 160-minute solar cycle

The term "160-minute solar cycle" refers to a specific periodic phenomenon observed in the Sun's atmosphere, particularly in the context of solar magnetic activity and oscillations. One key aspect of this cycle is its association with the solar atmosphere's behavior, including coronal loops and solar flares. The cycle typically lasts approximately 160 minutes, and it is often observed in the context of solar oscillations and the magnetic field dynamics within the solar corona.