The 11 year sunspot cycle has been something I've posted about many times here, and have done six month progress reports on the current cycle (25) regularly - the most recent was at the end of last December, the 28th. Let me start by refreshing the end of the year solar cycle plot:
My frequent comment is that cycle 25 is doing well, but is still weaker than cycle 23 (red). Yes, it's stronger than cycle 24 (pink) but that one was the weakest solar cycle in a hundred years. In this plot cycle 24 is the one on the bottom, and at least as of this plot in December, the grayish plot of cycle 25 hadn't shown itself to be stronger than 23 in even one month's smoothed sunspot number.
The (roughly) 11 year sunspot cycle, referred to as the Schwabe cycle, has been tracked longer than other measures because it's something that can be done by photographing the sun and applying the rules of counting the spots. When researchers looked for more subtle signs that required more instrumentation, they found another cycle superimposed on this one that lasted on the order of 100 years or 9 Schwabe cycles, and called the Gleissberg cycle. Plotted together, they look like this:
Looking at this plot, cycle 24 (last peak on the right) doesn't look particularly weak, especially compared to the cycle at the last null in about 1913, barely above the minima of the Gleissberg cycle.
Let me change pace for a little more background that I'm sure some readers will appreciate. This plot of the two types of cycles comes from a story that gets a bit more into it and leads much deeper. The article is at the top of Spaceweather.com today. That article is one paragraph which reads:
THE CENTENNIAL GLEISSBERG CYCLE: You've heard of the 11-year sunspot cycle. But what about the Centennial Gleissberg Cycle? The Gleissberg Cycle is a slow modulation of the solar cycle, which suppresses sunspot numbers every 80 to 100 years. It may have been responsible for the remarkable weakness of Solar Cycle 24 in 2012-2013. New research published in the journal Space Weather suggests that the minimum of the Gleissberg Cycle has just passed. If so, solar cycles for the next 50 years could become increasingly intense. Read the paper here.
It would be "bad form" for me to change the way that second to last sentence is displaying in the excerpted paragraph because it might not be clear that I'm the one who modified it. So I'll say read that second to last sentence again, and put it right here: If so, solar cycles for the next 50 years could become increasingly intense.
The first link in that paragraph is to climate.gov, where the graphic of the two cycles just above comes from. The last link is to a full copy of "Turnover in Gleissberg Cycle Dependence of Inner Zone Proton Flux" at a journal called Space Weather of the AGU, the American Geophysical Union. Much of the research is done with various satellites in and around the South Atlantic Anomaly, where Earth's magnetic field has several oddities.
I have a lot of questions about the Gleissberg cycle and both the apparent correlations and non-correlations. If you look at the right end of that combined Schwabe and Gleissberg cycles plot, you'll see one Schwabe cycle that is far higher than those near it and the highest peak in history (back to 1700). That's cycle 19 in the late 1950s - the one that older hams and radio hobbyists still talk about. Note that it's before the Gleissberg Cycle peak and the next sunspot cycle, 20, while apparently exactly at the CGC peak, is much smaller than 19. There are other places in that plot that also seem like the correlation isn't that good.