aurimisjahutustsüklid
Aurimisjahutustsüklid, also known as auroral cooling cycles, refers to a phenomenon observed in some astrophysical contexts, particularly in the atmospheres of cool stars and brown dwarfs. These cycles are characterized by periodic fluctuations in the intensity of auroral emissions, which are a form of radiation produced when charged particles from a stellar wind interact with the planet's magnetic field.
The mechanism is thought to involve a feedback loop. Initially, a stellar flare or coronal mass ejection
The study of aurimisjahutustsüklid is important for understanding the complex interactions between stars and their circumplanetary