Category The Sun

The Sun is far more than just a steady source of light. It is a dynamic, magnetically active star whose influence reaches far beyond the boundaries of our planetary system. In this section, we focus on the study and observation of our central star and the complex processes that drive space weather.

We provide in-depth insights into the various layers and activities of the Sun:

  • Sunspots & Photosphere: Analysis of active regions (AR), where intense magnetic fields disrupt convection and create darker, cooler zones.

  • Flares & Prominences: Reports on high-energy eruptions and massive streams of matter ejected from the solar atmosphere into space.

  • Solar Corona & Space Weather: Learn how solar winds and coronal mass ejections (CME) interact with Earth’s magnetic field and trigger auroras.

By combining real-time observational data – such as our white-light captures in the archive – with scientific facts, we offer a comprehensive resource for every solar observer.

Sunspots and the Solar Cycle

Sunspots are the most visible manifestation of the Sun’s magnetic activity as darker, cooler regions on the solar surface that play a critical role in our understanding of the Sun’s variability and its impact on Earth. These fascinating phenomena are…