Why was the Sun’s recent solar maximum twice as strong as predicted? In 2024-2025, the Sun entered a fiery active phase that completely defied expectations. But thanks to NASA's Parker Solar Probe, we now have observations taken from inside the Sun's atmosphere, which could help explain what’s powering the unusual eruptions. What’s really going on inside our star? And should we be worried here on Earth?
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0:00 What’s Happening to the Sun? 1:59 Solar Cycle 25 4:34 Where Is the Tachocline? 6:06 Parker Solar Probe 9:13 Solar Switchbacks 12:38 The Sun’s South Pole 16:51 May 2024 Geomagnetic Storm 20:48 Plasma Storms 22:37 Risk to Earth 25:33 Future Solar Missions
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References: “Predicting Solar Cycles”, via arxiv.org https://astrumspace.info/solarcycles “The Sun Reversed Its Decades-Long Weakening Trend”, via iop.org https://astrumspace.info/sunreversed “Calibrating HMI Magnetograms”, viaiop.org https://astrumspace.info/hmimag “The Solar Dynamo Begins Near the Surface”, via nature.com https://astrumspace.info/solardynamo “Parker Solar Probe’s Closest Pass to Sun”, via.nasa.gov https://astrumspace.info/parkerclosest “Eugene Parker and the Parker Solar Probe”, via quantamagazine.org https://astrumspace.info/parker “In-Situ Observations of Alfvén Waves Heating the Solar Wind”, via science.org https://astrumspace.info/solarwind “Solar Orbiter Gets First Views of the Sun’s Poles”, via esa.int https://astrumspace.info/solarpole “The May 2024 Geomagnetic Storm”, via royalsocietypublishing.org https://astrumspace.info/may24storm “Electron density during the May 2024 geomagnetic storm ”, via springer.com https://astrumspace.info/ionstorm
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Credits: Writer: Julia Masselos Video Editor: Alan Parry Audio Editor: James Horsley Researcher: Shourya Shrivastava Script Editor: Damaris McColgan Thumbnail Designers: Peter Sheppard, Juane Dames Publishing Lead: Georgina Brenner Production Coordinator: Rose Unwin Edit Producer: Poppy Pinnock Head of Astrum: Jess Jordan Creator of Astrum: Alex McColgan
With special thanks to: NASA/ESO/ESA
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