- 23 Sep 2023 05:21
#15288155
Right,
Also, IMO, even if the air didn't mix, the CO2 molecules absorb the infrared=heat photons from above and below and don't heat up much. Instead, they reradiate the heat photons in all directions. Near the ground the heat photons going down hit the ground. At some altitude there is not enough CO2 to absorb all the heat photons, so the ones going up go pretty far before they are absorbed again. This means that the air at that altitude cools a little. And so, the heat photons escape toward space and then to space.
The experiment doesn't have this effect.
We use satellites to measure the heat photons coming up and out to space. So, we know for sure that they are escaping to space.
Pants-of-dog wrote:So I will ignore that whole tangent on convection that you supplied as an explanation for the lab experiment.
Now, would you like to discuss how convection works in the atmosphere and makes the lab experiment irrelevant?
https://journals.aps.org/pr/abstract/10 ... ev.38.1876
From the known amounts of the various gases of the atmosphere from sea level to about 20 km, from the observed light absorption coefficients of the gases and from the albedo of the earth's surface the temperature of the atmosphere in radiative equilibrium is calculated on the assumption that the sunlight is the only source of energy. The calculation is perhaps more rigorous than has hitherto been attempted, although it contains a number of approximations. The sea level temperature comes out to be about 19° above the observed world-wide average value 287°K, and the temperature above about 3 km falls many degrees below the observed temperatures. The temperature gradient in levels from 3 to 6 km is greater than that of convective equilibrium and hence the atmosphere would not be dynamically stable if radiation equilibrium prevailed. Therefore air currents take place to bring about convective equilibrium. Continuing the calculation it is found that only when the convective region extends to about 12 km (as is observed), with radiative equilibrium above 12 km (as is observed), does the atmosphere satisfy the conditions of dynamic stability and thermal equilibrium with the received solar energy. For this case the calculated sea level temperature is 290°K in good agreement with the observed value 287°K. Calculation shows that doubling or tripling the amount of the carbon dioxide of the atmosphere increases the average sea level temperature by about 4° and 7°K, respectively; halving or reducing to zero the carbon dioxide decreases the temperature by similar amounts. Such changes in temperature are about the same as those which occur when the earth passes from an ice age to a warm age, or vice versa. Thus the calculation indicates that the carbon dioxide theory of the ice ages, originally proposed by Tyndall, is a possible theory.
Received 9 October 1931
So, Angstrom was correct that the air quickly became unable to absorb any more infrared, but his lab experiment did not account for convection, as you just pointed out.
When convection is applied, we see that convection moves the air around and this then mixes the air and spreads the heat around for the first 12 km above sea level.
So when discussing anthropogenic climate change, it is not relevant to discuss what is happening in the first 12 km. Instead, we need to look at the heat interactions above that level.
Right,
Also, IMO, even if the air didn't mix, the CO2 molecules absorb the infrared=heat photons from above and below and don't heat up much. Instead, they reradiate the heat photons in all directions. Near the ground the heat photons going down hit the ground. At some altitude there is not enough CO2 to absorb all the heat photons, so the ones going up go pretty far before they are absorbed again. This means that the air at that altitude cools a little. And so, the heat photons escape toward space and then to space.
The experiment doesn't have this effect.
We use satellites to measure the heat photons coming up and out to space. So, we know for sure that they are escaping to space.