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NASA scientists have spotted a massive coronal hole on the Sun, which is 20 times larger than Earth, unleashing solar winds towards Earth.
Solar winds impact Earth’s magnetic field, satellites and technology.
Solar winds also lead to generation of aurora at higher latitudes on Earth.
Coronal Holes
Coronal holes are areas which appear dark in solar corona in extreme ultraviolet and soft x-ray solar images.
These are regions on the sun’s surface from where fast solar wind gushes out into space.
In these regions, the magnetic field is open to interplanetary space, sending solar material out in a high-speed stream of solar wind i.e. geomagnetic storm.
They have lower temperatures and appear much darker than their surroundings as they contain little solar material.
Coronal holes can last between a few weeks to months.
The holes are not a unique phenomenon, appearing throughout the sun’s approximately 11-year solar cycle. They can last much longer during solar minimum, a period of time when activity on the Sun is substantially diminished.