Not that you'd know it with the weather we've been having, but the current solar cycle appears to be ramping up in terms of activity, with more sunspots and bigger prominences than in previous years. At the minimum around 2019, three quarters of days showed no sunpots. So far this year, not long admittedly, there has been at least one every day.
The experts point out that the previous 11 year solar cycle started in the same way as the current one, but overall it did not build to a maximum that could be called spectacular.
I took a shot of current sunspots in a clear spell on the morning of 5 February 2022 at 10:27:08 (Lunt 60 f8.3/500mm and zwo asi 120 colour, stacked best 25% of 500 rather shaky video frames).
I've made a collage of this image with the sunspot number references taken from the NASA solar dynamics observatory, as well as an SDO diagram of the magnetic field lines from the sunspots in the image, 2939 and 2940, and others . My photo isn't quite at the proper sun rotational angle but the sunspot numbers provide the reference points (the published diagram is not updated daily, and relates to a later day with yet more sunspots).
The interesting feature to my mind is the way the magnetic field lines join all sunspots together as a sun wide phenomenon, over massive distances, not just locally. Sunspots often appear in pairs suggesting a bar magnet arrangement, as vaguely with 2939 and definitely with SP 2940 with one pair and a triple, but things turn out to be far more complex.
The SDO was launched in 2010 into a synchronous earth orbit. It can observe the sun more or less continuously. Info here
This includes the explanation of how the field lines are measured, "using the Zeeman effect to work out the polarisation of the same field line and give the magnetic field over the sun surface". I am none the wiser but mightily impressed it can be done.
James