dduggan47 wrote:
"gpobserver wrote:
Mr. Peterson also has a nasty habit of resorting to ad hominem attacks when pressed on a point.
I've been following this discussion from the day it started but I haven't kept track of who said what. I think you're probably right but I also think that he's a long way from being the worst offender. You imply that you've been polite and I certainly haven't noticed anything to the contrary (... and I'm not going to go back and look! ), so thank you for that."
If it was implied, I shouldn't have. I have tried to be polite and civil but I have occasionally failed, much to my embarrassment and chagrin. In one instance I was unecessarily rude to Mr. Mark Swain for which I shortly afterward apologized. I am only human and being addressed rudely does wear upon my patience. It is unfortunate that the global climate debate has become so politicized and emotionally charged. I am reminded of the "blue eye/brown eye" experiment of years ago (
http://www.janeelliott.com/,
http://www.pbs.org/wgbh/pages/frontline/shows/divided/ ). Some of the uglier aspects of human nature were revealed by this experiment. I'm of the opinion that this video, "A Class Divided", should be required viewing for all students, everywhere.
dduggan47 wrote:
"You also wrote that the sun is a simpler system. (I'm tempted to ask for a citation! ) I'll take your word for it but is it better understood than climate or even weather? That's not a shot, it's a real question."
A citation? Oh, goodness... I read this in an astrophysics text so long ago I couldn't recall which one. However, let's look at the facts. The sun's composition is principally hydrogen and helium with a small amount of heavier elements (referred to simply as 'metals' in astrophysics). This material was condensed from the interstellar medium of a neighborhood of the galaxy as it existed 4.6 billion years ago, approximately eight billion years after the Big Bang or whatever event it was that started our universe. At the time of the formation of our galaxy, the elemental composition of the universe was principally hydrogen, helium, and a bit of lithium. There was no significant production of elements heavier than lithium due to the very short lifetime (0.067 femtoseconds) of the radioactive isotope Be-8, formed when two helium nuclei collide with sufficient energy. The Be-8 would usually decay before another hydrogen or helium nuclei could fuse with it, producing a heavier nucleus. Lithium is a fossil element left over from the Big Bang. Nuclear reactions in stars only destroy it.
The sun's composition is generally pretty homogeneous except as you approach the core where the abundance of helium is being increased by nucleosynthesis. The sun is entirely a plasma, an electrically-conducting fluid, which is influenced by electric and magnetic fields in ways explained by classical electrodynamics. The nuclear reactions occurring at the core are generally well-understood and our understanding has been assisted by the observations of neutrinos produced by those reactions (
http://en.wikipedia.org/wiki/Neutrino). The internal structure of the sun has been studied by means of helioseismology (
http://en.wikipedia.org/wiki/Helioseismology,
http://gong.nso.edu/info/helioseismology.html). Energy is transported from the nuclear reactions in the core, first by radiation in the deeper regions of the sun (
http://en.wikipedia.org/wiki/Radiative_transfer), and then by convection nearer the surface. The size of a star is a balancing act between the force of gravity tending to compress the volume of compressible plasma and expansion produced by the internal heat source warming the plasma. There is some influence on this energy transport due to the 'metals' in the composition of the star increasing the 'opacity' of the material in the same way that so-called Greenhouse Gases do in our atmosphere. The luminosity of a Main Sequence (
http://hyperphysics.phy-astr.gsu.edu/hb ... errus.html) star is almost entirely a function of the total mass of the star.
As mentioned before, there are no continents, no oceans, no solid surface, no clouds, no precipitation, no biology, no chemistry, no external heat sources warming the surface (except for multiple star systems). About the only thing complicating this simple picture is the rotation of a star which introduces coriolis forces that influence the convection of the atmosphere. As simple as a star is, it is still difficult to predict many of its behaviors because of their chaotic nature. The course of future activity is sensitively dependent upon initial starting conditions. Yes, I will assert that a star is much simpler than a planet and its climate system. Simple but still difficult to predict in many ways. I am reminded of what we used to say in experimental biology, "Under precisely controlled and duplicated experimental and environmental conditions, an experimental animal will do whatever it damned well pleases."
dduggan47 wrote:
"As for the citation you did provide, I promise to read it in its entirety when you send me $85. Can you paraphrase relevant passages?"
Oh my! My intent was to present that as a thousand page example of the volume of knowledge we have of the sun and its history. After all these years I still haven't read all of my copy.
dduggan47 wrote:
"If I'm smart now I'll go back to lurking. I'm well over my head."
An important thing is to never stop seeking new knowledge.
I've enjoyed chatting with you, Sir.
Best regards,
- Roy Tucker