How does the Equinox affect the Auroras?
The earth’s magnetic field and charged particles from the sun interact to produce auroras. The auroras are brought on by charged particles from the sun that are caught in the Earth’s magnetic field and are most frequently observed in high-latitude areas close to the poles. When these particles hit with atoms in the Earth’s upper atmosphere as they travel towards the poles, light is produced as a result of the release of energy. The solar cycle and the solar wind are a couple of the factors that can have an impact on the auroras’ frequency and intensity throughout time. There are times of high and low solar activity throughout the solar cycle, which lasts around 11 years. The sun produces more charged particles when solar activity is high, which can result in more powerful and frequent auroras.
Although the autumn equinox doesn’t directly affect auroras, it does signal the change from summer to fall in the Northern Hemisphere. The longer evenings allow for more opportunities to watch the lights, which can make it easier to see the auroras at high latitudes.
Autumnal Equinox: Definition, Dates & Facts
Autumnal Equinox is often referred to as the September equinox or the fall equinox. The Autumnal Equinox is an astronomical event that takes place twice a year, on March 20 in the Southern Hemisphere and around September 22 in the Northern Hemisphere. Autumn equinox designates the time when the sun appears to move from north to south across the celestial equator, a fictitious line in the sky above the Earth’s equator.