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Images of 'Protuberance' found, 62

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Le Soleil vu by STEREO 29/09/2008 - Solar activity seen by STEREO spacecraft on september 29 2008 - Protuberances observed by one of the STEREO satellites on September 29, 2008. The STEREO spacecraft observed this visually stunning prominence eruption on Sept. 29, 2008, in the 304 angstrom wavelength of extreme UV light. Prominences are relatively cool clouds of gas suspended above the sun and controlled by magnetic forces. The prominence rose and cascaded to the right over several hours, appearing something like a flag unfurling, as it broke apart and headed into space. The prominence is composed of ionized Helium that is about 60,000 degrees Kelvin

Le Soleil vu by STEREO 29/09/2008 - Solar activity seen by STEREO spacecraft on september 29 2008 - Protuberances observed by one of the STEREO satellites on September 29, 2008. The STEREO spacecraft observed this visually stunning prominence eruption on Sept. 29, 2008, in the 304 angstrom wavelength of extreme UV light. Prominences are relatively cool clouds of gas suspended above the sun and controlled by magnetic forces. The prominence rose and cascaded to the right over several hours, appearing something like a flag unfurling, as it broke apart and headed into space. The prominence is composed of ionized Helium that is about 60,000 degrees Kelvin

PIX4627123

Le Soleil vu en cut- Illustration - Cutaway of the Sun

Le Soleil vu en cut- Illustration - Cutaway of the Sun

Miller, Ron (b.1947)

PIX4583452

Le Soleil vu by STEREO on 16/08/2008 - Solar activity seen by STEREO spacecraft on august 16 2008 - Protuberances observed by one of the STEREO satellites on 16 August 2008. A STEREO spacecraft observed several solar prominences rise and gyrate above the Sun over a two - day period (Aug. 15 - 16, 2008), with the largest one arcing a distance at least equal to 30 Earth diameters. They are spread out with one in each quadrant. Magnetic forces control solar prominences that rise above the Sun's surface. The prominences were seen in the 304 Angstroms wavelength of ultraviolet light. The material observed is actually ionized Helium at about 60,000 degrees. Prominences are relatively cool clouds of gas suspended above the Sun and controlled by magnetic forces. They can last from hours to months, but most usually remain for just a few days

Le Soleil vu by STEREO on 16/08/2008 - Solar activity seen by STEREO spacecraft on august 16 2008 - Protuberances observed by one of the STEREO satellites on 16 August 2008. A STEREO spacecraft observed several solar prominences rise and gyrate above the Sun over a two - day period (Aug. 15 - 16, 2008), with the largest one arcing a distance at least equal to 30 Earth diameters. They are spread out with one in each quadrant. Magnetic forces control solar prominences that rise above the Sun's surface. The prominences were seen in the 304 Angstroms wavelength of ultraviolet light. The material observed is actually ionized Helium at about 60,000 degrees. Prominences are relatively cool clouds of gas suspended above the Sun and controlled by magnetic forces. They can last from hours to months, but most usually remain for just a few days

PIX4627116

Solar eruption seen by Skylab - Solar prominence seen by Skylab - Ultraviolet view of the Sun obtained from Skylab Station in December 1973. Ultraviolet image of a giant loop prominence on the Sun, recorded by the Skylab space station on December 19, 197

Solar eruption seen by Skylab - Solar prominence seen by Skylab - Ultraviolet view of the Sun obtained from Skylab Station in December 1973. Ultraviolet image of a giant loop prominence on the Sun, recorded by the Skylab space station on December 19, 197

PIX4626817

Le Soleil vu par SDO - The Sun seen by SDO - Le Soleil vu en ultraviolet by SDO (Solar Dynamics Observatory) on March 29, 2011 (20:44:57 UT). Image taken on March 29, 2011 (20:44:57 UT) by Solar Dynamics Observatory (SDO)

Le Soleil vu par SDO - The Sun seen by SDO - Le Soleil vu en ultraviolet by SDO (Solar Dynamics Observatory) on March 29, 2011 (20:44:57 UT). Image taken on March 29, 2011 (20:44:57 UT) by Solar Dynamics Observatory (SDO)

PIX4627243

Sunspots and solar flare - Sunspots and solar flare - Surface eruption and sunspots seen on 28 July 2004 with an H - Alpha filter. Solar flare and sunspots seen on july 28 2004 with an hydrogen alpha filter

Sunspots and solar flare - Sunspots and solar flare - Surface eruption and sunspots seen on 28 July 2004 with an H - Alpha filter. Solar flare and sunspots seen on july 28 2004 with an hydrogen alpha filter

Sebastian Voltmer

PIX4626565

Occipital bone, outer surface (engraving)

Occipital bone, outer surface (engraving)

English School, (19th century)

LLM3634213

Le Soleil August 15, 2016 - The Sun on Aug 15, 2016: Surface du Soleil et eruption solaire seen on August 15, 2016 with a H-Alpha filter. - Solar flare seen on august 15 2016 with an hydrogen alpha filter

Le Soleil August 15, 2016 - The Sun on Aug 15, 2016: Surface du Soleil et eruption solaire seen on August 15, 2016 with a H-Alpha filter. - Solar flare seen on august 15 2016 with an hydrogen alpha filter

Sebastian Voltmer

PIX4626624

Occipital bone, inner surface (engraving)

Occipital bone, inner surface (engraving)

English School, (19th century)

LLM3634210

Surface of the Sun - Illustration

Surface of the Sun - Illustration

Miller, Ron (b.1947)

PIX4583453

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.

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

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)

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 September 19, 2010 - The Sun seen by SDO. September 19, 2010 - The Sun seen in ultraviolet by SDO (Solar Dynamics Observatory) on September 19, 2010. A full - disk extreme ultraviolet image of the sun taken by SDO (Solar Dynamics Observatory) on September 19, 2010

Le Soleil vu by SDO on September 19, 2010 - The Sun seen by SDO. September 19, 2010 - The Sun seen in ultraviolet by SDO (Solar Dynamics Observatory) on September 19, 2010. A full - disk extreme ultraviolet image of the sun taken by SDO (Solar Dynamics Observatory) on September 19, 2010

PIX4627212

Le Soleil vu by SDO on 27 October 2014 - The Sun seen by SDO - October 27 2014 - Solar eruption (shining spot below right) seen by SDO (Solar Dynamics Observatory) on 27 October 2014. Nasa's Solar Dynamics Observatory captured this image of an X2.0-class solar flare bursting off the lower right side of the sun on Oct. 27, 2014. The image shows a blend of extreme ultraviolet light with wavelengths of 131 and 171 Angstroms.

Le Soleil vu by SDO on 27 October 2014 - The Sun seen by SDO - October 27 2014 - Solar eruption (shining spot below right) seen by SDO (Solar Dynamics Observatory) on 27 October 2014. Nasa's Solar Dynamics Observatory captured this image of an X2.0-class solar flare bursting off the lower right side of the sun on Oct. 27, 2014. The image shows a blend of extreme ultraviolet light with wavelengths of 131 and 171 Angstroms.

PIX4627266

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

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. A full - disk extreme ultraviolet image of the sun taken by SDO (Solar Dynamics Observatory) on March 30, 2010

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. A full - disk extreme ultraviolet image of the sun taken by SDO (Solar Dynamics Observatory) on March 30, 2010

PIX4627163

Le Soleil vu par SDO on 16 April 2012 - The Sun seen by SDO - April 2012 - Le Soleil vu en ultraviolet by SDO (Solar Dynamics Observatory) on 16 April 2012 (17:44:21 UT). Image taken on April 16, 2012 (17:44:21 UT) by Solar Dynamics Observatory (SDO)

Le Soleil vu par SDO on 16 April 2012 - The Sun seen by SDO - April 2012 - Le Soleil vu en ultraviolet by SDO (Solar Dynamics Observatory) on 16 April 2012 (17:44:21 UT). Image taken on April 16, 2012 (17:44:21 UT) by Solar Dynamics Observatory (SDO)

PIX4627209

Le Soleil en H - Alpha - 21/06/2004 - The Sun - June 21, 2004 - Le Soleil vu le 21 juin 2004. The image shows sunspots, protuberances and a very active region near the center of the image (AR 10652). The Sun on June 21, 2004. The image shows sunspots, filaments, prominences and a very active region (AR 10652) near the center of the sun

Le Soleil en H - Alpha - 21/06/2004 - The Sun - June 21, 2004 - Le Soleil vu le 21 juin 2004. The image shows sunspots, protuberances and a very active region near the center of the image (AR 10652). The Sun on June 21, 2004. The image shows sunspots, filaments, prominences and a very active region (AR 10652) near the center of the sun

Stefan Seip

PIX4626697

Le Soleil vu par SDO le 2 mars 2012 - The Sun seen by SDO - March 2012 - Solar eruption seen in ultraviolet by SDO (Solar Dynamics Observatory) on 2 mars 2012. On March 2, 2012, a giant eruption of solar material exploded up off the surface of the right side of the sun, as captured in this image from Nasa's Solar Dynamics Observatory. Known as a prominence eruption, most of the material usually falls right back down on to the sun

Le Soleil vu par SDO le 2 mars 2012 - The Sun seen by SDO - March 2012 - Solar eruption seen in ultraviolet by SDO (Solar Dynamics Observatory) on 2 mars 2012. On March 2, 2012, a giant eruption of solar material exploded up off the surface of the right side of the sun, as captured in this image from Nasa's Solar Dynamics Observatory. Known as a prominence eruption, most of the material usually falls right back down on to the sun

PIX4627202

Le Soleil vu by SDO on May 23, 2010 - The Sun seen by SDO. May 23, 2010 - Le Soleil vu en ultraviolet by SDO (Solar Dynamics Observatory) on May 23, 2010. This image taken by SDO (Solar Dynamics Observatory) is a composite of three extreme ultraviolet wavelengths: 211 A (false - color yellow) 193 A (green) and 171 A (blue), each tracing a different gas temperature ranging from 1 to 2 million degrees K

Le Soleil vu by SDO on May 23, 2010 - The Sun seen by SDO. May 23, 2010 - Le Soleil vu en ultraviolet by SDO (Solar Dynamics Observatory) on May 23, 2010. This image taken by SDO (Solar Dynamics Observatory) is a composite of three extreme ultraviolet wavelengths: 211 A (false - color yellow) 193 A (green) and 171 A (blue), each tracing a different gas temperature ranging from 1 to 2 million degrees K

PIX4627172

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)

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 vu en ultraviolet by SOHO on 18/11/2009 - The Sun seen in ultraviolet by Soho. November 18, 2009 - A protuberance, a plasma cloud, escapes from the Sun. White areas are the hottest and most active areas. Prominences are cooler clouds of gases suspended above the Sun by magnetic forces

Le Soleil vu en ultraviolet by SOHO on 18/11/2009 - The Sun seen in ultraviolet by Soho. November 18, 2009 - A protuberance, a plasma cloud, escapes from the Sun. White areas are the hottest and most active areas. Prominences are cooler clouds of gases suspended above the Sun by magnetic forces

PIX4627010

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

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

Total Eclipse of Sun in Zambia. 21/06/2001 - Total Solar Eclipse of 2001 june 21 - Solar protuberances observed during the total eclipse of Sun of 21 June 2001. Solar prominences seen during the totality

Total Eclipse of Sun in Zambia. 21/06/2001 - Total Solar Eclipse of 2001 june 21 - Solar protuberances observed during the total eclipse of Sun of 21 June 2001. Solar prominences seen during the totality

Sebastian Voltmer

PIX4627740

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

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

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

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

Total solar eclipse in Libya 03/2006 - Total solar eclipse in Libya - Total solar eclipse seen on 29/03/2006 in Libya. Composite of 60 images. Very high resolution image of the solar crown. Total solar eclipse observed in Libya on March 29, 2006. Processing Composition of 60 images

Total solar eclipse in Libya 03/2006 - Total solar eclipse in Libya - Total solar eclipse seen on 29/03/2006 in Libya. Composite of 60 images. Very high resolution image of the solar crown. Total solar eclipse observed in Libya on March 29, 2006. Processing Composition of 60 images

PIX4627876

Total Eclipse of Sun - 13/11/2012 - Total Solar Eclipse - November 13 2012 - Total Eclipse of Sun of 13 November 2012 seen in Australia. The total solar eclipse of November 13 2012 seen in Australia

Total Eclipse of Sun - 13/11/2012 - Total Solar Eclipse - November 13 2012 - Total Eclipse of Sun of 13 November 2012 seen in Australia. The total solar eclipse of November 13 2012 seen in Australia

Sebastian Voltmer

PIX4628330

Sun cutaway - Sun cutaway - At the bottom left, the Earth is represented. Bottom left is the Earth

Sun cutaway - Sun cutaway - At the bottom left, the Earth is represented. Bottom left is the Earth

PIX4629407

Total Eclipse of Sun in Zambia. 21/06/2001 - Total Solar Eclipse of 2001 june 21 - Composite of several images showing details in the crown. Different images combined to create an image which captures the visual appearance of the corona

Total Eclipse of Sun in Zambia. 21/06/2001 - Total Solar Eclipse of 2001 june 21 - Composite of several images showing details in the crown. Different images combined to create an image which captures the visual appearance of the corona

Sebastian Voltmer

PIX4627764

Total Eclipse of Sun. 01/08/2008 - Total Solar Eclipse of 2008 august 01 - Composite of 23 images showing the solar crown, the ash light (the Moon lit by the Earth) and the stars. Solar corona, Earth - lit Moon and stars It is a composition of 23 images showing the solar corona in very high resolution and also the Earth - lit Moon and stars up to 11 magnitude. The brightest star (4 magn.) is slightly blurred by the motion of the Sun during the eclipse. The position of the Moon represents the situation 54 seconds after the second contact (18:04:29 local time in Mongolia). Both the display of the solar corona and the lunar surface in the resulting image are beyond the ability of human vision during the eclipse

Total Eclipse of Sun. 01/08/2008 - Total Solar Eclipse of 2008 august 01 - Composite of 23 images showing the solar crown, the ash light (the Moon lit by the Earth) and the stars. Solar corona, Earth - lit Moon and stars It is a composition of 23 images showing the solar corona in very high resolution and also the Earth - lit Moon and stars up to 11 magnitude. The brightest star (4 magn.) is slightly blurred by the motion of the Sun during the eclipse. The position of the Moon represents the situation 54 seconds after the second contact (18:04:29 local time in Mongolia). Both the display of the solar corona and the lunar surface in the resulting image are beyond the ability of human vision during the eclipse

PIX4628057

Total solar eclipse 10/1995 - Total solar eclipse 10/1995 - Total solar eclipse observed in India on 24 October 1995. This image shows the typical shape of the solar crown observed during the minimum solar activity cycle. The structure of the solar crown changes significantly during the eleven years of a solar cycle; it extends in all directions during the solar maximum, as in the total eclipses of 1990, 1999 or 2001, while close to the solar minimum the intensity of the crown is much more important at the equator than at the poles. Total solar eclipse as seen in India. October 24, 1995. This image shows the coronal shape typical for minimum of the solar activity cycle. The coronal structure is changing during the eleven - year solar cycle significantly. It is spread approximately evenly to all spatial directions near the solar cycle maximum (for example 1990, 1999, 2001 eclipses) but near the solar cycle minimum the coronal intensity is much greater in equatorial plane than in polar r

Total solar eclipse 10/1995 - Total solar eclipse 10/1995 - Total solar eclipse observed in India on 24 October 1995. This image shows the typical shape of the solar crown observed during the minimum solar activity cycle. The structure of the solar crown changes significantly during the eleven years of a solar cycle; it extends in all directions during the solar maximum, as in the total eclipses of 1990, 1999 or 2001, while close to the solar minimum the intensity of the crown is much more important at the equator than at the poles. Total solar eclipse as seen in India. October 24, 1995. This image shows the coronal shape typical for minimum of the solar activity cycle. The coronal structure is changing during the eleven - year solar cycle significantly. It is spread approximately evenly to all spatial directions near the solar cycle maximum (for example 1990, 1999, 2001 eclipses) but near the solar cycle minimum the coronal intensity is much greater in equatorial plane than in polar r

PIX4627374

Total Eclipse de Soleil. 01/08/2008 - Total Solar Eclipse of 2008 august 01 - All phases of the total eclipse of Sun from August 1st 2008. One image every 5 minutes before and after Total Solar Eclipse of 2008 august 01 seen in Mongolia. The different phases are shown in this composite of images taken every 5 minutes

Total Eclipse de Soleil. 01/08/2008 - Total Solar Eclipse of 2008 august 01 - All phases of the total eclipse of Sun from August 1st 2008. One image every 5 minutes before and after Total Solar Eclipse of 2008 august 01 seen in Mongolia. The different phases are shown in this composite of images taken every 5 minutes

G. Cannat

PIX4628172

Sun cutaway - Sun cutaway - At the bottom left, the Earth is represented. Bottom left is the Earth

Sun cutaway - Sun cutaway - At the bottom left, the Earth is represented. Bottom left is the Earth

PIX4629404

Total solar eclipse -Turkey 29 March 2006 - Total solar eclipse -Turkey -March 29, 2006

Total solar eclipse -Turkey 29 March 2006 - Total solar eclipse -Turkey -March 29, 2006

Alex Conu

PIX4583381

Total Eclipse of Sun - 09/03/2016 - Total Solar Eclipse - March 9 2016: Total Eclipse of Sun of 9 March 2016 seen in Indonesia. Baily grains. Baily's beads.

Total Eclipse of Sun - 09/03/2016 - Total Solar Eclipse - March 9 2016: Total Eclipse of Sun of 9 March 2016 seen in Indonesia. Baily grains. Baily's beads.

PIX4628461

A male Turkey showing off his Snood, (photo)

A male Turkey showing off his Snood, (photo)

DGC834308

Total Eclipse of Sun 22/07/2009 - Total Solar Eclipse - July 22 2009 - Total Sun Eclipse of 22 July 2009 seen in China, about fifty kilometers from Hangzhou city. Total Solar Eclipse seen from China near Hangzhou

Total Eclipse of Sun 22/07/2009 - Total Solar Eclipse - July 22 2009 - Total Sun Eclipse of 22 July 2009 seen in China, about fifty kilometers from Hangzhou city. Total Solar Eclipse seen from China near Hangzhou

PIX4628150

Total Eclipse of Sun - 21/08/2017 - Total Solar Eclipse - August 21 2017: Diamond effect at the end of the total eclipse. Ocean Lake, Wyoming, USA. Total solar eclipse on 2017 August 21 from Ocean Lake, Wyoming, USA

Total Eclipse of Sun - 21/08/2017 - Total Solar Eclipse - August 21 2017: Diamond effect at the end of the total eclipse. Ocean Lake, Wyoming, USA. Total solar eclipse on 2017 August 21 from Ocean Lake, Wyoming, USA

Sebastian Voltmer

PIX4628479

Total Eclipse of Sun. 01/08/2008 - Total Solar Eclipse of 2008 august 01 - Composite of images showing the solar crown, the ash light (the Moon lit by the Earth) the stars around the Sun (with the cluster of stars M44 at the top right) and the planet Mercury (bright dot on the left). 01/08/2008, Mongolia. Data from two different cameras were used for this image creation. The open cluster M 44 Praesepae (NGC 2632) dominates the star field. The bright object in the left part of the image is Mercury. The solar corona is traceable up to the distance of 20 solar radii. The position of the Moon represents the situation 62 seconds after the second contact (18:04:37 mongolia local time). Display of the solar corona, lunar surface and stars in the resulting image are highly beyond the ability of human vision during the eclipse

Total Eclipse of Sun. 01/08/2008 - Total Solar Eclipse of 2008 august 01 - Composite of images showing the solar crown, the ash light (the Moon lit by the Earth) the stars around the Sun (with the cluster of stars M44 at the top right) and the planet Mercury (bright dot on the left). 01/08/2008, Mongolia. Data from two different cameras were used for this image creation. The open cluster M 44 Praesepae (NGC 2632) dominates the star field. The bright object in the left part of the image is Mercury. The solar corona is traceable up to the distance of 20 solar radii. The position of the Moon represents the situation 62 seconds after the second contact (18:04:37 mongolia local time). Display of the solar corona, lunar surface and stars in the resulting image are highly beyond the ability of human vision during the eclipse

PIX4628063

Total Eclipse of Sun - 21/08/2017 - Total Solar Eclipse - August 21 2017: Last sunlight before total eclipse. Ocean Lake, Wyoming, USA.

Total Eclipse of Sun - 21/08/2017 - Total Solar Eclipse - August 21 2017: Last sunlight before total eclipse. Ocean Lake, Wyoming, USA.

Sebastian Voltmer

PIX4628452

Total Eclipse of Sun - 21/08/2017 - Total Solar Eclipse - August 21 2017: High resolution image. Ocean Lake, Wyoming, USA.

Total Eclipse of Sun - 21/08/2017 - Total Solar Eclipse - August 21 2017: High resolution image. Ocean Lake, Wyoming, USA.

Sebastian Voltmer

PIX4583437

Total Eclipse of Sun - 21/08/2017 - Total Solar Eclipse - August 21 2017: High resolution image. Ocean Lake, Wyoming, USA

Total Eclipse of Sun - 21/08/2017 - Total Solar Eclipse - August 21 2017: High resolution image. Ocean Lake, Wyoming, USA

Sebastian Voltmer

PIX4583450

Total Eclipse of Soleil - 21/08/2017 - Solar corona during the eclipse of August 21 2017 - Composite image highlighting the solar crown. Ocean Lake, Wyoming, USA. A composite of multiple frames to reveal the huge dynamic range of the Solar corona. Earthshine is also visible on the Moon. The image was taken during the August 21 2017 total solar eclipse in Wyoming, USA

Total Eclipse of Soleil - 21/08/2017 - Solar corona during the eclipse of August 21 2017 - Composite image highlighting the solar crown. Ocean Lake, Wyoming, USA. A composite of multiple frames to reveal the huge dynamic range of the Solar corona. Earthshine is also visible on the Moon. The image was taken during the August 21 2017 total solar eclipse in Wyoming, USA

Alex Conu

PIX4628486

Total Eclipse of Sun - 21/08/2017 - Total Solar Eclipse - August 21 2017: Protuberances visible during total eclipse. Ocean Lake, Wyoming, USA. Chromosphere & Prominences, Eclipse 2017; USA from Ocean Lake, Wyoming, USA

Total Eclipse of Sun - 21/08/2017 - Total Solar Eclipse - August 21 2017: Protuberances visible during total eclipse. Ocean Lake, Wyoming, USA. Chromosphere & Prominences, Eclipse 2017; USA from Ocean Lake, Wyoming, USA

Sebastian Voltmer

PIX4583433

Total Solar Eclipse - 21/08/2017 - Total Solar Eclipse - August 21 2017: Total solar eclipse on 2017 August 21 from Ocean Lake, Wyoming, USA

Total Solar Eclipse - 21/08/2017 - Total Solar Eclipse - August 21 2017: Total solar eclipse on 2017 August 21 from Ocean Lake, Wyoming, USA

Sebastian Voltmer

PIX4628476

Solar protuberance seen in ultraviolet by SOHO on 31 - 07 - 2003 - A protuberance, a plasma cloud, escapes from the Sun

Solar protuberance seen in ultraviolet by SOHO on 31 - 07 - 2003 - A protuberance, a plasma cloud, escapes from the Sun

PIX4626914

Solar protuberance seen in ultraviolet by SOHO on 25 - 10 - 2002 - A protuberance, a plasma cloud, escapes from the Sun

Solar protuberance seen in ultraviolet by SOHO on 25 - 10 - 2002 - A protuberance, a plasma cloud, escapes from the Sun

PIX4626906

The Sun Seen in Ultraviolet by SOHO 18 - 01 - 2000 - A protuberance, a plasma cloud, escapes from the Sun. White regions are the hottest and most active areas

The Sun Seen in Ultraviolet by SOHO 18 - 01 - 2000 - A protuberance, a plasma cloud, escapes from the Sun. White regions are the hottest and most active areas

PIX4626854

The Sun seen in ultraviolet by SOHO on 14 - 09 - 1997 - A protuberance, a plasma cloud, escapes from the Sun. White regions are the hottest and most active areas

The Sun seen in ultraviolet by SOHO on 14 - 09 - 1997 - A protuberance, a plasma cloud, escapes from the Sun. White regions are the hottest and most active areas

PIX4626880

The Sun seen in ultraviolet by SOHO on 23 - 04 - 2001 - A protuberance, a plasma cloud, escapes from the Sun. White regions are the hottest and most active areas

The Sun seen in ultraviolet by SOHO on 23 - 04 - 2001 - A protuberance, a plasma cloud, escapes from the Sun. White regions are the hottest and most active areas

PIX4626889

The Sun seen in ultraviolet by SOHO on 25 - 10 - 2002 - A protuberance, a plasma cloud, escapes from the Sun. White regions are the hottest and most active areas

The Sun seen in ultraviolet by SOHO on 25 - 10 - 2002 - A protuberance, a plasma cloud, escapes from the Sun. White regions are the hottest and most active areas

PIX4626893

The Sun seen in ultraviolet by SOHO on 20 - 10 - 2001 - A protuberance, a plasma cloud, escapes from the Sun. White regions are the hottest and most active areas

The Sun seen in ultraviolet by SOHO on 20 - 10 - 2001 - A protuberance, a plasma cloud, escapes from the Sun. White regions are the hottest and most active areas

PIX4626883

The Sun seen in ultraviolet by SOHO on 11 - 04 - 2003 - A protuberance, a plasma cloud, escapes from the Sun. White regions are the hottest and most active areas

The Sun seen in ultraviolet by SOHO on 11 - 04 - 2003 - A protuberance, a plasma cloud, escapes from the Sun. White regions are the hottest and most active areas

PIX4626921

The Sun seen in ultraviolet by SOHO on 27 - 08 - 1997 - A protuberance, a plasma cloud, escapes from the Sun for over 350,000 km. White regions are the hottest and most active areas

The Sun seen in ultraviolet by SOHO on 27 - 08 - 1997 - A protuberance, a plasma cloud, escapes from the Sun for over 350,000 km. White regions are the hottest and most active areas

PIX4626838

The Sun seen in ultraviolet by SOHO on 28 - 07 - 2005 - A protuberance, a plasma cloud, escapes from the Sun. White regions are the hottest and most active areas

The Sun seen in ultraviolet by SOHO on 28 - 07 - 2005 - A protuberance, a plasma cloud, escapes from the Sun. White regions are the hottest and most active areas

PIX4626934

The Sun seen in ultraviolet by SOHO 01 - 07 - 2002 - A protuberance, a plasma cloud, escapes from the Sun. White regions are the hottest and most active areas

The Sun seen in ultraviolet by SOHO 01 - 07 - 2002 - A protuberance, a plasma cloud, escapes from the Sun. White regions are the hottest and most active areas

PIX4626965

The Sun seen in ultraviolet by SOHO on 09 - 06 - 2002 - A huge protuberance, a plasma cloud, escapes from the Sun. White regions are the hottest and most active areas

The Sun seen in ultraviolet by SOHO on 09 - 06 - 2002 - A huge protuberance, a plasma cloud, escapes from the Sun. White regions are the hottest and most active areas

PIX4626869

Clay cup with bow-shaped protuberance with small serrated edge and decorated with motif depicting tangle of ropes, circa 1000 BC, 9.5 cm, Japanese civilization, late Jomon period, 2000-200 BC

Clay cup with bow-shaped protuberance with small serrated edge and decorated with motif depicting tangle of ropes, circa 1000 BC, 9.5 cm, Japanese civilization, late Jomon period, 2000-200 BC

Japanese School, Jomon Period (c.14000-300 B.C.)

DGA1085446

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