The English translation
repeats the differential equations, and the solution is given in the
specified form for Gold's problem.
While
in Schwarzschild's original terms it is evident from one sight that the
difference of A and E, the net radiation at the lower boundary, is
unequivocally equal to A
0/2, independently of
the optical
depth, it is less straightforward in Emden's formulation of the
solution, and even less obvious in the English translation.
Therefore,
from the viewpoint of Manabe-Moller and Manabe-Strickler, the emphasis
in this research was not on Schwarzschild's equations, but on Emden's
solution. But with this shift of focus, the right-hand side of the
equation, its constrained character, and the prescribed magnitude,
finally disappeared.
The books an atmospheric physics and
radiation brought back Schwarzshild's equations into the
attention, but the climate papers went on computing temperature changes
by the greenhouse gases and simulated Earth's climate through computer
models, where the changes in convection were functions of the surface
temperature, but not restricted by radiative transfer constraints.
Manabe (971), Manabe and Wetherald (1967, 1975, 1980) are talking about
climate sensitivity without mentioning the existence of the constrained
character of surface net radiation.
Their followers,
Ramanathan and Coakley (1978), Ramanathan et al. (1979), and The
Charney Report (1979) do not refer to Schwarzshild's constraint,
although at that time it was already there in Goody (1964, Mentzel
(1967), Houghton (1977), Chamberlain (1978), and so on.
And finally, it it missing from all the IPCC Reports (1990-2021).
In
1991, Dr. Graeme Stephens had a huge opportunity to re-introduce
Schwarzschild to the climate community. When the GEWEX project was
initiated, he wrote four papers in the Earth's radiation budget and its
relation to atmospheric hydrology (JGR), and in the first paper he took
the equations from Mihalas (1978) and from Goody and Yung (1989), in
this form:
The
first equation is the upward beam (the second term) in Schwarzshild
(1906, eq. 11), and the second equation is the emission at the surface
(the first term); therefore their difference must give the net
radiation at the surface (the third, unnumbered equation). But because
of a technical misuse, a division by two was lost on the right-hand
side, therefore the third (unnumbered) equation incorrectly connects
net radiation at the surface to the effective emission, thus their data
evidently didn't fit, so this approach proved unuseful.
The fourth paper of the series (1994) gives the equations correctly:
Here
the first equation is still the middle-term is Schwarzschild (1906,
eq.11), but the second equation is not the first term (the emission of
the layer), but the third term (the downward emission). So here the net
radiation can be calculated correctly is F
∞/2,
but it is not expressed explicitly. This problem could have been
avoided if he took the equations directly from Schwarzschild.
But
finally, the all-sky version of this equation, together with its
total-energy counterpart, is verified with a difference of 0.1 Wm-2 in
the most recent, and most comprehensive study on 30 years of GEWEX, by
Stephens and Coauthors (2023, BAMS).
***