112 images found
Display Options:
Currently displaying images 1-25 of 112
1 2 3
Sort by:
NASA's Solar Dynamics Observatory shows that over the course of just one day a tiny active region grew to became almost as large as its many-days-old neighbor (Aug. 23-24, 2018).
NASA's Solar Dynamics Observatory shows that over the course of just one day a tiny active region grew to became almost as large as its many-days-old neighbor (Aug. 23-24, 2018).

New Active Region Grows Up

NASA's Solar Dynamics Observatory shows that over the course of just one day a tiny active region grew to became almost as large as its many-days-old neighbor (Aug. 23-24, 2018).

Target: Sun
Mission: Solar Dynamics Observatory (SDO)
Instrument: Atmosphere Imaging Assembly (AIA)
ID#: PIA22680
Added: 2018-09-03

Views: 143

New Active Region Grows Up

NASA's Solar Dynamics Observatory shows that over the course of just one day a tiny active region grew to became almost as large as its many-days-old neighbor (Aug. 23-24, 2018).

Email this page Post this page to your Facebook wall Tweet this page

Formats:
Full-Res TIFF: Download, Full-Res JPEG: Download

Add image to your album
NASA's Solar Dynamics Observatory shows a minor eruption of charged particles rising up and twisting about before falling back into the Sun in this close-up of the Sun from a two-hour period on Aug. 13, 2018.
NASA's Solar Dynamics Observatory shows a minor eruption of charged particles rising up and twisting about before falling back into the Sun in this close-up of the Sun from a two-hour period on Aug. 13, 2018.

Twisting Outburst

NASA's Solar Dynamics Observatory shows a minor eruption of charged particles rising up and twisting about before falling back into the Sun in this close-up of the Sun from a two-hour period on Aug. 13, 2018.

Target: Sun
Mission: Solar Dynamics Observatory (SDO)
Instrument: Atmosphere Imaging Assembly (AIA)
ID#: PIA22673
Added: 2018-08-20

Views: 288

Twisting Outburst

NASA's Solar Dynamics Observatory shows a minor eruption of charged particles rising up and twisting about before falling back into the Sun in this close-up of the Sun from a two-hour period on Aug. 13, 2018.

Email this page Post this page to your Facebook wall Tweet this page

Formats:
Full-Res TIFF: Download, Full-Res JPEG: Download

Add image to your album
NASA's Solar Dynamics Observatory scientists use their computer models to generate a view of the sun's magnetic field. An extreme ultraviolet view of the sun is compared with the same image showing the superimposed field lines on August 10, 2018.
NASA's Solar Dynamics Observatory scientists use their computer models to generate a view of the sun's magnetic field. An extreme ultraviolet view of the sun is compared with the same image showing the superimposed field lines on August 10, 2018.

Magnetic Field Portrayed

NASA's Solar Dynamics Observatory scientists use their computer models to generate a view of the sun's magnetic field. An extreme ultraviolet view of the sun is compared with the same image showing the superimposed field lines on August 10, 2018.

Target: Sun
Mission: Solar Dynamics Observatory (SDO)
Instrument: Atmosphere Imaging Assembly (AIA)
ID#: PIA22662
Added: 2018-08-14

Views: 686

Magnetic Field Portrayed

NASA's Solar Dynamics Observatory scientists use their computer models to generate a view of the sun's magnetic field. An extreme ultraviolet view of the sun is compared with the same image showing the superimposed field lines on August 10, 2018.

Email this page Post this page to your Facebook wall Tweet this page

Formats:
Full-Res TIFF: Download, Full-Res JPEG: Download

Add image to your album
NASA's Solar Dynamics Observatory observes two relatively small prominences above the Sun's surface twisted and streamed charged particles over a 20-hour period July 30-31, 2018.
NASA's Solar Dynamics Observatory observes two relatively small prominences above the Sun's surface twisted and streamed charged particles over a 20-hour period July 30-31, 2018.

Twisting Prominences

NASA's Solar Dynamics Observatory observes two relatively small prominences above the Sun's surface twisted and streamed charged particles over a 20-hour period July 30-31, 2018.

Target: Sun
Mission: Solar Dynamics Observatory (SDO)
Instrument: Atmosphere Imaging Assembly (AIA)
ID#: PIA22661
Added: 2018-08-07

Views: 254

Twisting Prominences

NASA's Solar Dynamics Observatory observes two relatively small prominences above the Sun's surface twisted and streamed charged particles over a 20-hour period July 30-31, 2018.

Email this page Post this page to your Facebook wall Tweet this page

Formats:
Full-Res TIFF: Download, Full-Res JPEG: Download

Add image to your album
Over a three-week period July 3-24, 2018, NASA's Solar Dynamics Observatory observed the Sun produced just one small, short-lived sunspot -- an almost spotless record.
Over a three-week period July 3-24, 2018, NASA's Solar Dynamics Observatory observed the Sun produced just one small, short-lived sunspot -- an almost spotless record.

An Almost Spotless Record

Over a three-week period July 3-24, 2018, NASA's Solar Dynamics Observatory observed the Sun produced just one small, short-lived sunspot -- an almost spotless record.

Target: Sun
Mission: Solar Dynamics Observatory (SDO)
Instrument: Atmosphere Imaging Assembly (AIA)
ID#: PIA22646
Added: 2018-07-30

Views: 233

An Almost Spotless Record

Over a three-week period July 3-24, 2018, NASA's Solar Dynamics Observatory observed the Sun produced just one small, short-lived sunspot -- an almost spotless record.

Email this page Post this page to your Facebook wall Tweet this page

Formats:
Full-Res TIFF: Download, Full-Res JPEG: Download

Add image to your album
NASA's Solar Dynamics Observatory zoomed in to watch close-up the dynamics of this single active region on the sun over a two-day period on July 14-16, 2018. These regions are often the sources of large eruptions that cause solar storms.
NASA's Solar Dynamics Observatory zoomed in to watch close-up the dynamics of this single active region on the sun over a two-day period on July 14-16, 2018. These regions are often the sources of large eruptions that cause solar storms.

Detailed Loops Above an Active Region

NASA's Solar Dynamics Observatory zoomed in to watch close-up the dynamics of this single active region on the sun over a two-day period on July 14-16, 2018. These regions are often the sources of large eruptions that cause solar storms.

Target: Sun
Mission: Solar Dynamics Observatory (SDO)
Instrument: Atmosphere Imaging Assembly (AIA)
ID#: PIA22645
Added: 2018-07-23

Views: 205

Detailed Loops Above an Active Region

NASA's Solar Dynamics Observatory zoomed in to watch close-up the dynamics of this single active region on the sun over a two-day period on July 14-16, 2018. These regions are often the sources of large eruptions that cause solar storms.

Email this page Post this page to your Facebook wall Tweet this page

Formats:
Full-Res TIFF: Download, Full-Res JPEG: Download

Add image to your album
NASA's Solar Dynamics Observatory observed this profile perspective of an active region revealed above it June 24-25, 2018. Charged particles spinning along these field lines are illuminated in this wavelength of extreme ultraviolet light.
NASA's Solar Dynamics Observatory observed this profile perspective of an active region revealed above it June 24-25, 2018. Charged particles spinning along these field lines are illuminated in this wavelength of extreme ultraviolet light.

Festoons of Loops

NASA's Solar Dynamics Observatory observed this profile perspective of an active region revealed above it June 24-25, 2018. Charged particles spinning along these field lines are illuminated in this wavelength of extreme ultraviolet light.

Target: Sun
Mission: Solar Dynamics Observatory (SDO)
Instrument: Atmosphere Imaging Assembly (AIA)
ID#: PIA22589
Added: 2018-07-17

Views: 318

Festoons of Loops

NASA's Solar Dynamics Observatory observed this profile perspective of an active region revealed above it June 24-25, 2018. Charged particles spinning along these field lines are illuminated in this wavelength of extreme ultraviolet light.

Email this page Post this page to your Facebook wall Tweet this page

Formats:
Full-Res TIFF: Download, Full-Res JPEG: Download

Add image to your album
NASA's Solar Dynamics Observatory observed an active region on June 19th, quickly growing in size over two days June 20-22, 2018. Active regions are areas of enhanced magnetic activity on the Sun's surface, generating the huge loops and dynamic surges.
NASA's Solar Dynamics Observatory observed an active region on June 19th, quickly growing in size over two days June 20-22, 2018. Active regions are areas of enhanced magnetic activity on the Sun's surface, generating the huge loops and dynamic surges.

Rambunctious Active Region

NASA's Solar Dynamics Observatory observed an active region on June 19th, quickly growing in size over two days June 20-22, 2018. Active regions are areas of enhanced magnetic activity on the Sun's surface, generating the huge loops and dynamic surges.

Target: Sun
Mission: Solar Dynamics Observatory (SDO)
Instrument: Atmosphere Imaging Assembly (AIA)
ID#: PIA22582
Added: 2018-07-05

Views: 622

Rambunctious Active Region

NASA's Solar Dynamics Observatory observed an active region on June 19th, quickly growing in size over two days June 20-22, 2018. Active regions are areas of enhanced magnetic activity on the Sun's surface, generating the huge loops and dynamic surges.

Email this page Post this page to your Facebook wall Tweet this page

Formats:
Full-Res TIFF: Download, Full-Res JPEG: Download

Add image to your album
NASA's Solar Dynamics Observatory observed a small prominence hovered above the sun's surface over a two-day period June 12-14, 2018, before breaking off into space.
NASA's Solar Dynamics Observatory observed a small prominence hovered above the sun's surface over a two-day period June 12-14, 2018, before breaking off into space.

Evolving Prominence

NASA's Solar Dynamics Observatory observed a small prominence hovered above the sun's surface over a two-day period June 12-14, 2018, before breaking off into space.

Target: Sun
Mission: Solar Dynamics Observatory (SDO)
Instrument: Atmosphere Imaging Assembly (AIA)
ID#: PIA22537
Added: 2018-06-25

Views: 362

Evolving Prominence

NASA's Solar Dynamics Observatory observed a small prominence hovered above the sun's surface over a two-day period June 12-14, 2018, before breaking off into space.

Email this page Post this page to your Facebook wall Tweet this page

Formats:
Full-Res TIFF: Download, Full-Res JPEG: Download

Add image to your album
NASA's Solar Dynamics Observatory observed giant, bright coronal loops trace out the magnetic field lines above an active region from June 4-6, 2018.
NASA's Solar Dynamics Observatory observed giant, bright coronal loops trace out the magnetic field lines above an active region from June 4-6, 2018.

Ballet of Loops

NASA's Solar Dynamics Observatory observed giant, bright coronal loops trace out the magnetic field lines above an active region from June 4-6, 2018.

Target: Sun
Mission: Solar Dynamics Observatory (SDO)
Instrument: Atmosphere Imaging Assembly (AIA)
ID#: PIA22508
Added: 2018-06-11

Views: 308

Ballet of Loops

NASA's Solar Dynamics Observatory observed giant, bright coronal loops trace out the magnetic field lines above an active region from June 4-6, 2018.

Email this page Post this page to your Facebook wall Tweet this page

Formats:
Full-Res TIFF: Download, Full-Res JPEG: Download

Add image to your album
This close-up from a video clip taken May 30-June 1, 2018 by NASA's Solar Dynamics Observatory shows a large active region in extreme ultraviolet light as the bright magnetic field lines above it shift and twist.
This close-up from a video clip taken May 30-June 1, 2018 by NASA's Solar Dynamics Observatory shows a large active region in extreme ultraviolet light as the bright magnetic field lines above it shift and twist.

Dynamic Looping Action

This close-up from a video clip taken May 30-June 1, 2018 by NASA's Solar Dynamics Observatory shows a large active region in extreme ultraviolet light as the bright magnetic field lines above it shift and twist.

Target: Sun
Mission: Solar Dynamics Observatory (SDO)
Instrument: Atmosphere Imaging Assembly (AIA)
ID#: PIA22475
Added: 2018-06-04

Views: 193

Dynamic Looping Action

This close-up from a video clip taken May 30-June 1, 2018 by NASA's Solar Dynamics Observatory shows a large active region in extreme ultraviolet light as the bright magnetic field lines above it shift and twist.

Email this page Post this page to your Facebook wall Tweet this page

Formats:
Full-Res TIFF: Download, Full-Res JPEG: Download

Add image to your album
On May 23-25, 2018, NASA's Solar Dynamics Observatory observed an active region that rotated into view and sputtered with numerous small flares and towering magnetic field lines that stretched out many times the diameter of Earth.
On May 23-25, 2018, NASA's Solar Dynamics Observatory observed an active region that rotated into view and sputtered with numerous small flares and towering magnetic field lines that stretched out many times the diameter of Earth.

New Active Region Sputtering with Small Flares

On May 23-25, 2018, NASA's Solar Dynamics Observatory observed an active region that rotated into view and sputtered with numerous small flares and towering magnetic field lines that stretched out many times the diameter of Earth.

Target: Sun
Mission: Solar Dynamics Observatory (SDO)
Instrument: Atmosphere Imaging Assembly (AIA)
ID#: PIA22461
Added: 2018-05-29

Views: 293

New Active Region Sputtering with Small Flares

On May 23-25, 2018, NASA's Solar Dynamics Observatory observed an active region that rotated into view and sputtered with numerous small flares and towering magnetic field lines that stretched out many times the diameter of Earth.

Email this page Post this page to your Facebook wall Tweet this page

Formats:
Full-Res TIFF: Download, Full-Res JPEG: Download

Add image to your album
On May 16-18, 2018, NASA's Solar Dynamics Observatory observed a good-sized coronal hole come around to where it is just about faced Earth. Coronal holes are areas of open magnetic field from which solar wind (charged particles) streams into space.
On May 16-18, 2018, NASA's Solar Dynamics Observatory observed a good-sized coronal hole come around to where it is just about faced Earth. Coronal holes are areas of open magnetic field from which solar wind (charged particles) streams into space.

Coronal Hole Rotating Towards Us

On May 16-18, 2018, NASA's Solar Dynamics Observatory observed a good-sized coronal hole come around to where it is just about faced Earth. Coronal holes are areas of open magnetic field from which solar wind (charged particles) streams into space.

Target: Sun
Mission: Solar Dynamics Observatory (SDO)
Instrument: Atmosphere Imaging Assembly (AIA)
ID#: PIA00575
Added: 2018-05-22

Views: 292

Coronal Hole Rotating Towards Us

On May 16-18, 2018, NASA's Solar Dynamics Observatory observed a good-sized coronal hole come around to where it is just about faced Earth. Coronal holes are areas of open magnetic field from which solar wind (charged particles) streams into space.

Email this page Post this page to your Facebook wall Tweet this page

Formats:
Full-Res TIFF: Download, Full-Res JPEG: Download

Add image to your album
On May 2-4, 2018, NASA's Solar Dynamics Observatory observed an extensive equatorial coronal hole has rotated so that it is now facing Earth. The dark coronal hole extends about halfway across the solar disk.
On May 2-4, 2018, NASA's Solar Dynamics Observatory observed an extensive equatorial coronal hole has rotated so that it is now facing Earth. The dark coronal hole extends about halfway across the solar disk.

Coronal Hole Facing Earth

On May 2-4, 2018, NASA's Solar Dynamics Observatory observed an extensive equatorial coronal hole has rotated so that it is now facing Earth. The dark coronal hole extends about halfway across the solar disk.

Target: Sun
Mission: Solar Dynamics Observatory (SDO)
Instrument: Atmosphere Imaging Assembly (AIA)
ID#: PIA00577
Added: 2018-05-15

Views: 316

Coronal Hole Facing Earth

On May 2-4, 2018, NASA's Solar Dynamics Observatory observed an extensive equatorial coronal hole has rotated so that it is now facing Earth. The dark coronal hole extends about halfway across the solar disk.

Email this page Post this page to your Facebook wall Tweet this page

Formats:
Full-Res TIFF: Download, Full-Res JPEG: Download

Add image to your album
NASA's Solar Dynamics Observatory observed an extensive equatorial, dark coronal hole extending about halfway across the solar disk on May 2-4, 2018.
NASA's Solar Dynamics Observatory observed an extensive equatorial, dark coronal hole extending about halfway across the solar disk on May 2-4, 2018.

Coronal Hole Facing Earth

NASA's Solar Dynamics Observatory observed an extensive equatorial, dark coronal hole extending about halfway across the solar disk on May 2-4, 2018.

Target: Sun
Mission: Solar Dynamics Observatory (SDO)
Instrument: Atmosphere Imaging Assembly (AIA)
ID#: PIA00624
Added: 2018-05-08

Views: 609

Coronal Hole Facing Earth

NASA's Solar Dynamics Observatory observed an extensive equatorial, dark coronal hole extending about halfway across the solar disk on May 2-4, 2018.

Email this page Post this page to your Facebook wall Tweet this page

Formats:
Full-Res TIFF: Download, Full-Res JPEG: Download

Add image to your album
NASA's Solar Dynamics Observatory observed a lone active region visible on the sun putting on a fine display with its tangled magnetic field lines swaying and twisting above it (Apr. 24-26, 2018) in a wavelength of extreme ultraviolet light.
NASA's Solar Dynamics Observatory observed a lone active region visible on the sun putting on a fine display with its tangled magnetic field lines swaying and twisting above it (Apr. 24-26, 2018) in a wavelength of extreme ultraviolet light.

Tangled Up in Blue

NASA's Solar Dynamics Observatory observed a lone active region visible on the sun putting on a fine display with its tangled magnetic field lines swaying and twisting above it (Apr. 24-26, 2018) in a wavelength of extreme ultraviolet light.

Target: Sun
Mission: Solar Dynamics Observatory (SDO)
Instrument: Atmosphere Imaging Assembly (AIA)
ID#: PIA22449
Added: 2018-05-01

Views: 617

Tangled Up in Blue

NASA's Solar Dynamics Observatory observed a lone active region visible on the sun putting on a fine display with its tangled magnetic field lines swaying and twisting above it (Apr. 24-26, 2018) in a wavelength of extreme ultraviolet light.

Email this page Post this page to your Facebook wall Tweet this page

Formats:
Full-Res TIFF: Download, Full-Res JPEG: Download

Add image to your album
A good-sized active region with bright, towering arches began to rotate into NASA's Solar Dynamics Observatory's view (Apr. 18-19, 2018).
A good-sized active region with bright, towering arches began to rotate into NASA's Solar Dynamics Observatory's view (Apr. 18-19, 2018).

Active Region Coming Around the Bend

A good-sized active region with bright, towering arches began to rotate into NASA's Solar Dynamics Observatory's view (Apr. 18-19, 2018).

Target: Sun
Mission: Solar Dynamics Observatory (SDO)
Instrument: Atmosphere Imaging Assembly (AIA)
ID#: PIA22430
Added: 2018-04-23

Views: 348

Active Region Coming Around the Bend

A good-sized active region with bright, towering arches began to rotate into NASA's Solar Dynamics Observatory's view (Apr. 18-19, 2018).

Email this page Post this page to your Facebook wall Tweet this page

Formats:
Full-Res TIFF: Download, Full-Res JPEG: Download

Add image to your album
The sun featured just one, rather small active region over the past few days, but it developed rapidly and sported a lot of magnetic activity in just one day (Apr. 11-12, 2018) as observed by NASA's Solar Dynamics Observatory.
The sun featured just one, rather small active region over the past few days, but it developed rapidly and sported a lot of magnetic activity in just one day (Apr. 11-12, 2018) as observed by NASA's Solar Dynamics Observatory.

Small but Dynamic Active Region

The sun featured just one, rather small active region over the past few days, but it developed rapidly and sported a lot of magnetic activity in just one day (Apr. 11-12, 2018) as observed by NASA's Solar Dynamics Observatory.

Target: Sun
Mission: Solar Dynamics Observatory (SDO)
Instrument: Atmosphere Imaging Assembly (AIA)
ID#: PIA06676
Added: 2018-04-20

Views: 342

Small but Dynamic Active Region

The sun featured just one, rather small active region over the past few days, but it developed rapidly and sported a lot of magnetic activity in just one day (Apr. 11-12, 2018) as observed by NASA's Solar Dynamics Observatory.

Email this page Post this page to your Facebook wall Tweet this page

Formats:
Full-Res TIFF: Download, Full-Res JPEG: Download

Add image to your album
For much of this week the sun featured three substantial coronal holes observed by NASA's Solar Dynamics Observatory April 3-6, 2018. These are areas of open magnetic field from which high speed solar wind rushes out into space.
For much of this week the sun featured three substantial coronal holes observed by NASA's Solar Dynamics Observatory April 3-6, 2018. These are areas of open magnetic field from which high speed solar wind rushes out into space.

Three Coronal Holes

For much of this week the sun featured three substantial coronal holes observed by NASA's Solar Dynamics Observatory April 3-6, 2018. These are areas of open magnetic field from which high speed solar wind rushes out into space.

Target: Sun
Mission: Solar Dynamics Observatory (SDO)
Instrument: Atmosphere Imaging Assembly (AIA)
ID#: PIA22414
Added: 2018-04-16

Views: 1201

Three Coronal Holes

For much of this week the sun featured three substantial coronal holes observed by NASA's Solar Dynamics Observatory April 3-6, 2018. These are areas of open magnetic field from which high speed solar wind rushes out into space.

Email this page Post this page to your Facebook wall Tweet this page

Formats:
Full-Res TIFF: Download, Full-Res JPEG: Download

Add image to your album
With no active regions currently on the face of the sun, NASA's Solar Dynamics Observatory observed a bristling active region showing numerous arches of bright, magnetic field lines blossoming out and towering above it beginning to rotate into view.
With no active regions currently on the face of the sun, NASA's Solar Dynamics Observatory observed a bristling active region showing numerous arches of bright, magnetic field lines blossoming out and towering above it beginning to rotate into view.

Wavelength Comparisons

With no active regions currently on the face of the sun, NASA's Solar Dynamics Observatory observed a bristling active region showing numerous arches of bright, magnetic field lines blossoming out and towering above it beginning to rotate into view.

Target: Sun
Mission: Solar Dynamics Observatory (SDO)
Instrument: Atmosphere Imaging Assembly (AIA)
ID#: PIA22411
Added: 2018-04-09

Views: 353

Wavelength Comparisons

With no active regions currently on the face of the sun, NASA's Solar Dynamics Observatory observed a bristling active region showing numerous arches of bright, magnetic field lines blossoming out and towering above it beginning to rotate into view.

Email this page Post this page to your Facebook wall Tweet this page

Formats:
Full-Res TIFF: Download, Full-Res JPEG: Download

Add image to your album
NASA's Solar Dynamics Observatory ran together three sequences of the sun taken in three different extreme ultraviolet wavelengths to show how different features appearing in one sequence are difficult to see in the others (Mar. 20-21, 2018).
NASA's Solar Dynamics Observatory ran together three sequences of the sun taken in three different extreme ultraviolet wavelengths to show how different features appearing in one sequence are difficult to see in the others (Mar. 20-21, 2018).

Wavelength Comparisons

NASA's Solar Dynamics Observatory ran together three sequences of the sun taken in three different extreme ultraviolet wavelengths to show how different features appearing in one sequence are difficult to see in the others (Mar. 20-21, 2018).

Target: Sun
Mission: Solar Dynamics Observatory (SDO)
Instrument: Atmosphere Imaging Assembly (AIA)
ID#: PIA22360
Added: 2018-04-02

Views: 669

Wavelength Comparisons

NASA's Solar Dynamics Observatory ran together three sequences of the sun taken in three different extreme ultraviolet wavelengths to show how different features appearing in one sequence are difficult to see in the others (Mar. 20-21, 2018).

Email this page Post this page to your Facebook wall Tweet this page

Formats:
Full-Res TIFF: Download, Full-Res JPEG: Download

Add image to your album
Coronal holes are areas of open magnetic fields from which solar wind rushes out into space. NASA's Solar Dynamics Observatory observed this long coronal hole that stretched out across more than half the diameter of the sun (Mar. 13-15, 2018).
Coronal holes are areas of open magnetic fields from which solar wind rushes out into space. NASA's Solar Dynamics Observatory observed this long coronal hole that stretched out across more than half the diameter of the sun (Mar. 13-15, 2018).

Elongated Coronal Hole

Coronal holes are areas of open magnetic fields from which solar wind rushes out into space. NASA's Solar Dynamics Observatory observed this long coronal hole that stretched out across more than half the diameter of the sun (Mar. 13-15, 2018).

Target: Sun
Mission: Solar Dynamics Observatory (SDO)
Instrument: Atmosphere Imaging Assembly (AIA)
ID#: PIA22345
Added: 2018-03-19

Views: 790

Elongated Coronal Hole

Coronal holes are areas of open magnetic fields from which solar wind rushes out into space. NASA's Solar Dynamics Observatory observed this long coronal hole that stretched out across more than half the diameter of the sun (Mar. 13-15, 2018).

Email this page Post this page to your Facebook wall Tweet this page

Formats:
Full-Res TIFF: Download, Full-Res JPEG: Download

Add image to your album
A relatively small active region erupted twice in 18 hours on Mar. 2, 2018, as observed by NASA's Solar Dynamics Observatory. After each burst, one can see the magnetic fields lines, which appear as bright coils, spiraling around the region.
A relatively small active region erupted twice in 18 hours on Mar. 2, 2018, as observed by NASA's Solar Dynamics Observatory. After each burst, one can see the magnetic fields lines, which appear as bright coils, spiraling around the region.

Small Bursts

A relatively small active region erupted twice in 18 hours on Mar. 2, 2018, as observed by NASA's Solar Dynamics Observatory. After each burst, one can see the magnetic fields lines, which appear as bright coils, spiraling around the region.

Target: Sun
Mission: Solar Dynamics Observatory (SDO)
Instrument: Atmosphere Imaging Assembly (AIA)
ID#: PIA22260
Added: 2018-03-05

Views: 607

Small Bursts

A relatively small active region erupted twice in 18 hours on Mar. 2, 2018, as observed by NASA's Solar Dynamics Observatory. After each burst, one can see the magnetic fields lines, which appear as bright coils, spiraling around the region.

Email this page Post this page to your Facebook wall Tweet this page

Formats:
Full-Res TIFF: Download, Full-Res JPEG: Download

Add image to your album
NASA's Solar Dynamics Observatory observed the sun's only visible active region as it sputtered and spurted and eventually unleashed a small (C-class) flare on Feb. 7, 2018.
NASA's Solar Dynamics Observatory observed the sun's only visible active region as it sputtered and spurted and eventually unleashed a small (C-class) flare on Feb. 7, 2018.

One Small Flare

NASA's Solar Dynamics Observatory observed the sun's only visible active region as it sputtered and spurted and eventually unleashed a small (C-class) flare on Feb. 7, 2018.

Target: Sun
Mission: Solar Dynamics Observatory (SDO)
Instrument: Atmosphere Imaging Assembly (AIA)
ID#: PIA22244
Added: 2018-02-15

Views: 561

One Small Flare

NASA's Solar Dynamics Observatory observed the sun's only visible active region as it sputtered and spurted and eventually unleashed a small (C-class) flare on Feb. 7, 2018.

Email this page Post this page to your Facebook wall Tweet this page

Formats:
Full-Res TIFF: Download, Full-Res JPEG: Download

Add image to your album
NASA's Solar Dynamics Observatory observed no sunspots for almost two weeks (as of Feb. 1, 2018) and just has a single, tiny one that appeared on Jan. 31, 2018.
NASA's Solar Dynamics Observatory observed no sunspots for almost two weeks (as of Feb. 1, 2018) and just has a single, tiny one that appeared on Jan. 31, 2018.

Spotless Days

NASA's Solar Dynamics Observatory observed no sunspots for almost two weeks (as of Feb. 1, 2018) and just has a single, tiny one that appeared on Jan. 31, 2018.

Target: Sun
Mission: Solar Dynamics Observatory (SDO)
Instrument: Atmosphere Imaging Assembly (AIA)
ID#: PIA22242
Added: 2018-02-07

Views: 1142

Spotless Days

NASA's Solar Dynamics Observatory observed no sunspots for almost two weeks (as of Feb. 1, 2018) and just has a single, tiny one that appeared on Jan. 31, 2018.

Email this page Post this page to your Facebook wall Tweet this page

Formats:
Full-Res TIFF: Download, Full-Res JPEG: Download

Add image to your album
Currently displaying images 1-25 of 112
1 2 3