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Dec. 21, 2006: Evidence is mounting: the next
solar cycle is going to be a big one.
Solar
cycle 24, due to peak in 2010 or 2011 "looks like its
going to be one of the most intense cycles since
record-keeping began almost 400 years ago," says solar
physicist David Hathaway of the Marshall Space Flight
Center. He and colleague Robert Wilson presented this
conclusion last week at the American Geophysical Union
meeting in San Francisco.
Right: An erupting solar prominence
photographed by the Solar and Heliospheric Observatory (SOHO).
[More]
Their forecast is based on historical records of
geomagnetic storms.
Hathaway explains: "When a gust of solar wind hits
Earth's magnetic field, the impact causes the magnetic
field to shake. If it shakes hard enough, we call it a
geomagnetic storm." In the extreme, these storms cause
power outages and make compass needles swing in the
wrong direction. Auroras are a beautiful side-effect.
Hathaway and Wilson looked at records of geomagnetic
activity stretching back almost 150 years and noticed
something useful:. "The amount of geomagnetic activity
now tells us what the solar cycle is going to be like 6
to 8 years in the future," says Hathaway. A picture is
worth a thousand words:

Above: Peaks in geomagnetic activity
(red) foretell solar maxima (black) more than six years
in advance. [More]
In the plot, above, black curves are solar cycles; the
amplitude is the sunspot number. Red curves are
geomagnetic indices, specifically the Inter-hour
Variability Index or IHV. "These indices are derived
from magnetometer data recorded at two points on
opposite sides of Earth: one in England and another in
Australia. IHV data have been taken every day since
1868," says Hathaway.
Cross correlating sunspot number vs. IHV, they found
that the IHV predicts the amplitude of the solar cycle
6-plus years in advance with a 94% correlation
coefficient.
"We don't know why this works," says Hathaway. The
underlying physics is a mystery. "But it does work."
According
to their analysis, the next Solar Maximum should peak
around 2010 with a sunspot number of 160 plus or minus
25. This would make it one of the strongest solar cycles
of the past fifty years—which is to say, one of the
strongest in recorded history.
Left: Hathaway and Wilson's prediction
for the amplitude of Solar Cycle 24. [More]
Astronomers have been counting sunspots since the days
of Galileo, watching solar activity rise and fall every
11 years. Curiously, four of the five biggest cycles on
record have come in the past 50 years. "Cycle 24 should
fit right into that pattern," says Hathaway.
These results are just the latest signs pointing to a
big Cycle 24. Most compelling of all, believes Hathaway,
is the work of Mausumi Dikpati and colleagues at the
National Center for Atmospheric Research (NCAR) in
Boulder, Colorado. "They have combined observations of
the sun’s 'Great Conveyor Belt' with a sophisticated
computer model of the sun’s inner dynamo to produce a
physics-based prediction of the next solar cycle." In
short, it's going to be intense. Details may be found in
the Science@NASA story
Solar Storm Warning.
"It all hangs together," says Hathaway. Stay tuned for
solar activity.
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Author:
Dr. Tony
Phillips | Production Editor:
Dr. Tony Phillips | Credit:
Science@NASA
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More to the story....
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Hathaway points out that there are actually two
types of geomagnetic activity:
(1) storms caused by the gentle buffeting of
solar wind streams and
(2) storms caused by the more forceful
impact of flares and coronal mass ejections
(CMEs).
"Only the first type has predictive value," says
Hathaway. "Storms caused by solar wind streams
come and go in a regular pattern that foretells
the solar cycle. Storms caused by flares and
CMEs don't have this property." To improve their
results, Hathaway and Wilson used a technique
developed by Joan Feynman to remove storms
caused by flares and CMEs from their data.
Reference: Hathaway, D. H. and
Wilson, R. M. 2006, "Geomagnetic
activity indicates large amplitude for sunspot
cycle 24", Geophys. Res. Lett. in press.
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