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Images of 'Sdo' found, 27

 
Transit of Venus in front of the Sun. 05/06/2012 - Venus Transit. 05/06/2012 - Beginning of the transit of Venus in front of the Sun seen by the SDO satellite, June 5, 2012. Beginning of Venus transit on 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

PIX4588485

Transit of Venus in front of the Sun. 05/06/2012 - Venus Transit. 05/06/2012 - Beginning of the transit of Venus in front of the Sun seen by the SDO satellite, June 5, 2012. Beginning of Venus transit on 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

PIX4588485

 
La comete ISON pres du Soleil - 11/2013 - Comet ISON with Sun - 11/2013 - Comet ISON seen before and after its passage near the Sun. Composite of 60 images obtained by the Soho space telescope on 28 and 29 November 2013. This view captures the transformation of Comet ISON as it rounded the sun. It combines 60 SOHO C2 frames in which ISON appears (Nov. 28, 1248 UT, to Nov. 29, 0316 UT) with stars, noise and particle tracks removed, plus an SDO AIA 171 image of the sun taken just before the spacecraft attempted to image the comet near perihelion

PIX4571403

La comete ISON pres du Soleil - 11/2013 - Comet ISON with Sun - 11/2013 - Comet ISON seen before and after its passage near the Sun. Composite of 60 images obtained by the Soho space telescope on 28 and 29 November 2013. This view captures the transformation of Comet ISON as it rounded the sun. It combines 60 SOHO C2 frames in which ISON appears (Nov. 28, 1248 UT, to Nov. 29, 0316 UT) with stars, noise and particle tracks removed, plus an SDO AIA 171 image of the sun taken just before the spacecraft attempted to image the comet near perihelion

PIX4571403

 
The first lunar transit observed by NASA's Solar Dynamics Observatory

UIG2912231

The first lunar transit observed by NASA's Solar Dynamics Observatory

UIG2912231

 
Transit of Venus in front of the Sun. 05/06/2012 - Venus Transit. 05/06/2012 - Beginning of the transit of Venus in front of the Sun seen by the SDO satellite, June 5, 2012. Beginning of Venus transit on 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

PIX4588443

Transit of Venus in front of the Sun. 05/06/2012 - Venus Transit. 05/06/2012 - Beginning of the transit of Venus in front of the Sun seen by the SDO satellite, June 5, 2012. Beginning of Venus transit on 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

PIX4588443

 
Transit of Venus in front of the Sun. 05/06/2012 - Venus Transit. 05/06/2012 - Beginning of the transit of Venus in front of the Sun seen by the SDO satellite, June 5, 2012. Beginning of Venus transit on 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

PIX4588448

Transit of Venus in front of the Sun. 05/06/2012 - Venus Transit. 05/06/2012 - Beginning of the transit of Venus in front of the Sun seen by the SDO satellite, June 5, 2012. Beginning of Venus transit on 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

PIX4588448

 
Le Soleil vu by SDO on March 30, 2010 - The Sun seen by SDO. March 30, 2010 - The Sun seen in ultraviolet by SDO (Solar Dynamics Observatory) on March 30, 2010. In red, the coldest regions, in blue and green, the warmer regions. SDO (Solar Dynamics Observatory) First Light Image. A full - disk multiwavelength extreme ultraviolet image of the sun taken by SDO on March 30, 2010. False colors trace different gas temperatures. Reds are relatively cool (about 60,000 Kelvin, or 107,540 F); blues and greens are hotter (greater than 1 million Kelvin, or 1,799,540 F)

PIX4627139

Le Soleil vu by SDO on March 30, 2010 - The Sun seen by SDO. March 30, 2010 - The Sun seen in ultraviolet by SDO (Solar Dynamics Observatory) on March 30, 2010. In red, the coldest regions, in blue and green, the warmer regions. SDO (Solar Dynamics Observatory) First Light Image. A full - disk multiwavelength extreme ultraviolet image of the sun taken by SDO on March 30, 2010. False colors trace different gas temperatures. Reds are relatively cool (about 60,000 Kelvin, or 107,540 F); blues and greens are hotter (greater than 1 million Kelvin, or 1,799,540 F)

PIX4627139

 
The Sun seen by SDO on October 26, 2014 - The Sun seen by SDO - October 26, 2014 - Solar eruption (bright spot below right) seen by SDO (Solar Dynamics Observatory) on October 26, 2014. The bright light in the lower right of the sun shows an X-class solar flare on Oct. 26, 2014, as captured by NASA's SDO. This was the third X-class flare in 48 hours, which erupted from the largest active region seen on the sun in 24 years. This flare was classified as an X2.0-class flare and it peaked at 6:56 a.m. EDT.

PIX4627305

The Sun seen by SDO on October 26, 2014 - The Sun seen by SDO - October 26, 2014 - Solar eruption (bright spot below right) seen by SDO (Solar Dynamics Observatory) on October 26, 2014. The bright light in the lower right of the sun shows an X-class solar flare on Oct. 26, 2014, as captured by NASA's SDO. This was the third X-class flare in 48 hours, which erupted from the largest active region seen on the sun in 24 years. This flare was classified as an X2.0-class flare and it peaked at 6:56 a.m. EDT.

PIX4627305

 
Solar eruption - The Sun seen by SDO: Coronal rain (right) during an eruption on the surface of the Sun, ultraviolet view by SDO (Solar Dynamics Observatory) on July 19, 2012. On July 19, 2012, an eruption occurred on the sun that produced a moderately powerful solar flare and a dazzling magnetic display known as coronal rain. Hot plasma in the corona cooled and condensed along strong magnetic fields in the region. Magnetic fields, are invisible, but the charged plasma is forced to move along the lines, showing up brightly in the extreme ultraviolet wavelength of 304 angstroms, and outlining the fields as it slowly falls back to the solar surface

PIX4583365

Solar eruption - The Sun seen by SDO: Coronal rain (right) during an eruption on the surface of the Sun, ultraviolet view by SDO (Solar Dynamics Observatory) on July 19, 2012. On July 19, 2012, an eruption occurred on the sun that produced a moderately powerful solar flare and a dazzling magnetic display known as coronal rain. Hot plasma in the corona cooled and condensed along strong magnetic fields in the region. Magnetic fields, are invisible, but the charged plasma is forced to move along the lines, showing up brightly in the extreme ultraviolet wavelength of 304 angstroms, and outlining the fields as it slowly falls back to the solar surface

PIX4583365

 
Le Soleil vu par SDO on 12 January 2015 - The Sun seen by SDO - January 12 2015 - Solar eruption (bright spot on the right) seen by SDO (Solar Dynamics Observatory) on 12 January 2015. The sun emitted a mid-level solar flare, peaking at 11:24 p.m. EST on Jan. 12, 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 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

PIX4627273

Le Soleil vu par SDO on 12 January 2015 - The Sun seen by SDO - January 12 2015 - Solar eruption (bright spot on the right) seen by SDO (Solar Dynamics Observatory) on 12 January 2015. The sun emitted a mid-level solar flare, peaking at 11:24 p.m. EST on Jan. 12, 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 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

PIX4627273

 
Le Soleil vu by SDO on December 6, 2010 - The Sun seen by SDO. December 6, 2010 - Le Soleil vu en ultraviolet by SDO (Solar Dynamics Observatory) on December 6, 2010. It shows a gas filament of nearly a million miles breaking. A very long solar filament that had been snaking around the Sun erupted on December 6, 2010 with a flourish. Nasa's Solar Dynamics Observatory (SDO) 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 ago before it rotated out of view. Filaments are elongated clouds of cooler gases suspended above the Sun by magnetic forces. They are rather unstable and often break away from the Sun

PIX4627176

Le Soleil vu by SDO on December 6, 2010 - The Sun seen by SDO. December 6, 2010 - Le Soleil vu en ultraviolet by SDO (Solar Dynamics Observatory) on December 6, 2010. It shows a gas filament of nearly a million miles breaking. A very long solar filament that had been snaking around the Sun erupted on December 6, 2010 with a flourish. Nasa's Solar Dynamics Observatory (SDO) 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 ago before it rotated out of view. Filaments are elongated clouds of cooler gases suspended above the Sun by magnetic forces. They are rather unstable and often break away from the Sun

PIX4627176

 
Le Soleil vu by SDO on December 6, 2010 - The Sun seen by SDO. December 6, 2010 - Le Soleil vu en ultraviolet by SDO (Solar Dynamics Observatory) on December 6, 2010. It shows a gas filament of nearly a million miles breaking. A very long solar filament that had been snaking around the Sun erupted on December 6, 2010 with a flourish. Nasa's Solar Dynamics Observatory (SDO) 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 ago before it rotated out of view. Filaments are elongated clouds of cooler gases suspended above the Sun by magnetic forces. They are rather unstable and often break away from the Sun

PIX4627223

Le Soleil vu by SDO on December 6, 2010 - The Sun seen by SDO. December 6, 2010 - Le Soleil vu en ultraviolet by SDO (Solar Dynamics Observatory) on December 6, 2010. It shows a gas filament of nearly a million miles breaking. A very long solar filament that had been snaking around the Sun erupted on December 6, 2010 with a flourish. Nasa's Solar Dynamics Observatory (SDO) 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 ago before it rotated out of view. Filaments are elongated clouds of cooler gases suspended above the Sun by magnetic forces. They are rather unstable and often break away from the Sun

PIX4627223

 
Le Soleil en maximum solaire - The Sun seen by SDO - Composite - Le Soleil vu en ultraviolet by SDO (Solar Dynamics Observatory) from February 11, 2013 to February 11, 2014. Image composed of 25 different images, illustrating the sun in high activity. This image is a composite of 25 separate images spanning the period of February 11, 2013 to February 11, 2014. It uses the SDO AIA wavelength of 304 Angstroms and reveals the zones on the sun where active regions and associated eruptions most commonly occur during Solar Maximum

PIX4627235

Le Soleil en maximum solaire - The Sun seen by SDO - Composite - Le Soleil vu en ultraviolet by SDO (Solar Dynamics Observatory) from February 11, 2013 to February 11, 2014. Image composed of 25 different images, illustrating the sun in high activity. This image is a composite of 25 separate images spanning the period of February 11, 2013 to February 11, 2014. It uses the SDO AIA wavelength of 304 Angstroms and reveals the zones on the sun where active regions and associated eruptions most commonly occur during Solar Maximum

PIX4627235

 
Le Soleil eclipse partially par la Terre - The Sun cut by the Earth seen by SDO - Le Soleil vu en ultraviolet by SDO (Solar Dynamics Observatory) on March 29, 2011 (07:14:57 UT). In this image the Sun is cut by the Earth because at the time of shooting, the SDO satellite was passing behind the Earth. Differences in the density of the Earth's atmosphere block light inevenly, which explains why the Sun does not appear to cut evenly. Nasa's Solar Dynamics Observatory (SDO) observes a partial solar eclipse. Twice a year, the SDO enters an eclipse season where the spacecraft slips behind Earth for up to 72 minutes a day. Image taken on March 29 2011 (07:14:57 UT)

PIX4627193

Le Soleil eclipse partially par la Terre - The Sun cut by the Earth seen by SDO - Le Soleil vu en ultraviolet by SDO (Solar Dynamics Observatory) on March 29, 2011 (07:14:57 UT). In this image the Sun is cut by the Earth because at the time of shooting, the SDO satellite was passing behind the Earth. Differences in the density of the Earth's atmosphere block light inevenly, which explains why the Sun does not appear to cut evenly. Nasa's Solar Dynamics Observatory (SDO) observes a partial solar eclipse. Twice a year, the SDO enters an eclipse season where the spacecraft slips behind Earth for up to 72 minutes a day. Image taken on March 29 2011 (07:14:57 UT)

PIX4627193

 
The Sun as seen by SDO on October 2, 2014

PIX7223384

The Sun as seen by SDO on October 2, 2014

PIX7223384

 
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Male figures, fragment of amphora from mound tomb in Tumulo II of Sodo, Cortona, Tuscany, Italy, Etruscan civilization, 6th century BC

Sandro Vannini

DGA923463

Male figures, fragment of amphora from mound tomb in Tumulo II of Sodo, Cortona, Tuscany, Italy, Etruscan civilization, 6th century BC

Sandro Vannini

DGA923463

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