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Filtered Images

Seen with the human eye, the Sun appears as an intensely bright object in the sky. The light it emits appears to be white although if we shine sunlight through a prism we see a continous rainbow of colors. These colors make up the visible white light of the Sun.

Visible light makes up a very small portion of the electromagnetic spectrum. With special equipment, it's possible to examine the Sun in wavelengths other than visible light. Scientists take "pictures" of the Sun as it appears in infrared, ultraviolet, and even x-ray wavelengths. Obviously, we can't see these non-visible portions of the spectrum. However, sophisticated instruments can detect these wave lengths which are then converted into images we can see. You'll notice the Sun looks different when viewed through the "eyes" of these instruments. Scientists use these different images to better understand the features and the workings of the Sun.

 

x-ray image
Soft x-ray image of the Sun. Taken on September 13, 2001 by the Yohkoh Spacecraft. (Click for a larger image.)
Extreme ultraviolet
Extreme Ultraviolet image of the Sun. Taken on September 13, 2001 by the Extreme ultraviolet Imaging Telescope aboard the SOHO Spacecraft. (Click for a larger image.)
White Light Image
White-light image of the Sun. Taken on September 13, 2001 by the Big Bear Observatory. (Click for a larger image.)
H-alpha image
H-alpha image of the Sun. Taken on September 13, 2001 by the Big Bear Observatory. (Click for a larger image.)
globe icon See today's images of the Sun at the Solar Max 2000 Web site. (Requires an Internet connection)

Related to chapter 2 in the print guide.
Related Materials

For an overview of the Electromagnetic Spectrum, see the Electromagnetic Spectrum Chart.

Glossary Terms

Click for the definitions of the following words that are used on this page: (Definitions appear in a pop-up window.)

extreme ultraviolet
gamma rays
infrared radiation
ultraviolet radiation
white light
x-rays

View the full, printable version of the glossary.

 
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