The Sun recently decided to go naked for awhile, as is evident from this image acquired by NASA’s Solar Dynamics Observatory.
It lost its spots.
The image is from a video posted by NASA showing the Sun going naked from Jan. 26th to Jan. 30th, when a very small, lonely spot finally turns up. In fact, NASA says that with the exception of this one spot, the Sun was naked for almost two weeks.
Spotless periods like this are common as the Sun approaches the low point in its 11-year solar cycle. We’re headed for that minimum next year.
By contrast, during the peak of a solar cycle, the Sun is freckled with many spots. These crackle with intense magnetic activity producing flashes of x-rays and extreme ultraviolet radiation that can bathe the Earth.
Solar flares often are accompanied by explosions, called coronal mass ejections, that fling gargantuan quantities of energetic particles out into space. Earth can be bombarded by these CME particles, producing a storm in the magnetic bubble that surrounds the planet. This yields beautiful auroras but also potentially damaging effects on satellites, communication systems and power grids.
The Sun reached a peak in this activity in 2014, albeit a weak one. It was, in fact, the weakest maximum in solar activity since 1906.
We’ve been sliding toward solar minimum since then, with sunspots and activity subsiding. The low point in the cycle is expected occur in 2019 to 2020.
But just because the Sun is relatively calm, and often goes naked, doesn’t mean that it is in hibernation. The Sun is still active, just in a different way.
For example, during solar minimum the Sun often develops vast dark areas in its atmosphere, called coronal holes, where its magnetic field opens out into space. This allows particles to speed outward, forming an enhanced solar wind. When the wind hits the Earth’s geomagnetic field, the results can be similar to coronal mass ejections.