A solar flare is a sudden burst of light on the sun’s surface, usually accompanied by a giant release of radiation into space. At 7:49 p.m. EST on Feb. 24, 2014, what scientists call a significant solar flare peaked.
How significant is significant? The classification scale runs A, B, C, M and X, with X being the most intense. The scale is further divided into X1, X2, etc. The numbers give information about the strength of the flare: an X2 flare is twice as intense as an X1; an X3 is three times as intense. This flare is an X4.9-class flare.
Composite image of the solar flare showing the sun in ultraviolet light. Image: NASA/SDO
The radiation released by flare can’t pass through Earth’s atmosphere to reach the surface (and human life), but it can penetrate the atmosphere far enough to disturb GPS and communications signals.
Image: NASA/SDO
Here’s a coronagraph view of the coronal mass ejection that accompanied the flare:
Image: NASA&ESA/SOHO
NASA’s Solar Dynamics Observatory captured the event and produced the images seen here. Read more at: NASAs SDO Shows Images of Significant Solar Flare.
Ozone Hole Watch: Southern ozone map for 29 November 2014
NASA’s 2014 meteor shower schedule
NASA Portrait of Global Aerosols
Mapping the beautiful winds