As a pair of active regions began to rotate into view, their towering magnetic field lines above them bloomed into a dazzling display of twisting arches (Oct. 27-28, 2015) in this image from NASA's Solar Dynamics Observatory.

As a pair of active regions began to rotate into view, their towering magnetic field lines above them bloomed into a dazzling display of twisting arches (Oct. 27-28, 2015) in this image from NASA's Solar Dynamics Observatory.
SuperStock offers millions of photos, videos, and stock assets to creatives around the world. This image of As a pair of active regions began to rotate into view, their towering magnetic field lines above them bloomed into a dazzling display of twisting arches (Oct. 27-28, 2015) in this image from NASA's Solar Dynamics Observatory. by Piemags/PL Photography Limited is available for licensing today.

Visually Similar View more

RM
6145-45002500
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
RM
6145-45090299
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
RM
4389-1652
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.
RM
6145-45259691
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
RM
6145-44819426
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.
RM
6145-45257867
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=
RM
6145-45256905
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.
RM
6145-45111628
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.
RM
6145-45070365
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.
RM
6145-45004391
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.
RM
6145-45261725
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
RM
6145-44966117
Caption This image from June 20, 2013, at 11 15 p.m. EDT shows the bright light of a solar flare on the left side of the sun and an eruption of solar material shooting through the suns atmosphere, called a prominence eruption. Shortly thereafter, this same region of the sun sent a coronal mass ejection out into space. --- On June 20, 2013, at 11 24 p.m., the sun erupted with an Earth-directed coronal mass ejection or CME, a solar phenomenon that can send billions of tons of particles into space that can reach Earth one to three days later. These particles cannot travel through the atmosphere to harm humans on Earth, but they can affect electronic systems in satellites and on the ground. Experimental NASA research models, based on observations from NASAs Solar Terrestrial Relations Observatory and ESA/NASAs Solar and Heliospheric Observatory show that the CME left the sun at speeds of around 1350 miles per second, which is a fast speed for CMEs. Earth-directed CMEs can cause a space
RM
4389-1692
The Solar Terrestrial Relations Observatory (STEREO) spacecraft Ahead observed in the 304 Angstrom wavelength an eruptive solar prominence on the edge of the Sun using its Extreme Ultraviolet Imager (EUVI).
RM
6145-45256910
Extreme ultraviolet light streams out of an X-class solar flare as seen in this image captured on March 29, 2014, by NASA's Solar Dynamics Observatory. This image blends two wavelengths of light 304 and 171 Angstroms, which help scientists observe the lower levels of the sun's atmosphere. More info 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. To see how this event impacted 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 f
RM
6145-45256719
A giant arch of plasma rose up out of the Sun and then stretched itself until it had reached back to a point behind our view of the Sun (Sept, 17-18, 2014). Since it emerged from a magnetically intense active region, the arch is likely connecting to another active region over the Sun's horizon. We rarely see material extend this distance. The images were observed in the extreme ultraviolet wavelength of 171 Angstroms.
RM
6145-45232022
The Sun sported a very long filament that stretched out over 500,000 miles (800,000 km) and was visible for several days (June 3-4, 2014). It broke apart and dissipated soon after the end of the video clip. Filaments are tenuous strands of plasma held above the Sun's surface by magnetic forces. They appear darker because their temperature is somewhat cooler than that of the Sun's surface. The still image, shown in a combination of two wavelengths of extreme ultraviolet light, was taken at 11 33 UT on June 4.
RM
6145-45007457
Caption An X-class solar flare erupted on the left side of the sun on the evening of Feb. 24, 2014. This composite image, captured at 7 59 p.m. EST, shows the sun in X-ray light with wavelengths of both 131 and 171 angstroms.
RM
6145-45232162
NASA image captured December 6, 2010 To view a video of this event go here a href= http //www.flickr.com/photos/gsfc/5258354738 www.flickr.com/photos/gsfc/5258354738 /a A very long solar filament that had been snaking around the Sun erupted (Dec. 6, 2010) with a flourish. STEREO (Behind) caught the action in dramatic detail in extreme ultraviolet light of Helium. It had been almost a million km long (about half a solar radius) and a prominent feature on the Sun visible over two weeks earlier before it rotated out of view. Filaments, elongated clouds of cooler gases suspended above the Sun by magnetic forces, are rather unstable and often break away from the Sun.
RM
4239R-20480718
November 1-2, 2011 - One large and two good-sized, energetic active regions are rotating into view. The magnetic connection between the upper two areas clearly begin to reach over and interact with each other. Above them, the magnetic field lines, made visible in extreme ultraviolet light by particles spiraling along them, rise out and loop back to the Sun, constantly changing their structures. As these regions rotate towards the center of the Sun, any solar storms they generate could produce ef
RM
6145-45086494
An instrument on our Solar Dynamics Observatory (SDO) captured its 100 millionth image of the sun. The instrument is the Atmospheric Imaging Assembly, or AIA, which uses four telescopes working parallel to gather eight images of the sun - cycling through 10 different wavelengths -- every 12 seconds. This is a processed image of SDO multiwavelength blend from Jan. 19, 2015, the date of the spacecraft's 100th millionth image release.
RM
6177-V60455805
Image - Royalty Free Editorial
Royalty-Free Standard Editorial licenses are granted for worldwide, non-exclusive and perpetual NON-COMMERCIAL uses, unless specifically noted otherwise. All Royalty-Free transactions are final. The Royalty-Free Standard Editorial license has no limitations and covers up to 15 users.
  • $50.00 Low500 X 500
  • $150.00 Med750 X 750
  • $250.00 High2100 X 2100
  • $350.00 Super High7000 X 7000
Order a Framed Print
Looking for a license?
Click here, and we'll help you find it! Questions? Just ask!
DETAILS
Image Number: 6145-45099523Royalty FreeCredit Line:Piemags/PL Photography Limited/SuperStockCollection:PL Photography LimitedStory:Dynamic Solar PhenomenaContributor:PiemagsModel Release:NoProperty Release:NoResolution:720×720
Solar Dynamics Observatory (SDO)
sun|