Contact:
Michele Forsten or Alka Gupta
718/488-1015
michele.forsten@liu.edu
Brooklyn, NY — An unusual interdisciplinary study by astronomers and climatologists has found a striking correlation between holes in the outermost layer of the sun — or the corona — and the globally averaged temperature of the Earth, suggesting that the Earth’s atmospheric temperature may be strongly linked to solar magnetism changes over months or years.
In a paper that appears in the February 28 issue of the journal New Astronomy, climatologist Eric Posmentier of Long Island University’s Brooklyn Campus, solar physicists Willie Soon and Sallie Baliunas of the Harvard-Smithsonian Center for Astrophysics and physicist Pius Okeke of the University of Nigeria chart temperature anomalies seen in the Earth’s lower troposphere (i.e., the region of atmosphere in which we live) using Microwave Sounding Unit (MSU) radiometers aboard weather satellites.
The scientists compared the Earth’s temperature with the size of coronal holes reported on the Sun during a two-decade period, starting in January 1979 and ending April 1998. Results show a clear drop in terrestrial atmospheric temperature after the Sun’s magnetic field activity is most intense. At this point, there is a dropping off of magnetic activity and an enlargement of the coronal holes. "This is the first time anyone has combined these modern, reliable data sets to link solar activity and climate, and to cite several alternative mechanisms that might explain this link," Posmentier explained.
Coronal holes are, literally, gaps in the Sun’s outer atmosphere through which the stream of hot, supersonic particles known as the solar wind pours out into space to engulf the entire planetary system. At Earth, this hot bath of charged particles produces the aurorae (i.e., the aurora borealis), interferes with electrical and radio transmissions, and may threaten passengers aboard high-flying airliners or astronauts aboard unshielded spacecraft. The solar wind has also been long suspected as a possible indirect contributor to terrestrial climate change.
Posmentier and colleagues think that the connection between the solar wind and climate may be more direct, suggesting that the charged particles hitting the Earth’s atmosphere may affect the properties of terrestrial water clouds, particularly the percentage of those clouds covering the Earth. In turn, significant changes in the cloud cover influence the temperature of the lower troposphere, with temperatures falling with increased cloud cover. Another possibility is that the charged particles change ozone chemistry in the upper atmosphere, in turn affecting the dynamics of the climate.
The scientists note, however, that the charged particles hitting the Earth could come from either the Sun, or from galactic cosmic rays that are modulated by the solar wind. Or, from a combination of both sources. Regardless, the percentage of the Sun’s surface covered by coronal holes seems to be a fairly accurate indicator of temperature in the Earth’s troposphere over months or years.
The correlation comes with some caveats. As Posmentier and colleagues note, other major climate factors are also at work concurrently, thus complicating attempts to correlate Sun-Earth phenomena. Most notable in the past two decades have been the warming effects of the 1997-98 El Nino and the general cooling that followed the eruption of Mount Pinatubo in 1991.
According to Posmentier, their results do not rule out the possible climate influence of man-made fossil fuels, which have caused the atmosphere’s CO2 levels to rise. "During some parts of the last century, as the amount of CO2 increased, the temperature increased," he explained. "I don’t dispute that, and I’m not saying that CO2 can’t have significant effects in the future.
"What I am saying is the data do not unambiguously support the contention that CO2 increases are the dominant cause of climate variability," he added. "There are other reasons for climate variations that are significant. In fact, we’ve found that the strongest correlation is the one between the area of the Sun’s surface covered with holes and the globally averaged temperature of the Earth."
Support for this research came from the Mount Wilson Institute and the Electric Power Research Institute, with additional funding from the Massachusetts Space Grant Consortium, the Smithsonian Institution, the Richard C. Lounsbery Foundation, and NASA.
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Editors, please note: For a full-text version of the New Astronomy paper, click on http://www1.elsevier.com/journals/newast .
For more information, contact:
* Dr. Eric Posmentier
Long Island University
718-780-4163, posmentier@mindspring.com
* Dr. Sallie Baliunas
Harvard-Smithsonian Center for Astrophysics
617-495-7415, sbaliunas@cfa.harvard.edu
* Dr. Willie Soon
Harvard-Smithsonian Center for Astrophysics
617-495-7488, wsoon@cfa.harvard.edu
