Autographs of the sun, 1861-1863

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Largest available format 3504 × 1007 px 1 MB

	Dimension [pixels]	Dimension in 300dpi [mm]	File size [MB]	Online Purchase
Large	3504 × 1007 px	297 × 85 mm	544 KB
Medium	1024 × 295 px	87 × 25 mm	363 KB

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IMAGE number

UIS5087978

Image title

Autographs of the sun, 1861-1863

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photography

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Autographs of the sun, 1861-1863. Parts e, f and g from a booklet containing '10 Autographs of the Sun, taken with the Heliantograph of the Reverend William Selwyn at Ely by John Titterton, photographer'. All three images show areas of sunspot activity. Sunspots are relatively cool areas on the Sun's surface, the photosphere. The number of sunspots is greatest at the point in the cycle of solar activity known as the 'solar maximum', which occurs roughly every 11 years. They form when magnetic field lines below the surface become twisted and protrude through the photosphere. Sunspots are closely associated with solar flares, sudden outbursts of energy which extend far into the Sun's atmosphere. ©SSPL/National Media Museum

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SSPL/UIG / Bridgeman Images

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Largest available format 3504 × 1007 px 1 MB View all formats

	Dimension [pixels]	Dimension in 300dpi [mm]	File size [MB]	Online Purchase
Large	3504 × 1007 px	297 × 85 mm	544 KB
Medium	1024 × 295 px	87 × 25 mm	363 KB

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