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Solar Prominence

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24" x 24"
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Photographic Print
24" x 24" Photographic Print
$59.99
$44.99
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Solar prominence. Ultraviolet SOHO (Solar and Heliospheric Observatory) satellite image of a solar prominence (top right). The prominence is erupting from the chromosphere (orange), which lies above the Sun's visible surface, the photosp- here. Prominences are dense clouds of plasma, or ionised gas, in the Sun's outer layer, the corona. They are typically at temperatures of 60,000 Kelvin, much cooler than the several million Kelvin of the corona. Active regions (white) mark areas of high solar activity. The Sun's activity peaks every 10-11 years. Image produced by SOHO's Extreme Ultraviolet Imaging Telescope (EIT) on 14 September 1999, as the Sun approached such a time. This photographic print is digitally printed on archival photographic paper resulting in vivid, pure color and exceptional detail that is suitable for museum or gallery display.

24" x 24" Photographic Print
$59.99
$44.99
Ships in 1-2 days
ADD TO CART

Product Details

Solar prominence. Ultraviolet SOHO (Solar and Heliospheric Observatory) satellite image of a solar prominence (top right). The prominence is erupting from the chromosphere (orange), which lies above the Sun's visible surface, the photosp- here. Prominences are dense clouds of plasma, or ionised gas, in the Sun's outer layer, the corona. They are typically at temperatures of 60,000 Kelvin, much cooler than the several million Kelvin of the corona. Active regions (white) mark areas of high solar activity. The Sun's activity peaks every 10-11 years. Image produced by SOHO's Extreme Ultraviolet Imaging Telescope (EIT) on 14 September 1999, as the Sun approached such a time. This photographic print is digitally printed on archival photographic paper resulting in vivid, pure color and exceptional detail that is suitable for museum or gallery display.

Item# 22109359002A

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Solar prominence. Ultraviolet SOHO (Solar and Heliospheric Observatory) satellite image of a solar prominence (top right). The prominence is erupting from the chromosphere (orange), which lies above the Sun's visible surface, the photosp- here. Prominences are dense clouds of plasma, or ionised gas, in the Sun's outer layer, the corona. They are typically at temperatures of 60,000 Kelvin, much cooler than the several million Kelvin of the corona. Active regions (white) mark areas of high solar activity. The Sun's activity peaks every 10-11 years. Image produced by SOHO's Extreme Ultraviolet Imaging Telescope (EIT) on 14 September 1999, as the Sun approached such a time. This photographic print is digitally printed on archival photographic paper resulting in vivid, pure color and exceptional detail that is suitable for museum or gallery display.

Item# 22109359002A
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Solar Prominence

24" x 24" Photographic Print
$59.99
$44.99
Ships in 1-2 days
ADD TO CART