|
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SOHO/MDI's 'Window' Through
…
| Title |
SOHO/MDI's 'Window' Through the Sun |
| Abstract |
Using the mathematical techniques, the SOHO/MDI view of the front side of the Sun can be processed to reveal features on the far side of the Sun. |
| Completed |
2004-01-21 |
|
SOHO/MDI's 'Window' Through
…
| Title |
SOHO/MDI's 'Window' Through the Sun |
| Abstract |
Using the mathematical techniques, the SOHO/MDI view of the front side of the Sun can be processed to reveal features on the far side of the Sun. |
| Completed |
2004-01-21 |
|
SOHO/MDI's 'Window' Through
…
| Title |
SOHO/MDI's 'Window' Through the Sun |
| Abstract |
Using the mathematical techniques, the SOHO/MDI view of the front side of the Sun can be processed to reveal features on the far side of the Sun. |
| Completed |
2004-01-21 |
|
SOHO/MDI's 'Window' Through
…
| Title |
SOHO/MDI's 'Window' Through the Sun |
| Abstract |
Using the mathematical techniques, the SOHO/MDI view of the front side of the Sun can be processed to reveal features on the far side of the Sun. |
| Completed |
2004-01-21 |
|
SOHO/MDI's 'Window' Through
…
| Title |
SOHO/MDI's 'Window' Through the Sun |
| Abstract |
Using the mathematical techniques, the SOHO/MDI view of the front side of the Sun can be processed to reveal features on the far side of the Sun. |
| Completed |
2004-01-21 |
|
SOHO/MDI's 'Window' Through
…
| Title |
SOHO/MDI's 'Window' Through the Sun |
| Abstract |
Using the mathematical techniques, the SOHO/MDI view of the front side of the Sun can be processed to reveal features on the far side of the Sun. |
| Completed |
2004-01-21 |
|
SOHO/MDI Investigates Solar
…
| Title |
SOHO/MDI Investigates Solar Flows Under Sunspots |
| Abstract |
SOHO/MDI performs a 'sonogram' of the sun, revealing the subsurface temperature profile around a sunspot. Red isosurfaces denote regions where the sound speed (and temperature) are higher than average while blue isosurfaces directly under the spot illustrate where the sound speed (and temperature) are lower than average. |
| Completed |
2001-08-31 |
|
SOHO/MDI Investigates Solar
…
| Title |
SOHO/MDI Investigates Solar Flows Under Sunspots |
| Abstract |
SOHO/MDI performs a 'sonogram' of the sun, revealing the subsurface temperature profile around a sunspot. Red isosurfaces denote regions where the sound speed (and temperature) are higher than average while blue isosurfaces directly under the spot illustrate where the sound speed (and temperature) are lower than average. |
| Completed |
2001-08-31 |
|
SOHO/MDI Investigates Solar
…
| Title |
SOHO/MDI Investigates Solar Flows Under Sunspots |
| Abstract |
SOHO/MDI performs a 'sonogram' of the sun, revealing the subsurface temperature profile around a sunspot. Red isosurfaces denote regions where the sound speed (and temperature) are higher than average while blue isosurfaces directly under the spot illustrate where the sound speed (and temperature) are lower than average. |
| Completed |
2001-08-31 |
|
SOHO/MDI Investigates Solar
…
| Title |
SOHO/MDI Investigates Solar Flows Under Sunspots |
| Abstract |
SOHO/MDI performs a 'sonogram' of the sun, revealing the subsurface temperature profile around a sunspot. Red isosurfaces denote regions where the sound speed (and temperature) are higher than average while blue isosurfaces directly under the spot illustrate where the sound speed (and temperature) are lower than average. |
| Completed |
2001-08-31 |
|
SOHO/MDI Investigates Solar
…
| Title |
SOHO/MDI Investigates Solar Flows Under Sunspots |
| Abstract |
SOHO/MDI performs a 'sonogram' of the sun, revealing the subsurface temperature profile around a sunspot. Red isosurfaces denote regions where the sound speed (and temperature) are higher than average while blue isosurfaces directly under the spot illustrate where the sound speed (and temperature) are lower than average. |
| Completed |
2001-08-31 |
|
SOHO/MDI Investigates Solar
…
| Title |
SOHO/MDI Investigates Solar Flows Under Sunspots |
| Abstract |
SOHO/MDI performs a 'sonogram' of the sun, revealing the subsurface temperature profile around a sunspot. Red isosurfaces denote regions where the sound speed (and temperature) are higher than average while blue isosurfaces directly under the spot illustrate where the sound speed (and temperature) are lower than average. |
| Completed |
2001-08-31 |
|
Solar Tsunamis
| Title |
Solar Tsunamis |
| Abstract |
Push-in to a region of the Sun to witness a 'solar tsunami' after a flare event. The tsunami moves hot gas (bright) out of the region, revealing cooler regions (darker) below. |
| Completed |
2004-01-07 |
|
Solar Tsunamis
| Title |
Solar Tsunamis |
| Abstract |
Push-in to a region of the Sun to witness a 'solar tsunami' after a flare event. The tsunami moves hot gas (bright) out of the region, revealing cooler regions (darker) below. |
| Completed |
2004-01-07 |
|
Solar Tsunamis
| Title |
Solar Tsunamis |
| Abstract |
Push-in to a region of the Sun to witness a 'solar tsunami' after a flare event. The tsunami moves hot gas (bright) out of the region, revealing cooler regions (darker) below. |
| Completed |
2004-01-07 |
|
Solar Tsunamis
| Title |
Solar Tsunamis |
| Abstract |
Push-in to a region of the Sun to witness a 'solar tsunami' after a flare event. The tsunami moves hot gas (bright) out of the region, revealing cooler regions (darker) below. |
| Completed |
2004-01-07 |
|
Hinode's High-Resolution Vie
…
| Title |
Hinode's High-Resolution View of the Sun |
| Abstract |
A new sunspot collided with an existing sunspot which built up a highly sheared magnetic configuration. This resulted in a solar flare on December 13, 2006. |
| Completed |
2007-03-16 |
|
Hinode's High-Resolution Vie
…
| Title |
Hinode's High-Resolution View of the Sun |
| Abstract |
A new sunspot collided with an existing sunspot which built up a highly sheared magnetic configuration. This resulted in a solar flare on December 13, 2006. |
| Completed |
2007-03-16 |
|
Hinode's High-Resolution Vie
…
| Title |
Hinode's High-Resolution View of the Sun |
| Abstract |
A new sunspot collided with an existing sunspot which built up a highly sheared magnetic configuration. This resulted in a solar flare on December 13, 2006. |
| Completed |
2007-03-16 |
|
RHESSI Observes the Flare ov
…
| Title |
RHESSI Observes the Flare over AR9906 - rotate view without times |
| Abstract |
Zoom in (with rotation) to solar active region AR9906 on April 21, 2002 with SOHO/EIT, TRACE and RHESSI data. RHESSI observes x-rays from this flare. The red contours represent the 12-25 keV photon energy range and the blue contours represent 50-100 keV. |
| Completed |
2002-06-03 |
|
RHESSI Observes the Flare ov
…
| Title |
RHESSI Observes the Flare over AR9906 - rotate view without times |
| Abstract |
Zoom in (with rotation) to solar active region AR9906 on April 21, 2002 with SOHO/EIT, TRACE and RHESSI data. RHESSI observes x-rays from this flare. The red contours represent the 12-25 keV photon energy range and the blue contours represent 50-100 keV. |
| Completed |
2002-06-03 |
|
RHESSI Observes the Flare ov
…
| Title |
RHESSI Observes the Flare over AR9906 - rotate view without times |
| Abstract |
Zoom in (with rotation) to solar active region AR9906 on April 21, 2002 with SOHO/EIT, TRACE and RHESSI data. RHESSI observes x-rays from this flare. The red contours represent the 12-25 keV photon energy range and the blue contours represent 50-100 keV. |
| Completed |
2002-06-03 |
|
RHESSI Observes the Flare ov
…
| Title |
RHESSI Observes the Flare over AR9906 - rotate view without times |
| Abstract |
Zoom in (with rotation) to solar active region AR9906 on April 21, 2002 with SOHO/EIT, TRACE and RHESSI data. RHESSI observes x-rays from this flare. The red contours represent the 12-25 keV photon energy range and the blue contours represent 50-100 keV. |
| Completed |
2002-06-03 |
|
RHESSI Observes the Flare ov
…
| Title |
RHESSI Observes the Flare over AR9906 - rotate view without times |
| Abstract |
Zoom in (with rotation) to solar active region AR9906 on April 21, 2002 with SOHO/EIT, TRACE and RHESSI data. RHESSI observes x-rays from this flare. The red contours represent the 12-25 keV photon energy range and the blue contours represent 50-100 keV. |
| Completed |
2002-06-03 |
|
RHESSI Observes the Flare ov
…
| Title |
RHESSI Observes the Flare over AR9906 - rotate view without times |
| Abstract |
Zoom in (with rotation) to solar active region AR9906 on April 21, 2002 with SOHO/EIT, TRACE and RHESSI data. RHESSI observes x-rays from this flare. The red contours represent the 12-25 keV photon energy range and the blue contours represent 50-100 keV. |
| Completed |
2002-06-03 |
|
RHESSI Observes the Flare ov
…
| Title |
RHESSI Observes the Flare over AR9906 - rotate view without times |
| Abstract |
Zoom in (with rotation) to solar active region AR9906 on April 21, 2002 with SOHO/EIT, TRACE and RHESSI data. RHESSI observes x-rays from this flare. The red contours represent the 12-25 keV photon energy range and the blue contours represent 50-100 keV. |
| Completed |
2002-06-03 |
|
SOHO/MDI Views the Sun - 199
…
| Title |
SOHO/MDI Views the Sun - 1998 |
| Abstract |
This version projects the solar image on a flat plane. It runs at a third of the speed of the original version. |
| Completed |
2001-09-28 |
|
SOHO/MDI Views the Sun - 199
…
| Title |
SOHO/MDI Views the Sun - 1998 |
| Abstract |
This version projects the solar image on a flat plane. It runs at a third of the speed of the original version. |
| Completed |
2001-09-28 |
|
SOHO/MDI Views the Sun - 199
…
| Title |
SOHO/MDI Views the Sun - 1998 |
| Abstract |
This version projects the solar image on a flat plane. It runs at a third of the speed of the original version. |
| Completed |
2001-09-28 |
|
Solar Tsunamis - View with a
…
| Title |
Solar Tsunamis - View with a Spin |
| Abstract |
Push-in to a region of the Sun to witness a 'solar tsunami' after a flare event. The tsunami moves hot gas (bright) out of the region, revealing cooler regions (darker) below. This view rotates on the push-in to keep the region of the flare event visible (to the left in the final frame). |
| Completed |
2003-10-21 |
|
Solar Tsunamis - View with a
…
| Title |
Solar Tsunamis - View with a Spin |
| Abstract |
Push-in to a region of the Sun to witness a 'solar tsunami' after a flare event. The tsunami moves hot gas (bright) out of the region, revealing cooler regions (darker) below. This view rotates on the push-in to keep the region of the flare event visible (to the left in the final frame). |
| Completed |
2003-10-21 |
|
Solar Tsunamis - View with a
…
| Title |
Solar Tsunamis - View with a Spin |
| Abstract |
Push-in to a region of the Sun to witness a 'solar tsunami' after a flare event. The tsunami moves hot gas (bright) out of the region, revealing cooler regions (darker) below. This view rotates on the push-in to keep the region of the flare event visible (to the left in the final frame). |
| Completed |
2003-10-21 |
|
Solar Tsunamis - View with a
…
| Title |
Solar Tsunamis - View with a Spin |
| Abstract |
Push-in to a region of the Sun to witness a 'solar tsunami' after a flare event. The tsunami moves hot gas (bright) out of the region, revealing cooler regions (darker) below. This view rotates on the push-in to keep the region of the flare event visible (to the left in the final frame). |
| Completed |
2003-10-21 |
|
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