What are coronal holes?
Captured by the NASA Solar Dynamics Observatory, recently shared an image of the sun seemingly ‘smiling’ has dark patches on the sun’s surface resembling eyes and a smile.
NASA explained that the patches are called coronal holes, which can be seen in ultraviolet light but are typically invisible to our eyes.
What are coronal holes?
- These are regions on the sun’s surface from where fast solar wind gushes out into space. Because they contain little solar material, they have lower temperatures and thus appear much darker than their surroundings.
- Here, the magnetic field is open to interplanetary space, sending solar material out in a high-speed stream of solar wind.
- 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, according to NASA.
What do they tell us?
- These ‘coronal holes’ are important to understanding the space environment around the earth through which our technology and astronauts travel.
- NASA had said in 2016 when coronal holes covering “six-eight per cent of the total solar surface.
- While it is unclear what causes coronal holes, they correlate to areas on the sun where magnetic fields soar up and away, without looping back down to the surface as they do elsewhere.
- Scientists study these fast solar wind streams because they sometimes interact with earth’s magnetic field, creating what’s called a geomagnetic storm, which can expose satellites to radiation and interfere with communications signals.
What happens during a geomagnetic storm?
- According to the US government agency National Oceanic and Atmospheric Administration, geomagnetic storms relate to earth’s magnetosphere – the space around a planet that is influenced by its magnetic field.
- When a high-speed solar stream arrives at the earth, in certain circumstances it can allow energetic solar wind particles to hit the atmosphere over the poles.
- Such geomagnetic storms cause a major disturbance of the magnetosphere as there is a very efficient exchange of energy from the solar wind into the space environment surrounding earth.
- In cases of a strong solar wind reaching the earth, the resulting geomagnetic storm can cause changes in the ionosphere, part of the earth’s upper atmosphere.
- Radio and GPS signals travel through this layer of the atmosphere, and so communications can get disrupted.
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