02.8.2021

Tree Rings Help Reconstruct a Millennium of the Sun's Activity

By Jan Hattenbach

Astronomers are using tree rings as a historical record of solar activity — and they’ve found that the Sun was much more active in the past.

Our Sun is not the faithfully constant light source it appears to be. Solar activity varies in a fairly regular cycle of 11 years, most notably in the periodic rise and fall in the number of sunspots. Though German astronomer Samuel Heinrich Schwabe discovered the cycle in the 19th century, sunspot observations commenced about 400 years ago with Galileo Galilei, and the solar cycle has been traced back to these early observations.

Now, a team of scientists based in Switzerland has successfully reconstructed the 11-year Schwabe cycle all the way back to the year AD 969, using the Sun’s imprint on ancient trees on Earth. Their report appears in Nature Geoscience.

Sunspots at solar minimum vs. maximum
Visible-light images from NASA’s Solar Dynamics Observatory highlight the difference in sunspots at minimum (left) and maximum (right).
NASA

Tree Rings and Solar Activity

Tree rings provide a record of Earth’s environmental past. Trees grow new rings every year, their thickness depending on the abundance of water and general climatic conditions. By carefully assigning rings to specific years, scientists can study how Earth’s climate evolved over time.

Nicolas Brehm (ETH Zürich, Switzerland) and colleagues used samples of cut-down trees, some found as construction material in historic buildings in England and Switzerland, to reconstruct the Sun’s varying impact on our planet by measuring their content of radioactive carbon-14.

Carbon-14, or radiocarbon, has 14 neutrons and is a rare variant of the more typical carbon atom that has 12 neutrons. Due to the extra neutrons, the rarer nucleus decays into nitrogen with a half-life of 5,730 years.

Radiocarbon is present on Earth because energetic particles from the Sun are constantly hitting nitrogen atoms in the upper atmosphere, converting them into radiocarbon. The freshly produced carbon-14 atoms are incorporated into carbon dioxide molecules and ultimately absorbed by living plants or animals. As long a creature is alive, its ratio of radio to regular carbon remains constant, at about one part per billion. After death, the radiocarbon begins to decay, so scientists can measure its abundance to date historic organic material.       

Solar eruption
Generally, the Sun’s magnetic field and particle wind help protect Earth from more energetic charged particles coming from outside the solar system. As a result, the production of carbon-14 in the atmosphere drops during periods of high solar activity.
SDO / NASA

Brehm and colleagues turned this method on its head: First, they dated each sample, ring by ring, using available historic tree-ring records. Then, knowing  the exact age of each tree ring in their samples, they tried to figure out how much carbon-14 there was in the atmosphere as each tree ring grew, and how this abundance changed from one year to the next.

The tree rings should contain different amounts of carbon-14, depending on the Sun’s activity: In times of high activity, the solar magnetic field and the solar wind are stronger, effectively shielding Earth from radiocarbon-forming galactic cosmic rays. When solar activity is low, so is its protective shield, and more cosmic particles can reach Earth. Higher solar activity (as measured by sunspots) should thus generally yield lower C-14 abundances, and vice versa.

However, the Sun’s impact on carbon-14 production is very small, and weather-induced noise is of the same order of magnitude as the expected signal. Earlier attempts by other groups therefore yielded inconclusive results. Moreover, the very low concentration of carbon-14 requires large samples of tree cores, and its abundance takes a long time to measure. To cover a millennium-long timespan (from AD 969 to 1933) would be too time-consuming if done in the traditional way.

So the team took a novel approach: Instead of measuring radioactivity emitted by the decaying carbon-14, they counted the atoms directly with an accelerator mass-spectrometer. That is, they vaporize the samples to ionize their atoms, then use a magnetic field to accelerate them and separate them by mass. The scientists could thus use much smaller samples (from millimeter-thick drill holes), speed up the measurement process, and reach the precision required. 

The result, published in Nature Geoscience, more than doubles the previous annually resolved carbon-14 record. By successfully matching the carbon-14 production rates with solar activity over the past 400 years, the scientists could extend solar activity records into times well before the invention of the telescope.

Tree-ring record of solar activity
The first row of this plot shows the annual carbon-14 data, with red arrows marking possible events that would have caused carbon-14 production to surge. In the second row, this data is normalized. The third row shows solar activity, with the black line marking recorded sunspot numbers. The last row shows filtered data, with some associated events denoted with arrows. (The Little Ice Age is a period of cool weather in parts of the world, but its connection to solar activity is still debated.)
Brehm et al. / Nature Geoscience 2021

A Millennium of Solar Activity

During times of prolonged decreases in solar activity, carbon-14 production rates went up as expected: The periods when sunspots were scarce, especially during the Spörer, Maunder, and Dalton minima, are clearly visible in the tree-ring record.

The scientists also identified three sharp peaks of increased radiocarbon production, which they associate with exceptional solar eruption events in the years 993, 1052, and 1279. The first was originally discovered and published in 2013, from an independent tree-ring analysis. Now, with the four events detected in this study, it seems statistically improbable that anything other than the Sun could have caused them.

However, all three events seem to have originated from solar eruptions much more intense, or at least different from major solar eruptions observed in modern times — including the infamous Carrington event in 1859. In fact, the 1859 eruption left no trace in the carbon-14 records.

Coronal mass ejection
A solar eruption spews energetic charged particles from the Sun. If the eruption is strong enough and directed toward Earth, those particles can cause a surge of carbon-14 production.
SOHO ESA & NASA

It’s almost as if our Sun has a double personality: Most of the time it’s a kind of protective “older brother” that shields us from energetic particles zooming around the galaxy, but sometimes it turns into a violent bully, hitting us with its own punch of particles when we least expect it.

This work helps expand our star’s activity record over much longer timespans than were previously accessible. It also yields a better assessment about the probability of potentially dangerous solar eruptions, the authors write. Team member Lukas Wacker (ETH Zürich, Switzerland) says the team is already working on extending their analysis. Precisely dated tree-ring data are available for the last 12,000 years, and according to Wacker, there might already be evidence supporting other historic solar eruptions.        


Reference:

Brehm, N., Bayliss, A., Christl, M. et al. Eleven-year solar cycles over the last millennium revealed by radiocarbon in tree rings. Nat. Geosci. 14, 10–15 (2021). https://doi.org/10.1038/s41561-020-00674-0

This article appeared on the Sky & Telescope website at https://skyandtelescope.org/astronomy-news/tree-rings-reconstruct-millennium-solar-activity/

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