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Next sunspot cycle stronger, may be more damaging to satellites and communication networks

Next sunspot cycle stronger, may be more damaging to satellites and communication networks

Next sunspot cycle stronger, may be more damaging to satellites and communication networks
National Science Foundation release
March 6, 2006

The next sunspot cycle will be 30 to 50 percent stronger than the last one, and begin as much as a year late, according to a breakthrough forecast using a computer model of solar dynamics developed by scientists at the National Center for Atmospheric Research (NCAR) in Boulder, Colo. The research results, funded by the National Science Foundation (NSF) and NASA, were published on-line on March 3 in the American Geophysical Union journal Geophysical Research Letters.

Scientists now predict that the next cycle, known as Cycle 24, will produce sunspots across an area slightly larger than 2.5 percent of the visible surface of the Sun. The cycle is projected to reach its peak about 2012, one year later than indicated by alternative forecasting methods that rely on statistics.

By analyzing recent solar cycles, the scientists also hope to forecast sunspot activity two solar cycles, or 22 years, into the future. The team is planning in the next year to issue a forecast of Cycle 25, which will peak in the early 2020s.

The researchers expect that predicting the Sun’s cycles years in advance will lead to more accurate plans for solar storms, which can slow satellite orbits, disrupt communications, and bring down power systems.

The team has verified the information by using the relatively new technique of helioseismology, based in part on observations from NASA instruments. This technique tracks sound waves reverberating inside the Sun to reveal details about the interior, much as a doctor might use ultrasound to see inside a patient.

“Forecasting the solar cycle will help society anticipate solar storms,” says Paul Bellaire, program director in NSF’s division of atmospheric sciences, which funded the research. “Important discoveries are being made using helioseismology. Through this technique, we can image even the far side of the Sun.”

NASA’s Transition Region and Coronal Explorer (TRACE) spacecraft caught these coils of hot, electrified gas, known as coronal loops, above active sunspots. The loops (some more than 300,000 miles high and capable of spanning 30 Earths) rise while flowing along the solar magnetic field, then cool and crash back to the surface at more than 60 miles per second (100 kilometers per second). Credit: NASA / Stanford Lockheed Institute for Space Research.

The scientists gained additional confidence in the forecast by showing that the newly developed model could simulate the strength of the past eight solar cycles with more than 98 percent accuracy.

“The model has demonstrated the necessary skill to be used as a forecasting tool,” says NCAR scientist Mausumi Dikpati, the leader of the forecast team at NCAR’s High Altitude Observatory. The team also includes NCAR scientists Peter Gilman and Guiliana de Toma.

“This is a significant breakthrough with important applications, especially for satellite-dependent societies,” says Gilman.

The Sun goes through approximately 11-year cycles, from peak storm activity to quiet, and back again. Solar scientists have tracked these cycles without being able to predict their relative intensity or timing, says Dikpati.

Solar storms are linked to twisted magnetic fields that suddenly snap and release tremendous amounts of energy. They tend to occur near dark regions of concentrated magnetic fields, known as sunspots.

The NCAR computer model, known as the Predictive Flux-transport Dynamo Model, draws on research indicating that the evolution of sunspots is caused by a current of plasma, or electrified gas, that circulates between the Sun’s equator and its poles over a period of 17 to 22 years.

The plasma acts as a conveyor belt, transporting the imprints of sunspots from the previous two solar cycles. As they return toward the equator, they become stretched and twisted by the internal rotation of the Sun, gradually becoming less stable than the surrounding plasma. This eventually causes coiled-up magnetic field lines to rise up, tear through the Sun’s surface, and create new sunspots, beginning the cycle again.

This is a news release from the National Science Foundation. The National Science Foundation (NSF) is an independent federal agency that supports fundamental research and education across all fields of science and engineering, with an annual budget of nearly $5.47 billion. NSF funds reach all 50 states through grants to nearly 2,000 universities and institutions. Each year, NSF receives about 40,000 competitive requests for funding, and makes about 11,000 new funding awards. The NSF also awards over $200 million in professional and service contracts yearly.

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