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 The Lavoisier Group 2007 Workshop Rehabilitating Carbon Dioxide 'Rehabilitating Carbon Dioxide': An Overview 
  Ray Evans 
 The papers presented at the Lavoisier Group's Workshop
  Rehabilitating Carbon Dioxide held in Melbourne on 29th
  and 30th June 2007, covered the two most important scientific
  issues at the heart of the current debate over global warming
  and its causes. The first is the influence, if any, of atmospheric
  carbon dioxide on the earth's climate. The second is the very
  well documented correlation between sunspot activity and climate
  changes during the last 1500 years or more. In addition, two papers were given on economic issues that
  are consequent to the claims of anthropogenic control of our
  climate. The paper by Alex Robson discusses the Shergold Report,
  a report commissioned by the Prime Minister from a committee
  chaired by the Secretary of the Department of Prime Minister
  and Cabinet, Peter Shergold, on the merits of a cap and trade
  scheme of licences required by law to emit carbon dioxide. The
  paper by Tim Curtin analyses the Stern Review, a report published
  with great fanfare in October 2006 and submitted to the then
  UK Chancellor of the Exchequer, Gordon Brown, on the costs and
  benefits of introducing a regime of decarbonisation for the UK. It is noteworthy that Sir Nicholas Stern was released by Gordon
  Brown the day after the latter's Budget failed to adopt any of
  Stern's recommendations, but Peter Shergold continues as Secretary
  of PM&C. This overview will discuss the two key science issues of this
  debate; first the influence of atmospheric carbon dioxide on
  climate; and second the connection between sunspots and climate. It has been understood for at least twenty years that the
  physics of black-body radiation, described in the Stephan-Boltzmann
  black-body radiation curves (which used to be taught in high
  school physics courses), coupled with the radiation properties
  of carbon dioxide molecules, lead inexorably to the conclusion
  that once concentrations of carbon dioxide in the atmosphere
  exceed 50 ppmv, further increments of CO2 have an ever declining
  influence on the radiation balance at the outer surface of the
  atmosphere, and thus on the earth's temperature. The greenhouse
  contribution of CO2, already very small when compared with water
  vapour, gives the same small increase in global temperatures
  as it increases from 100 to 200 ppmv, from 200 to 400 ppmv, from
  400 to 800 ppmv, and from 800 to 1600 ppmv. Each doubling of
  CO2 yields a predicted 0.4 deg C increase in temperature, an
  increment which can be overwhelmed by changes in cloud cover
  in the lower atmosphere. This understanding of basic physics is briefly discussed in
  the 1990 IPCC's First Assessment Report but has not been mentioned
  in IPCC publications since. It was covered at length in David Archibald's paper, in Bill
  Kininmonth's paper, in Michael Hammer's paper, and in Tom Quirks'
  analysis of atmospheric carbon 14, and the implications are far
  reaching. It means that atmospheric carbon dioxide has played
  virtually no role in influencing our climate since concentrations
  exceeded 200 ppmv during the last glacial maximum 20,000 years
  ago, and will play no discernible role in the future, regardless
  of the size of any increase of these concentrations. All of the
  huffing and puffing at the G8 or wherever these issues are discussed
  by heads of government and their officials is completely beside
  the point. Whether anthropogenic emissions of carbon dioxide
  are reduced or increased will make no discernible difference
  to the radiation balance and thus to global temperatures. This is so basic a point, and so terminal for the decarbonisation
  ambitions of the Environmentalist movement, that it is a matter
  of concern and astonishment that it has not been pursued by the
  Kyoto sceptics (such as the Lavoisier Group) far more vigorously
  than it has been. Whatever our sins of omission in the past have
  been, we will be trying to make amends in the immediate future. If carbon dioxide (once it has exceeded 50 ppmv) has virtually
  no impact on the radiation balance and thus on climate (and there
  was never any evidence that it did) where can we find some rational
  explanation for the climatic changes that have taken place during
  the last two millennia, for example the Roman Warm Period, the
  Mediaeval Warm Period, the Little Ice Age, and the warming which
  has taken place since about 1880, the 20th Century Warm Period? Two papers at the workshop discussed the long-established
  connection between sunspots and climate. One of the earliest
  learned papers on this topic was written in 1801 by the discoverer
  of the planet Uranus, William Herschel, who found an excellent
  correlation between the history of wheat prices given by Adam
  Smith in the Wealth of Nations and the sun spot cycle
  for the same period. David Archibald took his analysis of this
  phenomenon to the point where he predicted a repeat during the
  next 23 years of the Dalton Minimum of 1796 to 1820, a period
  of low temperatures, little sunshine, and severe food shortages
  in Europe, particularly in Britain, which experienced a year
  without summer in 1816. Will Alexander discussed the river flow records from the Nile,
  which go back to 640 AD, the longest record of its kind, and
  the 22-23 year periodicity which characterises that record. So the connection between sunspots and climate change has
  long been observed but, up until 2005, never been explained.
  And here we introduce Henrik Svensmark, the Danish physicist,
  who in December 2004 began his experiments in the basement of
  a university building in Copenhagen which eventually proved that
  cosmic rays from far beyond the solar system, called galactic
  cosmic rays, were primarily responsible for initiating cloud
  formation in the lower atmosphere. This was the missing link in the chain of causation between
  sunspots and climate. The first step in the chain is the realisation
  that sunspots are a manifestation of dramatic changes in the
  Sun's magnetic field. This immense field, which projects solar
  influence far out into space, and which envelopes the earth,
  exhibits a 22-23 year cycle, the Hale cycle, or two sunspot cycles
  back to back. (Each sunspot cycle of approximately 11 years is
  called the Schwabe cycle.) When the solar magnetic field is strong,
  it protects the earth from galactic cosmic rays, and thus cloud
  formation is greatly diminished. When it is weak (as during the
  Dalton Minimum) then cosmic rays penetrate easily into the lower
  atmosphere and cloud cover is correspondingly increased. Clouds are the big influence on our climate. When abundant,
  they reflect the Sun's radiation back into space and the earth
  gets cold. When sparse, the Sun's radiation travels unimpeded
  to the surface of the earth and the earth warms. Cloud cover
  is the driver of climate, and cosmic rays determine in large
  measure the extent of that cloud cover. The General Circulation Models, which are used by the IPCC
  to predict the response of the earth to increasing atmospheric
  carbon dioxide, describe cloud behaviour very badly. The representation
  of clouds is largely statistical and thus ignores interaction
  with terrestrial radiation and the energy exchanges of the hydrological
  cycle. More recently, it has been shown that the computer models
  underestimate the variation of surface evaporation and precipitation
  with changing surface temperature, a fatal flaw in the projection
  of changing surface temperature with radiation forcing. These computer models, then, which have soaked up billions
  of dollars in programming and computer time, are worthless. Svensmark should win the Nobel prize for his pioneering work
  in this field and the basement which housed his big box containing
  atmospheric gas will become as famous as the squash court at
  the University of Chicago where Enrico Fermi built the first
  atomic pile and demonstrated the first nuclear chain reaction. Having completed the chain of causation from sunspots to climate,
  the next big step forward is in predicting the future behaviour
  of the Sun's magnetic field. David Archibald presents a number
  of different forecasts, but on the basis of empirical rules opts
  for a repeat of the Dalton minimum. Svensmark himself is much more cautious. In the book co-authored
  with Nigel Calder The Chilling Stars: A New Theory of Climate
  Change, published in Australia by Allen and Unwin, they
  write (p 222): 
      Cosmic rays conform only loosely with the sunspot count.
      Although generally high when sunspots are few, and reduced when
      there are many, there is no simple one-one connection. The next few years will be exciting for those who are involved
  in this field of scientific activity. If we experience something
  like a repeat of the Dalton Minimum the anthropogenists will
  have a lot of crow to eat, but that will be of small consequence
  compared with the economic upheavals caused by loss of agricultural
  production in the grain growing regions of North America and
  Northern Europe. Australian agricultural production will become
  more important in such a situation. It is important at this time that Australia does nothing to
  impede its economic growth and its potential to play an increasingly
  important role in the global economy. The Shergold endorsement
  of a carbon emissions trading scheme is arguably one of the most
  lunatic documents in the history of official advice to Australian
  governments, and it should be buried without delay. If the next
  twelve months give us continuing cool weather, high rainfall
  and consequent flooding, then there is a real chance that such
  burial can take place without too much fuss. Climate change has played a pivotal role in human history.
  During the Mediaeval Warm Period (850-1300 AD) European civilisation
  made huge progress in the arts and sciences, in agriculture,
  in technology, and in the formation of cities such as Florence,
  Milan, Genoa, and Venice, where the foundations of our market
  economies were established. With the advent of the Little Ice
  Age, Europe suffered a massive loss of population and it was
  not until 1550 that the population recovered to pre-1300 levels. The belief that mankind can 'stop climate change' by decarbonising
  our economy is as irrational a belief as one can find in any
  primitive religion. But in legislating for carbon emission trading
  schemes we are declaring our commitment to superstition of the
  most primitive kind. If the recent discoveries of the power of
  galactic cosmic rays to influence cloud formation become more
  widely known, faith in anthropogenic carbon dioxide as the controlling
  force on climate will become a joke and Australia will be able
  to build urgently needed power stations, and develop major natural
  gas fields, without the burden of sovereign risk now attending
  such investments. Let us achieve this ambition as soon as possible.
 
 
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