Monday, March 31, 2014

By @nasa “The sun emitted a significant solar flare, peaking at 1:48 p.m. EDT March 29, 2014, and NASA’s Solar Dynamics Observatory captured images of the event. Solar flares are powerful bursts of radiation. Harmful radiation from 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. This flare is classified as an X.1-class flare. X-class denotes the most intense flares, while the number provides more information about its strength. An X2 is twice as intense as an X1, an X3 is three times as intense, etc. This image blends two wavelengths of light: 304 and 171 Angstroms, which help scientists observe the lower levels of the sun’s atmosphere. Image Credit: NASA/SDO #nasa #flare #solarflare #heliophysics #sun #solar #sdo #nasasdo” via @PhotoRepost_app



By @nasa “The sun emitted a significant solar flare, peaking at 1:48 p.m. EDT March 29, 2014, and NASA’s Solar Dynamics Observatory captured images of the event. Solar flares are powerful bursts of radiation. Harmful radiation from 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. This flare is classified as an X.1-class flare. X-class denotes the most intense flares, while the number provides more information about its strength. An X2 is twice as intense as an X1, an X3 is three times as intense, etc. This image blends two wavelengths of light: 304 and 171 Angstroms, which help scientists observe the lower levels of the sun’s atmosphere. Image Credit: NASA/SDO #nasa #flare #solarflare #heliophysics #sun #solar #sdo #nasasdo” via @PhotoRepost_app