sunspot

Welcome to Solar Maximum – The Zine

 I discovered this amazing  website recently where you can make a “Quick and Dirty” Photo Zine. If fact that is the name of the website. It makes a small, well formatted  letter sized zine to print on regular paper on regular printers. It also has a QR code if you  want to bring you readers to a webpage or Youtube video.

To visit the Zine “webpage” click here.

To make you own zine click here .

Enjoy! 

So what exactly is Solar Maximum?

Solar maximum is the peak of the Sun’s approximately 11-year activity cycle. At this point the Sun’s magnetic field is at its most tangled and intense, producing the highest number of sunspots, solar flares, and coronal mass ejections. After solar maximum the activity gradually winds down toward solar minimum before building up again.

 

Solar differential rotation and twisted magnetic field lines Two suns showing how differential rotation twists straight pole-to-pole magnetic field lines into tightly wound spirals, causing sunspot pairs to emerge. Differential rotation & magnetic field line twisting 1. Cycle begins — straight field lines faster ▶ equator slower ▶ poles N S years of rotation 2. Equator laps poles many times sunspot sunspot N S Kinked, compressed field lines burst through surface → sunspot pairs Original illustration — royalty free for blog use

We are currently (in  2026) in the declining phase of solar  cycle 25  and we are now past the “peak”  of solar maximum which occured in 2025.

While the sun is  certainly having more “quiet” time,  every once in a while things flare up like it did on this day. ( see video below)

 

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