Text Size

The sun's pockmarked surface is always shifting. Sunspots and solar flares rise and fall every 11 years, a cycle associated with regular reversal of the star's magnetic field. Huge quantities of plasma—known as coronal mass ejections—fly into space, which can disrupt satellites and other electronic signals if they reach Earth. More solar activity during the cycle also amplifies auroras and warms Earth's temperatures slightly. Yet careful study has shown that longer periodicities exist, too. The Gleissberg cycle, first identified in 1862, strengthens and weakens the 11-year cycle over the course of a century (shown in yellow). One paper posits that the Gleissberg pattern is caused by a slow swaying of the sun's magnetic pole. The Suess-DeVries cycle (green) lasts about 200 years, whereas the Hallstatt cycle (blue) runs on the order of 2,400 years. Still, the sun can also be erratic, making it tricky for physicists to predict future sunspots, says Alexei Pevtsov, an astronomer at the National Solar Observatory in Boulder, Colo.: “There's an element of randomness.”

Read full article Scientific American article at:

https://www.scientificamerican.com/article/the-sunspot-cycle-is-more-intricate-than-previously-thought/

 

Sunday Night Net:
Time: 7 pm  Local.
Repeater : W9MID
146.835 w/151.4 PL
(Backup Repeater
443.525 w/151.4 PL)
  

Member Login

Paid Members can request a username and password or changes to their login information by sending their request to: webmaster@midstatehams.org

arrlAFC

 

 

 

 

 

 

Traffic Info

3.png3.png8.png8.png7.png3.png7.png
30 November 2021