The sunspot cycle is behaving a little like the stock market. Just when you think it has hit bottom, it goes even lower.
2008 was a bear. There were no sunspots observed on 266 of the year’s 366 days (73 per cent). To find a year with more blank Suns, you have to go all the way back to 1913, which had 311 spotless days. Prompted by these numbers, some observers suggested that the solar cycle had hit bottom in 2008.
Maybe not. Sunspot counts for 2009 have dropped even lower. As of 31 March, there were no sunspots on 78 of the year’s 90 days (87 per cent).
It adds up to one inescapable conclusion: “We’re experiencing a very deep solar minimum,” says solar physicist Dean Pesnell of Nasa’s Goddard Space Flight Centre in Greenbelt, Maryland.
“This is the quietest Sun we’ve seen in almost a century,” agrees forecaster David Hathaway of Nasa’s Marshall Space Flight Centre in Huntsville, Alabama.
Quiet Suns come along every 11 years or so. It’s a natural part of the sunspot cycle, discovered by German astronomer Heinrich Schwabe in the mid-1800s. Sunspots are planet-sized islands of magnetism on the surface of the Sun, and they are sources of solar flares, coronal mass ejections, and intense UV radiation. Plotting sunspot counts, Schwabe saw that peaks of solar activity were always followed by valleys of relative calm – a clockwork pattern that has held true for more than 200 years.
The current solar minimum is part of that pattern. In fact, it’s right on time. But is it supposed to be this quiet?
Measurements by the Ulysses spacecraft reveal a 20 per cent drop in solar wind pressure since the mid-1990s – the lowest point since such measurements began in the 1960s. The solar wind helps keep galactic cosmic rays out of the inner solar system. With the solar wind flagging, more cosmic rays penetrate the solar system, resulting in increased health hazards for astronauts. Weaker solar wind also means fewer geomagnetic storms and auroras on Earth.
Careful measurements by several Nasa spacecraft have also shown that the Sun’s brightness has dimmed by 0,02 per cent at visible wavelengths and a whopping 6 per cent at extreme UV wavelengths since the solar minimum of 1996. These changes are not enough to reverse global warming, but there are some other, noticeable side-effects.
Earth’s upper atmosphere is heated less by the Sun and it is therefore less “puffed up”. Satellites in Earth orbit experience less atmospheric drag, extending their operational lifetimes. That’s the good news. Unfortunately, space junk also remains in orbit longer, posing an increased threat to useful satellites.
Finally, radio telescopes are recording the dimmest “radio Sun” since 1955. After World War II, astronomers began keeping records of the Sun’s brightness at radio wavelengths, particularly 10,7 cm. Some researchers believe that the lessening of radio emissions during this solar minimum is an indication of weakness in the Sun’s global magnetic field. No one is certain, however, because the source of these long-monitored radio emissions is not fully understood.
All these lows have sparked a debate about whether the ongoing minimum is extreme or just an overdue market correction following a string of unusually intense solar maxima.
“Since the Space Age began in the 1950s, solar activity has been generally high,” notes Hathaway. “Five of the ten most intense solar cycles on record have occurred in the last 50 years. We’re just not used to this kind of deep calm.”
Deep calm was fairly common a hundred years ago. The solar minima of 1901 and 1913, for instance, were even longer than what we’re experiencing now. To match those minima in depth and longevity, the current minimum will have to last at least another year.
In a way, the calm is exciting, says Pesnell. “For the first time in history, we’re getting to observe a deep solar minimum.” A fleet of spacecraft – including the Solar and Heliospheric Observatory (SOHO), the twin probes of the Solar Terrestrial Relations Observatory (STEREO), and several other satellites – are all studying the Sun and its effects on Earth. Using technology that didn’t exist 100 years ago, scientists are measuring solar winds, cosmic rays, irradiance and magnetic fields and finding that solar minimum is much more interesting than anyone expected.
Modern technology cannot, however, predict what comes next. Competing models by dozens of solar physicists disagree, sometimes sharply, on when this solar minimum will end and how big the next solar maximum will be. The great uncertainty stems from one simple fact: no one fully understands the underlying physics of the sunspot cycle.
Pesnell believes sunspot counts should pick up again soon, “possibly by the end of the year”, to be followed by a solar maximum of below-average intensity in 2012 or 2013.
But like other forecasters, he knows he could be wrong. Bull or bear? Stay tuned for updates.