking out from his imagination coupled to mostly ignorance on the subject, instead.
There is an adage in computer programming -- "If it doesn't have to work, a program can be very short." One of the really nice things about having a fascile imagination that doesn't have to be well coupled to reality is that there is no limit to where one can fly with it. It's a lot of fun to let your "imagination balloon" drift far away from and high above the ground of harsh reality. And if your imagination doesn't have to conform to experimental result and earlier prosaic theory, showing off with new ideas is very quick and easy to do.
Like some facets of electronics design, the details of the exact mechanisms of global warming are non-trivial and most of the simplistic explanations one finds on the web, many more well meaning ones included, are simplified to the point of near-useless distortion. Even my earlier simplification, the idea of "replacing higher temperature Planck radiation at lower altitudes with lower temperature Planck radiation at higher altitudes," can only be taken so far. It cannot be used to deduce to specifics -- it is a short-hand notation about the consequence of other theories applied to our circumstances and not a theory itself. But it does provide a nutshell explanation, if one doesn't care about the details.
Some early scientists including some up through the early 1970s, lacking future knowledge on the subject or unable or unwilling to think more closely about what they did know at the time, have been misled in their conclusions. Which is part of the reason why I recommended the historical exhibits at the American Institute of Physics:
Among those exhibits, are pages on the Discovery of Global Warming:
As well as Rasool & Schneider's 1971 paper, which provides a very interesting capstone to the earlier period where there remained some fundamental confusions over the details with some serious scientists.
Some of those from the exhibits I cited were:
Some more are:
All of those are linked from this, though:
If one merely reads this much, they will begin to understand why pressure broadening not only has the meaning mentioned quantitatively in the chapter I referred to:
But also how it is that a lack of adequate resolution in spectroscopy in the earlier years, a lack of understanding of pressure broadening near ground level versus in the stratosphere, a lack of understanding the differences of pressure broadening of CO2 when it is the only gas at a particular pressure versus its different pressure broadening when it is in the presence of N2 and O2, etc., can lead otherwise intelligent and well-educated physicists towards wrong conclusions.
The upshot is that there is a great deal more known now in terms of theory, instrumentation is vastly more precise and well understood, and there is a lot of very good deductions to specifics from excellent theory that might serve to better inform anyone caring to try. (A bit of facility with understanding differential equations covers a lot here. But that's not an unusual skill for those in electronics design. It's part of the undergrad coursework, in fact.)
At least having some basic understanding of the history of the science in this area would help -- even if one fails to study the equations and their development. I've provided a link to a chapter where someone can go, for free, if they have a mind to... including the role that pressure broadening plays both in the detailed theories as well as in the fitful history of the field.
One can lead a horse to water, but cannot make them drink. Oh, well.
Jon