During the Maunder Minimum, a period of diminished solar activity between
1645 and 1715, sunspots were rare on the face of the
sun, sometimes disappearing entirely for months to years. At the same time,
Earth experienced a bitter cold period known as the "
Little Ice Age."
Were the events connected?
Scientists cannot say for sure, but it's quite likely. Slowdowns in solar activity -- evidenced by reductions in sunspot numbers -- are known to coincide with decreases in the amount of energy discharged by the sun. During the
Little Ice Age, though, few would have thought to track
total solar irradiance (TSI), the amount of
solar energy striking Earth's upper
atmosphere. In fact, the scientific instrument needed to make such measurements -- a
spaceborne radiometer -- was still three centuries into the future.
Modern scientists have several tools for studying TSI. Since the 1970s,
scientists have relied upon a collection of radiometers on American and European
spacecraft to keep a close eye on solar fluctuations from above the atmosphere, which intercepts much of the sun's radiation. When
NASA launches the
Glory satellite this fall (no earlier than October 2009), researchers will have a more accurate instrument for measuring
TSI than they've ever had before.
The
Total Irradiance Monitor (TIM) on Glory is more sophisticated, but still related in concept to the very earliest ground-based solar radiometers, which were invented in 1838. Where those radiometers used sunlight to heat water and indicate the intensity of the sun's brightness at the
Earth's surface, Glory's TIM instrument will use a black-coated metallic detector to measure how much heat is produced by solar radiation as it reaches the top of the Earth's atmosphere.
Solar bolometers, as this subset of radiometers is called, have been flown on ten previous missions.
Nimbus-7, launched in 1978, included one of the first
spaceborne bolometers, and progressively more advanced instruments have followed on other
NASA, National Oceanic and Atmospheric Administration, and European
Space Agency missions.
In 2003, a first generation
TIM instrument went aloft with the
Solar Radiation and Climate Experiment (
SORCE)
satellite. Learning from that instrument, engineers have tweaked the optical and electrical sensors to make the Glory TIM even more capable of measuring the true solar brightness and its fluctuations.
"The
Glory TIM should be three times more accurate than
SORCE TIM, and about ten times more accurate than earlier instruments," said
Greg Kopp, a physicist at the University of Colorado, Boulder, and leader of the
TIM science team.
"There's no doubt that's an ambitious goal, but I wouldn't be surprised if they pull it off," said
Joseph Rice, a physicist at the National Institute of Standards and Technology in Gaithersburg, Md.
Beyond engineering improvements, the
Glory irradiance monitor has another advantage: access to the one-of-a-kind
TSI Radiometer Facility. Funded by
NASA and built by the Laboratory for Atmospheric and Space Physics in Boulder, Colo., the new facility has allowed
Kopp's team to calibrate the instrument in the same configuration and under the same conditions as it will endure in space. In January 2009, the
Glory TIM instrument underwent a rigorous battery of tests while being compared to a highly accurate ground-based radiometer.
"This was the first time a
TSI instrument has ever been validated end-to-end,"
Kopp said. "The improvements in accuracy will make it possible to detect long-term changes in the sun's output much more quickly." The data will help scientists say more definitively whether the sun’s output is gradually trending upward or downward, and whether the trend is influencing the pace of climate change.
Existing measurements offer a rough sketch, but they’re not quite accurate enough over decades to centuries to paint a clear picture of whether changes in
TSI reflect real changes on the sun or just artifacts of different instrument designs. That's because the radiometers that have measured
TSI so far have all reported values at slightly different levels and have all been calibrated differently, injecting a degree of uncertainty into the record.
The new TIM should be sufficiently accurate to quickly yield definitive data on whether
solar irradiance is trending up or down. Modelers estimate that
TSI increased roughly 0.08 percent as the
Sun exited the Maunder Minimum, which lasted for much of the 1700s. But even if
TSI radiometers had been available at the time, the increase in irradiance was so gradual that identifying the trend would have been difficult.
Detecting such subtle changes is where the
Glory TIM shines. Prior to
SORCE, most
TSI instruments had only 0.1 percent accuracy, and could not have reliably detected a 0.08 percent change over a century, Kopp explained. The improved accuracy of the
SORCE TIM (0.035 percent) would detect such a change in about 35 years. The
Glory TIM, meanwhile, should reduce the time needed to nearly ten years.
Getting TSI right has profound implications for understanding
Earth's climate. Thanks to previous orbiting radiometers, scientists know
TSI varies by roughly 0.1 percent through the sun’s 11-year magnetic cycle. Such a variation cannot explain the intensity and speed of the warming trends on
Earth during the last century, explained Judith Lean, a
solar physicist at the U.S. Naval Research Laboratory in Washington, D.C. But, that's not to say that the sun has no influence on climate change.
While total
solar irradiance changes by 0.1 percent, the change in the intensity of ultraviolet light varies by much larger amounts,
scientists have
discovered. Research shows such variations in the Sun's emissions can affect the ozone layer and the way energy moves both vertically and horizontally through the
atmosphere.
After examining the historical
TSI database, some scientists have suggested that solar irradiance could account for as much as a quarter of recent global warming. But without a continuous and reliable
TSI record, Kopp and Lean point out, there will always be room for skeptics to blame global warming entirely on the sun, even when most evidence suggests human activities are the key influence on modern climate changes.
Beyond that, there's a big "what if" percolating through the scientific community. The 0.1 percent variation in
solar irradiance is certainly too subtle to explain all of the recent warming. "But, what if -- as many assume -- much longer solar cycles are also at work?" said Lean. In that case, it's not impossible that long-term patterns -- proceeding over hundreds or thousands of years -- could cause more severe swings in TSI.
Could a modern day Maunder Minimum offset the warming influence of greenhouse gases or even throw us back into another little ice age? "It's extremely unlikely," said Lean, "but we won't know for sure unless we keep up and perfect our measurements."
Related Links: > Solar variability: Striking a balance with climate change > NASA study finds increasing solar trend that can change climate > Glory mission at Goddard Space Flight Center > Glory science at Goddard Institute for Space Studies > TIM instrument on SORCE observes Total Solar Irradiance (TSI) during Mercury transit > Solar Influences Group at the Laboratory for Atmospheric and Space Physics > SORCE Mission TIM overview 
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