Tom Shula explains how the behaviour of the Pirani gauge precludes any significant greenhouse gas effect: YouTube | white paper (pdf) | WUWT
We can use the behaviour of the Pirani gauge to estimate what kind of heat transport should dominate in each layer of the atmosphere. The IPCC say radiative cooling dominates everywhere in the atmosphere; even at ground level. They are completely wrong. Not because 'the science is wrong'; but because the politicos politicized the science so much - they make it up.
The Pirani guage implies:
mode of heat transport | pressure | altitude | regions |
convection | above 4 Torr | below 35km | troposphere, tropopause, lower stratosphere |
conduction | 0.1 to 4 Torr | 35 to 65 km | upper stratosphere, stratopause, lower mesosphere |
radiation | below 0.1 Torr | above 65km | above mid-mesosphere |
Derivation of table above
In his book "A User's Guide to Vacuum Technology", 3rd edition, John F. O'Hanlon's presents the following diagram on page 88 to show that as one goes from atmospheric pressure to a vacuum, the cooling of the Pirani gauge sensor wire is dominated, in turn, by convection, conduction and radiation - the 3 heat transport mechanisms.
O'Hanlon's diagram did not label the axis because the precise curve one gets depends on the gas. But both axis are logarithmic. The basic outline (shape) of the curve is the same for all gases. So we can superipose the points - where convection gives way to conduction, and conduction gives way to radiation - onto the diagram supplied by Tom Shula. The enables us to find specific pressures at which these cross-overs happen.
convection (iii) gives way to conduction (ii) | ~ 4 Torr | |
conduction (ii) gives way to radiation (i) | ~ 0.1 Torr (100 microns). |
The diagram below relates altitude to atmospheric region
Conclusions
mode of heat transport | pressurealtitude | regions | |
convection | above 4 Torr | below 35km | troposphere, tropopause, lower stratosphere |
conduction | 0.1 to 4 Torr | 35 to 65 km | upper stratosphere, stratopause, lower mesosphere |
radiation | below 0.1 Torr | above 65km | above mid-mesosphere |
The table below, found here, associates specific pressures with altitude.
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