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Spots of bother? DURING the four centuries that it has been studied in detail, the sun has usually behaved in a regular manner. The number of spots on its surface has waxed and waned in cycles that last, on average, 11 years. Such cycles begin with spots appearing in mid-solar latitudes and end with them near the equator. And the more spots there are, the more solar storms there are around.
Sometimes, though, the sun sulks and this solar cycle stops. That has happened twice since records began: during the so-called Maunder minimum of 1645 to 1715 and the Dalton minimum of 1790 to 1830. These coincided with periods when global temperatures were lower than average, though why is a matter of debate.
An absence of sunspots also means an absence of solar flares and their more violent siblings, coronal mass ejections. Such outbursts disrupt radio and satellite communications, electricity grids and a variety of electronic equipment, so the pattern of solar activity is of more than academic interest. A new solar minimum, then, would test theories about how the climate works and also make communications more reliable. And many solar physicists think such a new minimum is on the cards. A group of them, who all work for America’s National Solar Observatory (NSO), have just had a meeting in New Mexico, under the aegis of the American Astronomical Society, to announce their latest results.
Intriguingly, however, Dr Hill’s studies indicate that the jet stream of a new cycle starts to form years before the sunspot pattern. This time, that has not happened. History suggests a new cycle should begin in 2019. If the sun were behaving itself, Dr Hill’s team would have seen signs of a new jet stream in 2008 or 2009. They did not. Nor are there indications of one even now. If a change in the jet stream really is a leading indicator of solar activity, then no new cycle is on the horizon.
The second study which suggests something odd is happening looked at the strengths of sunspots. Matthew Penn and William Livingston have analysed 13 years of data which indicate that, independently of the number of spots around, there has been a decrease in their strength.
Sunspots are caused by irruptions into its surface of the sun’s deeper magnetism. These create local drops in temperature, which make the surface gas darker. Over the period which Dr Penn and Dr Livingston analysed, the average magnetic strength of the irruptions has declined. Below a certain threshold, they will not be strong enough to overcome the convective mixing of the gas at the surface, and spots will disappear altogether. If the present trend continues, that will happen in 2021.
The third measure of the sun’s decline is in its outer atmosphere, the corona. At each solar maximum, the corona sloughs off the magnetic fingerprint of the previous cycle by pushing it to the poles. According to Richard Altrock, the leader of another NSO team at the meeting, that does not appear to be happening in the present cycle. It looks, then, as if a new, extended solar minimum is about to begin.
That is good news for operators of communications satellites. And it is interesting news for those who worry about global warming. If the Maunder and Dalton minima actually did affect the climate, then a new one might counteract the effects of the extra greenhouse gases people are now pumping into the atmosphere—at least, until the solar cycle returns. Whether the breathing space thus granted would be used wisely or squandered is another matter. Do not expect that debate to be as placid as the spotless sun.
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