Some Climate Science for Nuclear Scientists - HCH

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Some Climate Science for Nuclear Scientists Submitted to Nuclear News. Rejected on the grounds that it is not specifically about nuclear. (Never mind the editorials in NN about how nuclear will save the world from “climate change.”) Howard “Cork” Hayden, Prof. Emeritus of Physics, UConn corkhayden@comcast.net January 21, 2022

ABSTRACT Everybody in the nuclear industry is familiar with the erroneous conclusion that since power plants emit radiation it is dangerous. The problem is one of scale, or course. Exposure to radiation from a power plant is minuscule, but non-zero, and that gets mathematically challenged people up in arms. In a similar vein, it is true that adding CO2 to the atmosphere causes some global warming. Again, the problem is one of scale. Herein, we will discuss the relevant unassailable physical laws and delve into the numbers.

INTRODUCTION If we add some heat to a fixed amount of water in a well-insulated container, we can easily calculate the temperature rise. If we add some heat to (say) a conference room (with no people present) that has excellent insulated walls as well as tables, pitchers of water, chairs, draperies, slide projectors, and so forth, we can calculate the temperature rise if we account for all masses and specific heats. Now imagine adding a certain heat flux (in watts per square meter) all over the earth. The temperature rise of a square meter of puddle will be considerably different than the temperature rise of a square meter of ocean, a square meter of snow, a square meter of leaf, a square meter of sand or a square meter of rock. To do a proper evaluation, it would be necessary to know the specific heats and masses of everything, as well as the amounts of ice that could melt and the amount of water that could evaporate. Of course, if that heat flux impinges on something thin that has low thermal conductivity, the fraction of heat radiated away will be higher than the fraction that penetrates through the object. Get out your supercomputer! It is thus a fool’s errand to try to answer that question. If we turn the question around, however, we get unambiguous answers on a slide rule: If the temperature of the surface of the earth rises (say) 1ºC, how much more heat does it radiate? This simple question is the key to evaluating the results of climate models.

STEP 1: PLANETARY HEAT BALANCE Absent any significant source of energy within a planet, at equilibrium the heat the planet absorbs from the sun will equal the heat radiated to space. If the solar flux at orbit is Isun, the flux averaged over the spherical surface is Isun/4. Every planet reflects some sunlight with its own albedo (reflectivity) α, so the absorbed sunlight is

. It follows that

(1) Before going on to the next step, note that Equation 1 shows that the infrared emission to space at equilibrium depends on exactly two variables: the solar intensity at orbit and the albedo of the planet. The 1


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