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Images of 'Solar Rash' found, 22

 
Solar eruption seen by SOHO 02/04/2001 - Large solar flare seen by SOHO on april 2 2001 - Solar eruption seen by SOHO satellite; the Sun is masked by a coronographer. An image of the Sun taken at the same time by another satellite instrument was superimposed. A large solar flare occurred at 4:51 p.m. EDT, on Monday, April 2, 2001. as Observed by the Solar and Heliospheric Observatory (SOHO) satellite. Solar flares, among the solar systems mightiest eruptions, are tremendous explosions in the atmosphere of the Sun capable of releasing as much energy as a billion megatons of TNT. Caused by the sudden release of magnetic energy, in just a few seconds, solar flares can accelerate solar particles to very high velocities, almost to the speed of light, and heat solar material to tens of millions of degrees. The recent explosion from the active region near the sun's northwest limb hurled a coronal mass ejection into space at a whopping speed of roughly 7.2 million kilometers per hour. Luckily,

PIX4627092

Solar eruption seen by SOHO 02/04/2001 - Large solar flare seen by SOHO on april 2 2001 - Solar eruption seen by SOHO satellite; the Sun is masked by a coronographer. An image of the Sun taken at the same time by another satellite instrument was superimposed. A large solar flare occurred at 4:51 p.m. EDT, on Monday, April 2, 2001. as Observed by the Solar and Heliospheric Observatory (SOHO) satellite. Solar flares, among the solar systems mightiest eruptions, are tremendous explosions in the atmosphere of the Sun capable of releasing as much energy as a billion megatons of TNT. Caused by the sudden release of magnetic energy, in just a few seconds, solar flares can accelerate solar particles to very high velocities, almost to the speed of light, and heat solar material to tens of millions of degrees. The recent explosion from the active region near the sun's northwest limb hurled a coronal mass ejection into space at a whopping speed of roughly 7.2 million kilometers per hour. Luckily,

PIX4627092

 
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 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 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

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