Fast solar winds emerge from regions typically found at the sun's north and south poles, called coronal holes. This wind can reach speeds of around 750 kilometers per second. To pinpoint precisely where fast solar winds are coming from, colleagues needed to get as up close and personal to the sun as possible. NASA's Parker Solar Probe was launched in 2018, and it's been getting steadily closer to the sun. In 2021, the probe was able to observe the sun from about 9 million kilometers away - very close in astronomical terms. From there, it could take a range of measurements from ion spectra to plasma density and magnetic field strength.

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