The Sun Is About to Enter a Period of Peak Activity :
Scientists say the Sun is about to enter a peak activity period called a "solar maximum." This point in the solar cycle typically brings abundant sunspots and flares as the Sun's magnetic poles flip. But what does that mean for us here on Earth?
First, it's essential to understand what's happening on the Sun during a solar maximum. The Sun constantly undergoes a type of motion called convection, in which its plasma boils toward the surface, then sinks back toward the star's 27 million-degree core as it cools. This process is what builds strong magnetic fields at the Sun's poles. Every decade or so, however, this convection becomes unstable, causing the Sun's north and south poles to flip. This point in the solar cycle triggers a period of intense activity on the Sun's surface, resulting in what we call a solar maximum.
Solar maximum gives astronomers beautiful images of sunspots and bright solar flares. Astronomers also spend this period looking for coronal mass ejections, or CMEs, in which the Sun spits out massive balls of plasma at hundreds to thousands of kilometers per second. But because the Sun is so close to Earth, these phenomena have real-life implications for us humans and our electricity-dependent infrastructure.
(Score: 0) by Anonymous Coward on Friday March 03, @01:22PM
It depends upon where you are talking about bit flips. It looks like the Wiki article is talking about on the ground, but satellites take a beating during these solar maximum times and you get a lot of problems with them. The Wiki article is talking about how it is harder for galactic cosmic ray particles to make it to Earth and strike the atmosphere because, essentially, they have to fight their way inwards in the solar system against the more active magnetic fields coming out of the Sun. If you want to see a nice example of that, look up a time-series plot from a neutron detector station and you'll see how as the Sun is more active, you get less neutrons on the ground (which are the result of atmospheric showers caused by high energy cosmic rays striking the top of the atmosphere). For instance, Figure 11 here [jhuapl.edu] (which can easily fool you to think the opposite because you have to pay attention to the fact that they plotted the sunspot number on a decreasing scale!).