Illustration of the global coronal magnetic field as the Sun rotates. The background is the solar corona observed in extreme-ultraviolet waveband, with global coronal magnetic field maps measured ...
When these particles move about really quickly, they create magnetic fields which become entangled with one another and flow back into the Sun. However, coronal holes are areas in the huge star ...
Further storming may result from so-called "Coronal Hole High Speed Streams"—where the solar wind "blows" faster out ... clouds of plasma spat out from the sun—known as coronal mass ejections or ...
Further storming may result from so-called "Coronal Hole High Speed Streams"—where ... mass ejections or CMEs—hitting our planet's magnetic field and sparking a geomagnetic storm.
Oct. 3, 2024 — For the first time, scientists have taken near-daily measurements of the Sun's global coronal magnetic field, a region of the Sun that has only been observed irregularly in the past.
Two coronal mass ejections (CMEs) struck Earth’s magnetic field, causing geomagnetic storms that reached G3 levels on January 1. An X1.1-class solar flare on December 29, 2024, caused strong ...