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Science, the Poetry of Reality, Jewel in Humanity's Crown

Aristotle was tutor to Alexander the Great. You could be the tutor of Aristotle. And thrill him to the core of his being. Aristotle was one of the greatest intellects of all time. But you know far more. You have a deeper, more penetrating, more comprehensive understanding of the way the world wo ...
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Not Knowing is Most Intimate

The Second Law of Thermodynamics requires that everything always is trending toward entropy. We plunge towards the random and chaotic. Entropy points the arrow of time in just one direction, and we will not return here. For us, the Conquering Heroes entered battle and valiantly arose victorious, and now the parade is literally over and we face a long offseason. Already the Message Board demands to know what next year will provide. We ask how long we can enjoy this feeling while we already feel i...
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The Weekly Carboholic: Pew poll says climate lowest priority, but results are curious

Pew poll says climate lowest priority, but results are curious Talking heads continue to confuse weather for climate Study says some climate changes cannot be reversed NOAA research jet measures greenhouse gases around the Pacific Study says oceans to dissolve much less oxygen Waste heat to eventually overwhelm greenhouse gases New magnets may replace HFC…
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Exposing the glaring errors in Climatology Energy Budget diagrams

Above is an early "Energy Budget" diagram for Earth published by NASA. The only trouble is that when we quantify the 51% of solar energy shown as being absorbed by land and oceans we get about one-eighth of the solar constant, resulting in a figure of about 168w/m^2 that could not achieve a global mean temperature above 233K which is -40°C. Yes, that is a minus sign, and yes
Josef Loschmidt Roy Spencer Raymond Pierrehumbert Energy Budget Stefan Boltzmann Law Second Law

To understand the physics relating to supposed greenhouse gas warming you need to understand the Stefan-Boltzmann Law.

The Stefan-Boltzmann Law in physics enables us to determine not only the outward radiative flux from a body at a certain temperature, but also the maximum equilibrium temperature that any given single source of radiation could achieve in a target. There are online calculators such as here to which you may wish to refer. If you enter one (1) for both the emissivity and the
Stefan Boltzmann Law For Earth Second Law Surface Temperatures

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