Kaleidoscopic View of the Sun Reveals its Hidden Features

By Tom Yulsman | December 20, 2013 1:08 pm
Kaleidoscopic view of the Sun Solar Dynamics Observatory SDO

A screenshot of a movie of the sun from NASA’s Solar Dynamics Observatory. The pie-shaped slices show the sun in different wavelengths of light that are ordinarily invisible to our eyes. Each highlights different kinds of features on the sun’s surface and in its corona. (Source: NASA Goddard Space Flight Center)

The human visual system is an incredible example of natural engineering that far surpasses the very best cameras and lenses. To offer one example, on a bright day with extremely contrasty light, it can discern fine details in both the dark shadows and bright highlights — details that are all but lost in to a camera.

Even so, what we can see is extremely limited compared to what’s actually out there — a fact that is dramatically illustrated by the kaleidoscopic view of the sun above. It’s a frame from a movie put together by NASA to illustrate the abilities of the Solar Dynamics Observatory, an orbiting satellite that continuously monitors the sun.

SDO’s instruments are sensitive to wavelengths of light that are invisible to us. In the image, above (and the full video below), each pie-shaped slice represents a view of the sun in a particular wavelength. Viewing the sun in different wavelengths allows scientists to discern different kinds of features on its surface and in its atmosphere, called the corona.

Here’s the full video:

Remember that in the video, and the image up top, the coloring is artificial.

Here are a few examples of what the various colored views show:

  • Yellow: Shows light with a wavelength of 5,800 Angstroms emanating from material that’s at about 10,000 degrees F (5700 degrees C). This wavelength highlights features on the surface of the sun.
  • Green: Shows extreme ultraviolet light with a wavelength of 94 Angstroms. This light comes from atoms that are more than a thousand times hotter — at about 11 million degrees F (6,300,000 degrees C). Solar flares, which are extremely hot, show up well in this wavelength.
  • Red: Shows another wavelength of extreme ultraviolet light, at 304 Angstroms. Plasma made of helium II ions, the second most abundant element in the sun’s atmosphere, emit light in this wavelength, which is good for discerning gigantic loops of plasma that align with features of the sun’s magnetic field.

The video below shows a particularly spectacular example of what can be seen when viewing the sun in this latter wavelength. It was captured by SDO on July 19, 2012.

First, a moderately powerful solar flare explodes from the sun. This is followed by an ejection of solar material, a phenomenon that’s known as a coronal mass ejection, or CME. And then the really spectacular fireworks begin:

The massive loops of glowing material are what’s known as coronal rain. This happens as plasma cools and condenses along magnetic field lines.

With the flare and CME, the sun’s magnetic field has bulged outward here. Ordinarily, it can’t be seen. But the glowing plasma acts like a tracer, making it visible. The plasma rains down for almost a full day (which is compressed into about four minutes in the video), until the bulge in the magnetic field dissipates.

Kaleidoscopic view of the Sun full disk SDO

SDO images of the sun seen in different wavelengths.  (Source: NASA/SDO/Goddard Space Flight Center)

Last but not least, a mosaic of solar images showcasing the 13 different wavelengths of light that SDO’s instruments can discern.

Of course you should never look directly at the sun with the naked eye. Doing so could cause irreparable damage to that wonder of natural engineering — your vision. But the next time that you’re out and about on a sunny day, perhaps you can now see —  in your mind’s eye — all the amazing detail and activity that’s ordinarily hidden from us.




ImaGeo is a visual blog focusing on the intersection of imagery, imagination and Earth. It focuses on spectacular visuals related to the science of our planet, with an emphasis (although not an exclusive one) on the unfolding Anthropocene Epoch.

About Tom Yulsman

Tom Yulsman is Director of the Center for Environmental Journalism and a Professor of Journalism at the University of Colorado, Boulder. He also continues to work as a science and environmental journalist with more than 30 years of experience producing content for major publications. His work has appeared in the New York Times, Washington Post, Audubon, Climate Central, Columbia Journalism Review, Discover, Nieman Reports, and many other publications. He has held a variety of editorial positions over the years, including a stint as editor-in-chief of Earth magazine. Yulsman has written one book: Origins: the Quest for Our Cosmic Roots, published by the Institute of Physics in 2003.


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