A huge coronal hole of more than 800,000 kilometers is detected on the surface of the sun, which releases high -speed solar wind towards the Earth. The incident is expected to accelerate ororel activity on 31 January and 1 February. Solar air is traveling at a speed of more than 500 kilometers per second, which can lead to a minor geomagonic storm. These disturbances can result in high latitudes, vibrant northern and southern lights, which increases visibility for Arora enthusiasts.
High speed solar wind leads to Earth
As Informed By space.com, according to spaceweather.com, coronal holes are areas where the sun’s magnetic field opens, which survives the solar air. These areas appear deep in extreme ultraviolet images due to the absence of limited hot gases. The current coronal hole, which is estimated to exceed 62 times the diameter of the Earth, is issuing a powerful stream of particles charged in the space, some of which expect to reach the Earth’s magnetosphere.
The National Oceanic and Atmospheric Administration (NOAA) has released the G1 Geomagnetic Storm Watch for this period. From G-Scal, G1 (Minor) to G5 (peak), these disturbances classify them based on their intensity. While the G1 storms usually cause minor ups and downs in power grids and satellite operations, they can largely increase and increase the display.
Effect on the forecast of the weather and space season
As the solar air collides with the magnetic field of the Earth, it activates oxygen and nitrogen atoms in the upper atmosphere, resulting in the dazzling and dazzle and dazzle and dazzling and dazzling near the poles. Experts suggest that although G1 storms are not rare, their effects on Auroral activity may be different. The space weather is difficult to estimate, which means that the intensity of upcoming performances is uncertain.
