NASA’s Solar Dynamics Observatory captured this image of a mid-level solar flare on the Sun — as seen in the bright spot in the lower centre of the solar disc on 24 August 2015. The image shows a subset of extreme ultraviolet light that highlights the extremely hot solar material, which is typically colourised in red. Image credits: NASA/SDO.The Sun emitted a mid-level solar flare, peaking at 8:33am BST on 24 August 2015. NASA’s Solar Dynamics Observatory, which watches the Sun constantly, captured an image of the event. Solar flares are powerful bursts of radiation. Harmful radiation from such a flare cannot pass through Earth’s atmosphere to physically affect humans on the ground, however — when intense enough — they can disturb the atmosphere in the layer where GPS and communications signals travel.
To see how this event may affect Earth, please visit NOAA’s Space Weather Prediction Center, the U.S. government’s official source for space weather forecasts, alerts, watches and warnings.
This flare is classified as an M 5.6 class flare. M-class flares are a tenth the size of the most intense flares, the X-class flares. The number provides more information about its strength. An M2 is twice as intense as an M1, an M3 is three times as intense, etc.
The Sun’s magnetic field is responsible for everything from the solar explosions that cause space weather on Earth — such as aurorae — to the interplanetary magnetic field and radiation through which our spacecraft journeying around the solar system must travel. But even now, scientists are not sure exactly where in the Sun the magnetic field is created.
In his third report from the Royal Astronomical Society’s NAM2015, Kulvinder Singh Chadha examines the Sun in X-ray and ultraviolet wavelengths from three different spacecraft, dons a virtual reality planetarium headset, and investigates if the proposed James Webb Space Telescope (JWST) could discern Earth-sized worlds that are habitable.
NASA’s Interface Region Imaging Spectrograph satellite, or IRIS, and the Japan Aerospace Exploration Agency’s (JAXA)/NASA’s Hinode solar observatory, have just made a significant step towards understanding why the corona — the outermost, wispy layer of the Sun’s atmosphere — is hundreds of times hotter than the lower photosphere, which is the Sun’s visible surface.