-
Highlights From SDO's 10 Years of Solar Observation
In February 2020, NASA’s Solar Dynamics Observatory — SDO — is celebrating its 10th year in space. Over the past decade the spacecraft has kept a constant eye on the Sun, studying how the Sun creates solar activity and drives space weather — the dynamic conditions in space that impact the entire solar system, including Earth.
Since its launch on Feb. 11, 2010, SDO has collected millions of scientific images of our nearest star, giving scientists new insights into its workings. SDO’s measurements of the Sun — from the interior to the atmosphere, magnetic field, and energy output — have greatly contributed to our understanding of our closest star. SDO’s images have also become iconic — if you’ve ever seen a close-up of activity on the Sun, it was likely from an SDO image.
Read more: https...
published: 11 Feb 2020
-
The Dynamic Solar Magnetic Field
While the sun is well known as the overwhelming source of visible light in our solar system, a substantial part of its influence is driven by some aspects less visible to human perception - the magnetic field.
In this visualization, the sphere represents the solar photosphere, with neutral grey indicating a magnetic field of near zero intensity, black representing a magnetic field pointing INTO the sun (south or negative polarity) and white representing a magnetic field pointing OUT of the sun (north or positive polarity). We see that these magnetic regions often appear in nearby pairs of opposite polarities - which in visible light would often correspond to a pair of sunspots.
Using this measured magnetic field on the photosphere, combined with mathematical models based on Maxwell's eq...
published: 06 Feb 2018
-
The Dynamic Solar Magnetic Field with Introduction
While the sun is well known as the overwhelming source of visible light in our solar system, a substantial part of its influence is driven by some aspects less visible to human perception - the magnetic field.
In this visualization we start a view of the Sun in visible light (similiar to what you would see from the ground on Earth), to a view in extreme ultraviolet wavelengths (only visible to space-based instruments) which shows hot plasma streaming along magnetic field lines, to a magnetogram (derived from the visible light data) and finally to a three-dimensional magnetic field model built from that data. The sphere represents the solar photosphere, with neutral grey indicating a magnetic field of near zero intensity, black representing a magnetic field pointing INTO the sun (south o...
published: 12 Mar 2018
-
Space Solar Power Demonstrator
An animated look at Caltech's Space Solar Power Demonstrator.
More info: https://www.caltech.edu/about/news/caltech-to-launch-space-solar-power-technology-demo-into-orbit-in-january
published: 03 Jan 2023
-
Having a Solar Blast - Zoom
The Sun unleashed an M-2 (medium-sized) solar flare with a spectacular coronal mass ejection (CME) on June 7, 2011. The large cloud of particles mushroomed up and fell back down looking as if it covered an area of almost half the solar surface. The Solar Dynamic Observatory (SDO) observed the flare's peak at 1:41 AM ET. SDO recorded these images in extreme ultraviolet light that show a very large eruption of cool gas.
published: 20 May 2013
-
How the Solar System really moves (Update!)
Dear World,
Before I switch to the first spoken videos of 2021, here an update to the animation of the real movement of the Solar System. A lot of you liked the moving part of the last one but found it too short. Here a longer, more elaborate version, straight to the point.
Hope you like it.
If you like my content, please consider joining my supporters on Patreon
to get some background info and other goodies:
Starts with 1$ :)
----------------------------------------------------------------
https://www.patreon.com/morn1415/
----------------------------------------------------------------
Other social Media:
https://twitter.com/morn1415
https://www.facebook.com/morn1415/
https://www.instagram.com/morn1415/
Music:
"Sunset" by "O M II N" is licensed under a Creative Commons ...
published: 10 Mar 2021
-
Solar Dynamics Observatory - Multi-filter View
The Solar Dynamics Observatory (SDO), using 10 filters, sees connections in the solar atmosphere. This visualization experiment illustrates a mechanism for highlighting these connections.
The movie opens with a full-disk view of the Sun in visible wavelengths (SDO/HMI's 617.3 nm optical light). Then the filters of SDO/AIA are applied to small pie-shaped wedges of the Sun, starting with 170 nm (pink), then 160 nm (green), 33.5 nm (blue), 30.4 nm (orange), 21.1 nm (violet), 19.3 nm (bronze), 17.1 nm (gold), 13.1 nm (aqua) and 9.4 nm (green).
We've locked the camera to rotate the view of the Sun so each wedge-shaped wavelength filter passes over a region of the Sun. As the features pass from one wavelength to the next, we can see dramatic differences in solar structures that appear ...
published: 11 Dec 2016
-
The Solar Dynamics Observatory: The Sun Up Close and Personal
The first lecture in the 2011 Exploring Space Lecture Series featured Dean Pesnell, Project Scientist for the Solar Dynamics Observatory (SDO). SDO is designed to help us better understand how the Sun works and how it influences our lives. From the very start of its mission, SDO revealed incredible views of erupting prominences and flares with amazing clarity. Learn how SDO will change how we see the Sun inside and out!
Presented as a live webcast on Thursday, March 24, 2011 at 8pm ET at the National Air and Space Museum in Washington, DC.
For more information about past & future Exploring Space Lectures, visit http://airandspace.si.edu/exploringspace
published: 30 Mar 2011
-
Adaptive Facade | Solar Shading + Light Modulation
Adaptive facade is a second skin that adapts to the environment to minimize heat gain on a highrise residential building in Vancouver, BC.
Designed in Spring 2015 by students at the University of Oregon and the collaboration of faculty at Emily Carr University in Vancouver, BC.
Designed by:
Cody Tucker
Tristan Magnuson
Joe Hudec
Casey Williams
Special thanks to:
Thomas Groppi
Stephen Duff
Turner Exhibits
Jeremy Kramp
Emily Carr University of Art + Design
published: 12 Jun 2015
-
Nassim Haramein: Solar system dynamic, DNA imprinting information, Memory, Healing
Nassim Haramein presenting at COGNOS FEST in Barcelona, Spain
Nassim Haramein has spent more than 30 years researching and discovering connections in physics, mathematics, geometry, cosmology, quantum mechanics, biology and chemistry as well as anthropology and archeology.
These studies led Haramein to groundbreaking theories, published papers and patented inventions in unified physics, which are now gaining worldwide recognition and acceptance.
Learn more about his work in the Resonance Academy with a free comprehensive, self-paced online multimedia Unified Science Course packed with 30 years of research designed to provide a foundation of understanding of the field of Unified Physics and its implications and applications. People from over 80 different countries are engaging with each ...
published: 15 Sep 2016
5:13
Highlights From SDO's 10 Years of Solar Observation
In February 2020, NASA’s Solar Dynamics Observatory — SDO — is celebrating its 10th year in space. Over the past decade the spacecraft has kept a constant eye o...
In February 2020, NASA’s Solar Dynamics Observatory — SDO — is celebrating its 10th year in space. Over the past decade the spacecraft has kept a constant eye on the Sun, studying how the Sun creates solar activity and drives space weather — the dynamic conditions in space that impact the entire solar system, including Earth.
Since its launch on Feb. 11, 2010, SDO has collected millions of scientific images of our nearest star, giving scientists new insights into its workings. SDO’s measurements of the Sun — from the interior to the atmosphere, magnetic field, and energy output — have greatly contributed to our understanding of our closest star. SDO’s images have also become iconic — if you’ve ever seen a close-up of activity on the Sun, it was likely from an SDO image.
Read more: https://www.nasa.gov/feature/goddard/2020/ten-things-we-ve-learned-about-the-sun-from-nasa-s-sdo-this-decade
Music: “Unseen Husband“ from Universal Production Music
Credit: NASA's Goddard Space Flight Center
Scott Wiessinger (USRA): Lead Producer
Mara Johnson-Groh (Wyle Information Systems): Science Writer
Barb Mattson (University of Maryland College Park): Narrator
This video is public domain and along with other supporting visualizations can be downloaded from NASA Goddard's Scientific Visualization Studio at: https://svs.gsfc.nasa.gov/13524
If you liked this video, subscribe to the NASA Goddard YouTube channel: https://www.youtube.com/NASAGoddard
Follow NASA’s Goddard Space Flight Center
· Instagram http://www.instagram.com/nasagoddard · Twitter http://twitter.com/NASAGoddard
· Twitter http://twitter.com/NASAGoddardPix
· Facebook: http://www.facebook.com/NASAGoddard · Flickr http://www.flickr.com/photos/gsfc
https://wn.com/Highlights_From_Sdo's_10_Years_Of_Solar_Observation
In February 2020, NASA’s Solar Dynamics Observatory — SDO — is celebrating its 10th year in space. Over the past decade the spacecraft has kept a constant eye on the Sun, studying how the Sun creates solar activity and drives space weather — the dynamic conditions in space that impact the entire solar system, including Earth.
Since its launch on Feb. 11, 2010, SDO has collected millions of scientific images of our nearest star, giving scientists new insights into its workings. SDO’s measurements of the Sun — from the interior to the atmosphere, magnetic field, and energy output — have greatly contributed to our understanding of our closest star. SDO’s images have also become iconic — if you’ve ever seen a close-up of activity on the Sun, it was likely from an SDO image.
Read more: https://www.nasa.gov/feature/goddard/2020/ten-things-we-ve-learned-about-the-sun-from-nasa-s-sdo-this-decade
Music: “Unseen Husband“ from Universal Production Music
Credit: NASA's Goddard Space Flight Center
Scott Wiessinger (USRA): Lead Producer
Mara Johnson-Groh (Wyle Information Systems): Science Writer
Barb Mattson (University of Maryland College Park): Narrator
This video is public domain and along with other supporting visualizations can be downloaded from NASA Goddard's Scientific Visualization Studio at: https://svs.gsfc.nasa.gov/13524
If you liked this video, subscribe to the NASA Goddard YouTube channel: https://www.youtube.com/NASAGoddard
Follow NASA’s Goddard Space Flight Center
· Instagram http://www.instagram.com/nasagoddard · Twitter http://twitter.com/NASAGoddard
· Twitter http://twitter.com/NASAGoddardPix
· Facebook: http://www.facebook.com/NASAGoddard · Flickr http://www.flickr.com/photos/gsfc
- published: 11 Feb 2020
- views: 469341
2:27
The Dynamic Solar Magnetic Field
While the sun is well known as the overwhelming source of visible light in our solar system, a substantial part of its influence is driven by some aspects less ...
While the sun is well known as the overwhelming source of visible light in our solar system, a substantial part of its influence is driven by some aspects less visible to human perception - the magnetic field.
In this visualization, the sphere represents the solar photosphere, with neutral grey indicating a magnetic field of near zero intensity, black representing a magnetic field pointing INTO the sun (south or negative polarity) and white representing a magnetic field pointing OUT of the sun (north or positive polarity). We see that these magnetic regions often appear in nearby pairs of opposite polarities - which in visible light would often correspond to a pair of sunspots.
Using this measured magnetic field on the photosphere, combined with mathematical models based on Maxwell's equations and plasma physics, we can construct how the magnetic field would look above the photosphere. Here, the white magnetic field lines are considered 'closed'. They move up, and then return to the solar surface. We often see these closed lines associated with pairs of active regions on the sun. The green and violet lines represent field lines that are considered 'open'. Green represents positive magnetic polarity, and violet represents negative polarity. These field lines do not connect back to the sun but with more distant magnetic fields in space.
Here we build one of the simpler magnetic field models, called Potential Field Source Surface or PFSS, to construct how the magnetic 'lines of force' might look above the sun. The PFSS model represents the simplest and most steady magnetic field possible, though here we sample the field each day to illustrate the slow changes of the magnetic structure over time, in this case between January 1, 2011 through December 30, 2014.
Visualizer: Tom Bridgman (lead)
For more information or to download this public domain video, go to https://svs.gsfc.nasa.gov/4391#23751
https://wn.com/The_Dynamic_Solar_Magnetic_Field
While the sun is well known as the overwhelming source of visible light in our solar system, a substantial part of its influence is driven by some aspects less visible to human perception - the magnetic field.
In this visualization, the sphere represents the solar photosphere, with neutral grey indicating a magnetic field of near zero intensity, black representing a magnetic field pointing INTO the sun (south or negative polarity) and white representing a magnetic field pointing OUT of the sun (north or positive polarity). We see that these magnetic regions often appear in nearby pairs of opposite polarities - which in visible light would often correspond to a pair of sunspots.
Using this measured magnetic field on the photosphere, combined with mathematical models based on Maxwell's equations and plasma physics, we can construct how the magnetic field would look above the photosphere. Here, the white magnetic field lines are considered 'closed'. They move up, and then return to the solar surface. We often see these closed lines associated with pairs of active regions on the sun. The green and violet lines represent field lines that are considered 'open'. Green represents positive magnetic polarity, and violet represents negative polarity. These field lines do not connect back to the sun but with more distant magnetic fields in space.
Here we build one of the simpler magnetic field models, called Potential Field Source Surface or PFSS, to construct how the magnetic 'lines of force' might look above the sun. The PFSS model represents the simplest and most steady magnetic field possible, though here we sample the field each day to illustrate the slow changes of the magnetic structure over time, in this case between January 1, 2011 through December 30, 2014.
Visualizer: Tom Bridgman (lead)
For more information or to download this public domain video, go to https://svs.gsfc.nasa.gov/4391#23751
- published: 06 Feb 2018
- views: 27006
3:43
The Dynamic Solar Magnetic Field with Introduction
While the sun is well known as the overwhelming source of visible light in our solar system, a substantial part of its influence is driven by some aspects less ...
While the sun is well known as the overwhelming source of visible light in our solar system, a substantial part of its influence is driven by some aspects less visible to human perception - the magnetic field.
In this visualization we start a view of the Sun in visible light (similiar to what you would see from the ground on Earth), to a view in extreme ultraviolet wavelengths (only visible to space-based instruments) which shows hot plasma streaming along magnetic field lines, to a magnetogram (derived from the visible light data) and finally to a three-dimensional magnetic field model built from that data. The sphere represents the solar photosphere, with neutral grey indicating a magnetic field of near zero intensity, black representing a magnetic field pointing INTO the sun (south or negative polarity) and white representing a magnetic field pointing OUT of the sun (north or positive polarity). We see that these magnetic regions often appear in nearby pairs of opposite polarities - which in visible light would often correspond to a pair of sunspots.
Most of the solar photosphere has a magnetic field intensity of a few gauss while the active regions which form around sunspots can have magnetic fields of a few thousand gauss. Modern space-based instruments such as HMI (Helioseismic and Magnetic Imager) on the Solar Dynamics Observatory (SDO) enable us to measure the intensity of the magnetic field at the visible surface of the sun.
Using this measured magnetic field on the photosphere, combined with mathematical models based on Maxwell's equations and plasma physics, we can construct how the magnetic field would look above the photosphere. Here, the white magnetic field lines are considered 'closed'. They move up, and then return to the solar surface. We often see these closed lines associated with pairs of active regions on the sun. The green and violet lines represent field lines that are considered 'open'. Green represents positive magnetic polarity, and violet represents negative polarity. These field lines do not connect back to the sun but with more distant magnetic fields in space.
Here we build one of the simpler magnetic field models, called Potential Field Source Surface or PFSS, to construct how the magnetic 'lines of force' might look above the sun. The PFSS model represents the simplest and most steady magnetic field possible, though here we sample the field each day to illustrate the slow changes of the magnetic structure over time, in this case between January 1, 2011 through December 30, 2014.
Visualizer: Tom Bridgman (lead)
For more information or to download this public domain video, go to https://svs.gsfc.nasa.gov/4623#24684
https://wn.com/The_Dynamic_Solar_Magnetic_Field_With_Introduction
While the sun is well known as the overwhelming source of visible light in our solar system, a substantial part of its influence is driven by some aspects less visible to human perception - the magnetic field.
In this visualization we start a view of the Sun in visible light (similiar to what you would see from the ground on Earth), to a view in extreme ultraviolet wavelengths (only visible to space-based instruments) which shows hot plasma streaming along magnetic field lines, to a magnetogram (derived from the visible light data) and finally to a three-dimensional magnetic field model built from that data. The sphere represents the solar photosphere, with neutral grey indicating a magnetic field of near zero intensity, black representing a magnetic field pointing INTO the sun (south or negative polarity) and white representing a magnetic field pointing OUT of the sun (north or positive polarity). We see that these magnetic regions often appear in nearby pairs of opposite polarities - which in visible light would often correspond to a pair of sunspots.
Most of the solar photosphere has a magnetic field intensity of a few gauss while the active regions which form around sunspots can have magnetic fields of a few thousand gauss. Modern space-based instruments such as HMI (Helioseismic and Magnetic Imager) on the Solar Dynamics Observatory (SDO) enable us to measure the intensity of the magnetic field at the visible surface of the sun.
Using this measured magnetic field on the photosphere, combined with mathematical models based on Maxwell's equations and plasma physics, we can construct how the magnetic field would look above the photosphere. Here, the white magnetic field lines are considered 'closed'. They move up, and then return to the solar surface. We often see these closed lines associated with pairs of active regions on the sun. The green and violet lines represent field lines that are considered 'open'. Green represents positive magnetic polarity, and violet represents negative polarity. These field lines do not connect back to the sun but with more distant magnetic fields in space.
Here we build one of the simpler magnetic field models, called Potential Field Source Surface or PFSS, to construct how the magnetic 'lines of force' might look above the sun. The PFSS model represents the simplest and most steady magnetic field possible, though here we sample the field each day to illustrate the slow changes of the magnetic structure over time, in this case between January 1, 2011 through December 30, 2014.
Visualizer: Tom Bridgman (lead)
For more information or to download this public domain video, go to https://svs.gsfc.nasa.gov/4623#24684
- published: 12 Mar 2018
- views: 31407
1:08
Space Solar Power Demonstrator
An animated look at Caltech's Space Solar Power Demonstrator.
More info: https://www.caltech.edu/about/news/caltech-to-launch-space-solar-power-technology-demo...
An animated look at Caltech's Space Solar Power Demonstrator.
More info: https://www.caltech.edu/about/news/caltech-to-launch-space-solar-power-technology-demo-into-orbit-in-january
https://wn.com/Space_Solar_Power_Demonstrator
An animated look at Caltech's Space Solar Power Demonstrator.
More info: https://www.caltech.edu/about/news/caltech-to-launch-space-solar-power-technology-demo-into-orbit-in-january
- published: 03 Jan 2023
- views: 54077
0:06
Having a Solar Blast - Zoom
The Sun unleashed an M-2 (medium-sized) solar flare with a spectacular coronal mass ejection (CME) on June 7, 2011. The large cloud of particles mushroomed up ...
The Sun unleashed an M-2 (medium-sized) solar flare with a spectacular coronal mass ejection (CME) on June 7, 2011. The large cloud of particles mushroomed up and fell back down looking as if it covered an area of almost half the solar surface. The Solar Dynamic Observatory (SDO) observed the flare's peak at 1:41 AM ET. SDO recorded these images in extreme ultraviolet light that show a very large eruption of cool gas.
https://wn.com/Having_A_Solar_Blast_Zoom
The Sun unleashed an M-2 (medium-sized) solar flare with a spectacular coronal mass ejection (CME) on June 7, 2011. The large cloud of particles mushroomed up and fell back down looking as if it covered an area of almost half the solar surface. The Solar Dynamic Observatory (SDO) observed the flare's peak at 1:41 AM ET. SDO recorded these images in extreme ultraviolet light that show a very large eruption of cool gas.
- published: 20 May 2013
- views: 244456
1:51
How the Solar System really moves (Update!)
Dear World,
Before I switch to the first spoken videos of 2021, here an update to the animation of the real movement of the Solar System. A lot of you liked the...
Dear World,
Before I switch to the first spoken videos of 2021, here an update to the animation of the real movement of the Solar System. A lot of you liked the moving part of the last one but found it too short. Here a longer, more elaborate version, straight to the point.
Hope you like it.
If you like my content, please consider joining my supporters on Patreon
to get some background info and other goodies:
Starts with 1$ :)
----------------------------------------------------------------
https://www.patreon.com/morn1415/
----------------------------------------------------------------
Other social Media:
https://twitter.com/morn1415
https://www.facebook.com/morn1415/
https://www.instagram.com/morn1415/
Music:
"Sunset" by "O M II N" is licensed under a Creative Commons Licence.
http://bit.ly/2bd8gd2
https://youtu.be/POJYbY5vSrU
Outro Music:
"Bush Week" by "Nihilore"
is licensed under a Creative Commons Licence
http://bit.ly/CCMusicLicense
https://soundcloud.com/nihilore/bush-week
https://youtu.be/dE0f8AqLtLI
https://wn.com/How_The_Solar_System_Really_Moves_(Update_)
Dear World,
Before I switch to the first spoken videos of 2021, here an update to the animation of the real movement of the Solar System. A lot of you liked the moving part of the last one but found it too short. Here a longer, more elaborate version, straight to the point.
Hope you like it.
If you like my content, please consider joining my supporters on Patreon
to get some background info and other goodies:
Starts with 1$ :)
----------------------------------------------------------------
https://www.patreon.com/morn1415/
----------------------------------------------------------------
Other social Media:
https://twitter.com/morn1415
https://www.facebook.com/morn1415/
https://www.instagram.com/morn1415/
Music:
"Sunset" by "O M II N" is licensed under a Creative Commons Licence.
http://bit.ly/2bd8gd2
https://youtu.be/POJYbY5vSrU
Outro Music:
"Bush Week" by "Nihilore"
is licensed under a Creative Commons Licence
http://bit.ly/CCMusicLicense
https://soundcloud.com/nihilore/bush-week
https://youtu.be/dE0f8AqLtLI
- published: 10 Mar 2021
- views: 428568
2:55
Solar Dynamics Observatory - Multi-filter View
The Solar Dynamics Observatory (SDO), using 10 filters, sees connections in the solar atmosphere. This visualization experiment illustrates a mechanism for hig...
The Solar Dynamics Observatory (SDO), using 10 filters, sees connections in the solar atmosphere. This visualization experiment illustrates a mechanism for highlighting these connections.
The movie opens with a full-disk view of the Sun in visible wavelengths (SDO/HMI's 617.3 nm optical light). Then the filters of SDO/AIA are applied to small pie-shaped wedges of the Sun, starting with 170 nm (pink), then 160 nm (green), 33.5 nm (blue), 30.4 nm (orange), 21.1 nm (violet), 19.3 nm (bronze), 17.1 nm (gold), 13.1 nm (aqua) and 9.4 nm (green).
We've locked the camera to rotate the view of the Sun so each wedge-shaped wavelength filter passes over a region of the Sun. As the features pass from one wavelength to the next, we can see dramatic differences in solar structures that appear in different wavelengths.
- Filaments extending off the limb of the Sun which are bright in 30.4 nanometers, appear dark in many other wavelengths.
- Sunspots which appear dark in optical wavelengths, are festooned with glowing ribbons in ultraviolet wavelengths.
- Small flares, invisible in optical wavelengths, are bright ribbons in ultraviolet wavelengths.
- If we compare the visible light limb of the Sun with the 170 nm filter on the left, with the visible light limb and the 9.4 nm filter on the right, we see that the 'edge' is at different heights. This effect is due to the different amounts of absorption, and emission, of the solar atmosphere in ultraviolet light.
- In far ultraviolet light, the photosphere is dark since the black-body spectrum at a temperature of 5700 Kelvin emits very little light in this wavelength.
Visualizer: Tom Bridgman (lead)
For more information or to download this public domain video, go to https://svs.gsfc.nasa.gov/4117#16876.
https://wn.com/Solar_Dynamics_Observatory_Multi_Filter_View
The Solar Dynamics Observatory (SDO), using 10 filters, sees connections in the solar atmosphere. This visualization experiment illustrates a mechanism for highlighting these connections.
The movie opens with a full-disk view of the Sun in visible wavelengths (SDO/HMI's 617.3 nm optical light). Then the filters of SDO/AIA are applied to small pie-shaped wedges of the Sun, starting with 170 nm (pink), then 160 nm (green), 33.5 nm (blue), 30.4 nm (orange), 21.1 nm (violet), 19.3 nm (bronze), 17.1 nm (gold), 13.1 nm (aqua) and 9.4 nm (green).
We've locked the camera to rotate the view of the Sun so each wedge-shaped wavelength filter passes over a region of the Sun. As the features pass from one wavelength to the next, we can see dramatic differences in solar structures that appear in different wavelengths.
- Filaments extending off the limb of the Sun which are bright in 30.4 nanometers, appear dark in many other wavelengths.
- Sunspots which appear dark in optical wavelengths, are festooned with glowing ribbons in ultraviolet wavelengths.
- Small flares, invisible in optical wavelengths, are bright ribbons in ultraviolet wavelengths.
- If we compare the visible light limb of the Sun with the 170 nm filter on the left, with the visible light limb and the 9.4 nm filter on the right, we see that the 'edge' is at different heights. This effect is due to the different amounts of absorption, and emission, of the solar atmosphere in ultraviolet light.
- In far ultraviolet light, the photosphere is dark since the black-body spectrum at a temperature of 5700 Kelvin emits very little light in this wavelength.
Visualizer: Tom Bridgman (lead)
For more information or to download this public domain video, go to https://svs.gsfc.nasa.gov/4117#16876.
- published: 11 Dec 2016
- views: 5976
1:11:36
The Solar Dynamics Observatory: The Sun Up Close and Personal
The first lecture in the 2011 Exploring Space Lecture Series featured Dean Pesnell, Project Scientist for the Solar Dynamics Observatory (SDO). SDO is designed ...
The first lecture in the 2011 Exploring Space Lecture Series featured Dean Pesnell, Project Scientist for the Solar Dynamics Observatory (SDO). SDO is designed to help us better understand how the Sun works and how it influences our lives. From the very start of its mission, SDO revealed incredible views of erupting prominences and flares with amazing clarity. Learn how SDO will change how we see the Sun inside and out!
Presented as a live webcast on Thursday, March 24, 2011 at 8pm ET at the National Air and Space Museum in Washington, DC.
For more information about past & future Exploring Space Lectures, visit http://airandspace.si.edu/exploringspace
https://wn.com/The_Solar_Dynamics_Observatory_The_Sun_Up_Close_And_Personal
The first lecture in the 2011 Exploring Space Lecture Series featured Dean Pesnell, Project Scientist for the Solar Dynamics Observatory (SDO). SDO is designed to help us better understand how the Sun works and how it influences our lives. From the very start of its mission, SDO revealed incredible views of erupting prominences and flares with amazing clarity. Learn how SDO will change how we see the Sun inside and out!
Presented as a live webcast on Thursday, March 24, 2011 at 8pm ET at the National Air and Space Museum in Washington, DC.
For more information about past & future Exploring Space Lectures, visit http://airandspace.si.edu/exploringspace
- published: 30 Mar 2011
- views: 26750
1:13
Adaptive Facade | Solar Shading + Light Modulation
Adaptive facade is a second skin that adapts to the environment to minimize heat gain on a highrise residential building in Vancouver, BC.
Designed in Spring...
Adaptive facade is a second skin that adapts to the environment to minimize heat gain on a highrise residential building in Vancouver, BC.
Designed in Spring 2015 by students at the University of Oregon and the collaboration of faculty at Emily Carr University in Vancouver, BC.
Designed by:
Cody Tucker
Tristan Magnuson
Joe Hudec
Casey Williams
Special thanks to:
Thomas Groppi
Stephen Duff
Turner Exhibits
Jeremy Kramp
Emily Carr University of Art + Design
https://wn.com/Adaptive_Facade_|_Solar_Shading_Light_Modulation
Adaptive facade is a second skin that adapts to the environment to minimize heat gain on a highrise residential building in Vancouver, BC.
Designed in Spring 2015 by students at the University of Oregon and the collaboration of faculty at Emily Carr University in Vancouver, BC.
Designed by:
Cody Tucker
Tristan Magnuson
Joe Hudec
Casey Williams
Special thanks to:
Thomas Groppi
Stephen Duff
Turner Exhibits
Jeremy Kramp
Emily Carr University of Art + Design
- published: 12 Jun 2015
- views: 20183
11:07
Nassim Haramein: Solar system dynamic, DNA imprinting information, Memory, Healing
Nassim Haramein presenting at COGNOS FEST in Barcelona, Spain
Nassim Haramein has spent more than 30 years researching and discovering connections in physics, ...
Nassim Haramein presenting at COGNOS FEST in Barcelona, Spain
Nassim Haramein has spent more than 30 years researching and discovering connections in physics, mathematics, geometry, cosmology, quantum mechanics, biology and chemistry as well as anthropology and archeology.
These studies led Haramein to groundbreaking theories, published papers and patented inventions in unified physics, which are now gaining worldwide recognition and acceptance.
Learn more about his work in the Resonance Academy with a free comprehensive, self-paced online multimedia Unified Science Course packed with 30 years of research designed to provide a foundation of understanding of the field of Unified Physics and its implications and applications. People from over 80 different countries are engaging with each other and a progressive faculty team in a co-creative thriving learning community, participating in live monthly hang-outs with Nassim Haramein & the Resonance Science Foundation faculty, 24-hour live discussion boards, 7 in-depth educational modules, extensive source reference materials and monthly live group video interactions with a community of like-minds. : https://www.resonancescience.org/academy
Support the Resonance Science Foundation's mission of unifying science by being a Contributing Member (just 5/month) : https://www.resonancescience.org/contributing-membership-program
RSF Contributing Members gain access to:
• The first session of every Resonance Academy Elective Course (!)
• Ask direct questions live on monthly "Live with Nassim" calls
• Ask direct questions live on monthly Faculty Q&A calls
• Two Breakout Groups per month where you get to
connect with other members
• Extensive video archive of "Live with Nassim" & Faculty Q&A calls
• Access to a member-only Community Forum
• Access to a member-only Facebook group
• "The Connected Universe" feature film
• "Crossing The Event Horizon" extended documentary film by Nassim Haramein
More member content is added monthly.
https://wn.com/Nassim_Haramein_Solar_System_Dynamic,_Dna_Imprinting_Information,_Memory,_Healing
Nassim Haramein presenting at COGNOS FEST in Barcelona, Spain
Nassim Haramein has spent more than 30 years researching and discovering connections in physics, mathematics, geometry, cosmology, quantum mechanics, biology and chemistry as well as anthropology and archeology.
These studies led Haramein to groundbreaking theories, published papers and patented inventions in unified physics, which are now gaining worldwide recognition and acceptance.
Learn more about his work in the Resonance Academy with a free comprehensive, self-paced online multimedia Unified Science Course packed with 30 years of research designed to provide a foundation of understanding of the field of Unified Physics and its implications and applications. People from over 80 different countries are engaging with each other and a progressive faculty team in a co-creative thriving learning community, participating in live monthly hang-outs with Nassim Haramein & the Resonance Science Foundation faculty, 24-hour live discussion boards, 7 in-depth educational modules, extensive source reference materials and monthly live group video interactions with a community of like-minds. : https://www.resonancescience.org/academy
Support the Resonance Science Foundation's mission of unifying science by being a Contributing Member (just 5/month) : https://www.resonancescience.org/contributing-membership-program
RSF Contributing Members gain access to:
• The first session of every Resonance Academy Elective Course (!)
• Ask direct questions live on monthly "Live with Nassim" calls
• Ask direct questions live on monthly Faculty Q&A calls
• Two Breakout Groups per month where you get to
connect with other members
• Extensive video archive of "Live with Nassim" & Faculty Q&A calls
• Access to a member-only Community Forum
• Access to a member-only Facebook group
• "The Connected Universe" feature film
• "Crossing The Event Horizon" extended documentary film by Nassim Haramein
More member content is added monthly.
- published: 15 Sep 2016
- views: 6278