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Sunspot Activity at 8,000-Year High

By Robert Roy Britt
Senior Science Writer
posted: 27 October 2004
12:58 pm ET

Sunspots have been more common in the past seven decades than at any time in the last 8,000 years, according to a new historic reconstruction of solar activity.

Many researchers have tried to link sunspot activity to climate change, but the new results cannot be used to explain global warming, according to the scientists who did the study.

Sunspots are areas of intense magnetic energy. They act like temporary caps on upwelling matter, and they are the sites of occasional ferocious eruptions of light and electrified gas. More sunspots generally means increased solar activity.

Sunspots have been studied directly for about four centuries, and these direct observations provide the most reliable historic record of solar activity. Previous studies have suggested cooler periods on Earth were related to long stretches with low sunspot counts. From the 1400s to the 1700s, for example, Europe and North America experienced a "Little Ice Age." For a period of about 50 years during that time, there were almost no sunspots.

But a firm connection between sunspot numbers and climate remains elusive, many scientists say.

Better record

The new study, led by Sami Solanki of the Max Planck Institute in Germany, employed a novel approach to pinning down sunspot activity going back 11,400 years:

Cosmic rays constantly bombard Earth's atmosphere. Chemical interactions create a fairly constant source of stuff called carbon-14, which falls to Earth and is absorbed and retained by trees. But charged particles hurled at Earth by active sunspots deflect cosmic rays. So when the Sun gets wild, trees record less carbon-14.

While trees don't typically live more than a few hundred years or perhaps a couple thousand, dead and buried trees, if preserved, carry a longer record, "as long as tree rings can be identified," said Manfred Schuessler, another Max Planck Institute researcher who worked on the study.

The study's finding: Sunspot activity has been more intense and lasted longer during the past 60 to 70 years than at anytime in more than eight millennia.

Sunspot activity is known to ebb and flow in two cycles lasting 11 and 88 years (activity is currently headed toward a short-term minimum). Astronomers think that longer cycles -- or at least long-term variations -- also occur. Scientists in other fields have shown that during the past 11,000 years, Earth's climate has had many dramatic shifts.

"Whether solar activity is a dominant influence in these [climate] changes is a subject of intense debate," says Paula Reimer, a researcher at Queen's University Belfast who wrote an analysis of the new study for Nature. Why? Because "the exact relationship of solar irradiance to sunspot number is still uncertain."

In general, studies indicate changes in solar output affect climate during periods lasting decades or centuries, "but this interpretation is controversial because it is not based on any understanding of the relevant physical processes," study member Schuessler told SPACE.com. Translation: Scientists have a lot to learn about the Sun-Earth connection.

Better understanding

The study's methods appear solid: "The models reproduce the observed record of sunspots extremely well, from almost no sunspots during the seventeenth century to the current high levels," Reimer said.

The research could eventually help scientists understand why the climate has changed in the past and allow for better predictions of future change.

"The reconstructed sunspot number will nonetheless provide a much-needed record of solar activity," Reimer said. "This can then be compared with palaeoclimate data sets to test theories of possible solar-climate connections, as well as enabling physicists to model long-term solar variability."

Whatever the result, change is likely to continue.

Solanki's team calculates that, based on history, the chances of sunspot activity remaining at the currently high levels for another 50 years is 8 percent. Odds are just 1 percent the solar exuberance will last through the end of this century.

Are Sunspots Disappearing?

September 3, 2009: The sun is in the pits of the deepest solar minimum in nearly a century. Weeks and sometimes whole months go by without even a single tiny sunspot. The quiet has dragged out for more than two years, prompting some observers to wonder, are sunspots disappearing?

"Personally, I'm betting that sunspots are coming back," says researcher Matt Penn of the National Solar Observatory (NSO) in Tucson, Arizona. But, he allows, "there is some evidence that they won't."

Penn's colleague Bill Livingston of the NSO has been measuring the magnetic fields of sunspots for the past 17 years, and he has found a remarkable trend. Sunspot magnetism is on the decline:

Above: Sunspot magnetic fields measured by Livingston and Penn
from 1992 - Feb. 2009 using an infrared Zeeman splitting technique. [more]

"Sunspot magnetic fields are dropping by about 50 gauss per year," says Penn. "If we extrapolate this trend into the future, sunspots could completely vanish around the year 2015."

This disappearing act is possible because sunspots are made of magnetism. The "firmament" of a sunspot is not matter but rather a strong magnetic field that appears dark because it blocks the upflow of heat from the sun's interior. If Earth lost its magnetic field, the solid planet would remain intact, but if a sunspot loses its magnetism, it ceases to exist.

"According to our measurements, sunspots seem to form only if the magnetic field is stronger than about 1500 gauss," says Livingston. "If the current trend continues, we'll hit that threshold in the near future, and solar magnetic fields would become too weak to form sunspots."

"This work has caused a sensation in the field of solar physics," comments NASA sunspot expert David Hathaway, who is not directly involved in the research. "It's controversial stuff."

The controversy is not about the data. "We know Livingston and Penn are excellent observers," says Hathaway. "The trend that they have discovered appears to be real." The part colleagues have trouble believing is the extrapolation. Hathaway notes that most of their data were taken after the maximum of Solar Cycle 23 (2000-2002) when sunspot activity naturally began to decline. "The drop in magnetic fields could be a normal aspect of the solar cycle and not a sign that sunspots are permanently vanishing."

Penn himself wonders about these points. "Our technique is relatively new and the data stretches back in time only 17 years. We could be observing a temporary downturn that will reverse itself."

The technique they're using was pioneered by Livingston at the McMath-Pierce solar telescope near Tucson. He looks at a spectral line emitted by iron atoms in the sun's atmosphere. Sunspot magnetic fields cause the line to split in two—an effect called "Zeeman splitting" after Dutch physicist Pieter Zeeman who discovered the phenomenon in the 19th century. The size of the split reveals the intensity of the magnetism.

Above: Zeeman splitting of spectral lines from a strongly-magnetized
sunspot. [more]

Astronomers have been measuring sunspot magnetic fields in this general way for nearly a century, but Livingston added a twist. While most researchers measure the splitting of spectral lines in the visible part of the sun's spectrum, Livingston decided to try an infra-red spectral line. Infrared lines are much more sensitive to the Zeeman effect and provide more accurate answers. Also, he dedicated himself to measuring a large number of sunspots—more than 900 between 1998 and 2005 alone. The combination of accuracy and numbers revealed the downturn.

If sunspots do go away, it wouldn't be the first time. In the 17th century, the sun plunged into a 70-year period of spotlessness known as the Maunder Minimum that still baffles scientists. The sunspot drought began in 1645 and lasted until 1715; during that time, some of the best astronomers in history (e.g., Cassini) monitored the sun and failed to count more than a few dozen sunspots per year, compared to the usual thousands.

"Whether [the current downturn] is an omen of long-term sunspot decline, analogous to the Maunder Minimum, remains to be seen," Livingston and Penn caution in a recent issue of EOS. "Other indications of solar activity suggest that sunspots must return in earnest within the next year."

Whatever happens, notes Hathaway, "the sun is behaving in an interesting way and I believe we're about to learn something new."

Author: Dr. Tony Phillips | Credit: Science@NASA