Phys.org July 20, 2021 Unlike coronal mass ejections which typically show up clearly on the Sun as dimming or brightening, the ‘stealth CMEs’ often originate at higher altitudes in the Sun’s corona, in regions with weaker magnetic fields and they are usually only visible on coronagraphs designed to reveal the corona. An international team of researchers (USA – UC Berkeley, industry, University of Maryland, NASA, Belgium, Romania, UK, India, Russia) has shown that many stealth CMEs can be detected in time if current analysis methods for remote sensing are adapted. They compared remote sensing images of the Sun with the […]