NASA image release Sept 9, 2010 Just as sunspot 1105 was turning away from Earth on Sept. 8, the active region erupted, producing a solar flare and a fantastic prominence. The eruption also hurled a bright coronal mass ejection into space. The eruption was not directed toward any planets. View the video here a href= http //www.flickr.com/photos/gsfc/4974878090 www.flickr.com/photos/gsfc/4974878090 /a To see a full disk view go here a href= http //www.flickr.com/photos/gsfc/4975115754/ www.flickr.com/photos/gsfc/4975115754/ /a This is a snapshot of the prominence.

NASA image release Sept 9, 2010 Just as sunspot 1105 was turning away from Earth on Sept. 8, the active region erupted, producing a solar flare and a fantastic prominence. The eruption also hurled a bright coronal mass ejection into space. The eruption was not directed toward any planets. View the video here a href= http //www.flickr.com/photos/gsfc/4974878090 www.flickr.com/photos/gsfc/4974878090 /a To see a full disk view go here a href= http //www.flickr.com/photos/gsfc/4975115754/ www.flickr.com/photos/gsfc/4975115754/ /a This is a snapshot of the prominence.
SuperStock offers millions of photos, videos, and stock assets to creatives around the world. This image of NASA image release Sept 9, 2010 Just as sunspot 1105 was turning away from Earth on Sept. 8, the active region erupted, producing a solar flare and a fantastic prominence. The eruption also hurled a bright coronal mass ejection into space. The eruption was not directed toward any planets. View the video here a href= http //www.flickr.com/photos/gsfc/4974878090 www.flickr.com/photos/gsfc/4974878090 /a To see a full disk view go here a href= http //www.flickr.com/photos/gsfc/4975115754/ www.flickr.com/photos/gsfc/4975115754/ /a This is a snapshot of the prominence. by Piemags/PL Photography Limited is available for licensing today.

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A solar flare erupts on Jan. 30, 2014, as seen by the bright flash on the left side of the sun, captured here by NASA's Solar Dynamics Observatory. In the lower right corner the moon can be seen, having just passed between the observatory and the sun. --- The sun emitted a mid-level solar flare, peaking at 11 11 a.m. EST on Jan. 30, 2014. Images of the flare were captured by NASA's Solar Dynamics Observatory, or SDO, shortly after the observatory witnessed a lunar transit. The black disk of the moon can be seen in the lower right of the images. 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. To see how this event may impact Earth, please visit NOAA's Space Weather Prediction Center at a href= http //spaceweather.gov rel= nofollow spaceweather.gov /a , th
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NASAs Solar Dynamics Observatory, or SDO, captured this solar image on March 16, 2015, which clearly shows two dark patches, known as coronal holes. The larger coronal hole of the two, near the southern pole, covers an estimated 6- to 8-percent of the total solar surface. While that may not sound significant, it is one of the largest polar holes scientists have observed in decades. The smaller coronal hole, towards the opposite pole, is long and narrow. It covers about 3.8 billion square miles on the sun - only about 0.16-percent of the solar surface. Coronal holes are lower density and temperature regions of the suns outer atmosphere, known as the corona. Coronal holes can be a source of fast solar wind of solar particles that envelop the Earth. The magnetic field in these regions extends far out into space rather than quickly looping back into the suns surface. Magnetic fields that loop up and back down to the surface can be seen as arcs in non-coronal hole regions of the image, i
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A large coronal hole appears dark (such as this area in the top part of the Sun) when viewed in extreme ultraviolet light at 284 angstroms, such as this image taken by the Solar and Heliospheric Observatory (SOHO)'s EIT (Extreme ultraviolet Imaging Telescope). Coronal holes are sources of solar wind.
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NASA image captured June 5, 2012. On June 5-6 2012, SDO is collecting images of one of the rarest predictable solar events the transit of Venus across the face of the sun. This event happens in pairs eight years apart that are separated from each other by 105 or 121 years. The last transit was in 2004 and the next will not happen until 2117. i
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NASA image acquired May 1, 2010.As an active region rotated into view, it blew out three relatively small eruptions over about two days (Apr. 30 - May 2) as STEREO (Ahead) observed in extreme UV light. The first one was the largest and exhibited a pronounced twisting motion (shown in the still from May 1, 2010). The plasma, not far above the Sun's surface in these images, is ionized Helium heated to about 60,000 degrees. Note, too, the movement of plasma flowing along magnetic field lines that extend out beyond and loop back into the Sun's surface. Such activity occurs every day and is part of the dynamism of the changing Sun.
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This image, is a composite of 23 separate images spanning the period of January 11, 2015 to January 21, 2016. It uses the SDO AIA wavelength of 171 angstroms and reveals the zones on the sun where active regions are most common during this part of the solar cycle. There are wallpapers sized for some phones and tablets available to download here a href=
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A solar flare bursts off the left limb of the sun in this image captured by NASA's Solar Dynamics Observatory on June 10, 2014, at 7 41 a.m. EDT. This is classified as an X2.2 flare, shown in a blend of two wavelengths of light 171 and 131 angstroms, colorized in gold and red, respectively.
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Several arcing loops rotated into view and swirled above an active region, which gave us a nice profile view of the action from NASA's Solar Dynamics Observatory on June 26-27, 2016.
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On Aug. 24, 2014, the sun emitted a mid-level solar flare, peaking at 8 16 a.m. EDT. NASA's Solar Dynamics Observatory captured images of the flare, which erupted on the left side of the sun. 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. To see how this event may affect Earth, please visit NOAA's Space Weather Prediction Center at a href= http //spaceweather.gov rel= nofollow spaceweather.gov /a , the U.S. government's official source for space weather forecasts, alerts, watches and warnings. This flare is classified as an M5 flare. M-class flares are ten times less powerful than the most intense flares, called X-class flares.
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The dark region seen on the face of the sun at the end of March 2013 is a coronal hole (just above and to the right of the middle of the picture), which is a source of fast solar wind leaving the sun in this image from NASA's Solar Dynamic Observatory.
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NASA's Solar Dynamics Observatory captured this image of a mid-level solar flare - as seen in the bright flash in the middle -on Dec. 16, 2014 shortly before midnight EST. Read more a href= http //1.usa.gov/1BYLxsE rel= nofollow 1.usa.gov/1BYLxsE /a
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