A Prominence Bubble • This high resolution movie of a solar prominence highlights a phenomena called prominence bubbles. In regions where the Sun's magnetic field reverses sign, puffs of chromospheric material can be suspended above the Sun's surface. Sometimes, strong magnetic fields containing hot gas can occur under these puffs, forming what looks like a dome-shaped void. This void, called a magnetic bubble, can push up into the prominence material forming a bright ridge as seen in this movie

• A Prominence Eruption with a M-class Solar Flare • We can see prominence erupting to interplanetary space. A flare occurs simultaneously at the bottom region of the eruption. (Observed by Solar Optical Telescope (SOT), wavelength: calcium H line [396 nm]) [Instrument: Hinode/ Solar Optical Telescope (SOT), Wavelength: 394 nm Calcium H line)] Occurred on 16 April 2012. • Credit: “NAOJ, JAXA, NASA/MSFC” | Astronomy Nation

🔴 Incredible Solar Flare, Prominence Eruption and CME Event (304 angstroms) 15.7.2019 • On June 7, 2011, an M-2 flare occurred on the Sun which released a very large coronal mass ejection (CME). Much of the ejected material is much cooler (less than about 80,000K) and therefore appears dark against the brighter solar disk. Material which does not reach solar escape velocity can be seen falling back and striking the solar surface, sometimes triggering smaller events. This image sequence is captu