During the low point in the sun's 11-year cycle, the field lines up with the poles, resulting in sunspots. At the peak of the solar cycle, sunspots tend to form. During that phase of the solar cycle, intense bursts of radiation cause . This often occurs with coronal mass ejections, which are from the sun.
During the low point in the sun's 11-year cycle, the magnetic field lines up with the poles, resulting in the formation of sunspots. At the peak of the solar cycle, sunspots tend to form more frequently. During that phase of the solar cycle, intense bursts of radiation are emitted, causing solar flares. This often occurs with coronal mass ejections, which are large eruptions of plasma and magnetic field from the sun.
During the low point in the sun's 11-year cycle, the magnetic field lines of the sun tend to line up with the poles, resulting in the formation of sunspots. These sunspots are darker, cooler regions on the surface of the sun.
At the peak of the solar cycle, sunspots tend to form more frequently and in larger numbers. During this phase of the solar cycle, intense bursts of radiation and energy are often released from the sun. These bursts, known as solar flares, occur when the sun's magnetic field lines become twisted and release a huge amount of energy.
Solar flares can trigger coronal mass ejections (CMEs), which are massive eruptions of plasma and magnetic field lines from the sun's corona. These CMEs can release a large amount of particles and radiation into space.
Overall, during the peak of the solar cycle, sunspots form more frequently, leading to an increase in solar flares and CMEs, which can cause intense bursts of radiation and have various effects on space weather and communication systems on Earth.