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Solar Corona (Cig Card)

Solar Corona (Cig Card)


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Solar Corona (Cig Card)

SOLAR CORONA

Mary Evans Picture Library makes available wonderful images created for people to enjoy over the centuries

Media ID 600520

© Mary Evans Picture Library 2015 - https://copyrighthub.org/s0/hub1/creation/maryevans/MaryEvansPictureID/10138167

Corona Phenomena Solar Space 1928 Parhelia


EDITORS COMMENTS
This image captures the Solar Corona, the outermost layer of the Sun's atmosphere, as it appeared in 1928. The Solar Corona is a natural phenomenon that is not directly visible to the naked eye due to the Sun's intense brightness. However, during a total solar eclipse, the Corona can be observed as a halo of light surrounding the darkened disc of the Sun. This photograph, a Cig Card from the Mary Evans Picture Library, is a historical record of the Solar Corona's intricate and dynamic structure. The Corona is not a static feature; it is constantly in motion, with solar winds and solar flares releasing energy and particles that can impact the Earth's magnetic field and weather. The Solar Corona is composed of plasma, which is ionized gas that is heated to millions of degrees Celsius. The bright areas in this image are called solar prominences, where magnetic fields rise and form loops of plasma. The darker areas are sunspots, which are cooler regions on the Sun's surface. Parhelia, or sun dogs, are also visible in this image. They are caused by the refraction of sunlight by ice crystals in the Earth's atmosphere. The Solar Corona and parhelia combine to create a breathtaking display of natural phenomena, a reminder of the wonders of the universe that lie beyond our planet. This photograph is a testament to the advances in solar physics and astronomical observation over the last century. It invites us to marvel at the beauty and complexity of the Sun and the Solar System, and to continue exploring the mysteries of space.

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