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NASA / Sun / Full Disk / Poster
NASA / Sun / Full Disk / Poster
Full Disk Image of the Sun,This image was taken by the SECCHI Extreme UltraViolet Imager (EUVI) mounted on the STEREO-B spacecraft. STEREO-B is located behind the Earth, and follows the Earth in orbit around the Sun. This location enables us to view the Sun from the position of a virtual left eye in space. NASA's Solar TErrestrial RElations Observatory (STEREO) satellites have provided the first three-dimensional images of the Sun. For the first time, scientists will be able to see structures in the Sun's atmosphere in three dimensions. The new view will greatly aid scientists' ability to understand solar physics and thereby improve space weather forecasting. The EUVI imager is sensitive to wavelengths of light in the extreme ultraviolet portion of the spectrum. EUVI bands at wavelengths of 304, 171 and 195 Angstroms have been mapped to the red blue and green visible portion of the spectrum; and processed to emphasize the temperature difference of the solar material. The structure of the corona shows well in this image.Is a satellite of: Mission: Solar TErrestrial RElations Observatory (STEREO) Spacecraft: Solar TErrestrial RElations Observatory (STEREO) Instrument: SECCHI/Extreme Ultraviolet Imaging Telescope Product Size: 1920 x 1080 pixels (width x height) Produced By: JPL Full-Res TIFF: PIA09320.tif (6.23 MB) Full-Res JPEG: PIA09320.jpg (110.4 kB)
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NASA / Sun / Full Disk / Poster
Full Disk Image of the Sun,This image was taken by the SECCHI Extreme UltraViolet Imager (EUVI) mounted on the STEREO-B spacecraft. STEREO-B is located behind the Earth, and follows the Earth in orbit around the Sun. This location enables us to view the Sun from the position of a virtual left eye in space. NASA's Solar TErrestrial RElations Observatory (STEREO) satellites have provided the first three-dimensional images of the Sun. For the first time, scientists will be able to see structures in the Sun's atmosphere in three dimensions. The new view will greatly aid scientists' ability to understand solar physics and thereby improve space weather forecasting. The EUVI imager is sensitive to wavelengths of light in the extreme ultraviolet portion of the spectrum. EUVI bands at wavelengths of 304, 171 and 195 Angstroms have been mapped to the red blue and green visible portion of the spectrum; and processed to emphasize the temperature difference of the solar material. The structure of the corona shows well in this image.Is a satellite of: Mission: Solar TErrestrial RElations Observatory (STEREO) Spacecraft: Solar TErrestrial RElations Observatory (STEREO) Instrument: SECCHI/Extreme Ultraviolet Imaging Telescope Product Size: 1920 x 1080 pixels (width x height) Produced By: JPL Full-Res TIFF: PIA09320.tif (6.23 MB) Full-Res JPEG: PIA09320.jpg (110.4 kB)
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Product ID: 228591721120101424
Made on: 8/16/2012 6:28 AM