Solar structure, artwork C017 / 7363
Wall Art and Photo Gifts from Science Photo Library
Solar structure, artwork C017 / 7363
Solar structure. Cutaway computer artwork showing the structure of the Sun. At the Suns core (centre) hydrogen atoms undergo nuclear fusion, producing helium atoms and releasing heat and light energy as photons. These radiate outwards through the inner region (radiative zone, yellow) to the outer convection zone layer (orange). Here, solar plasma rises in thermal columns to the visible surface (photosphere) and falls back to the interior in convection currents (squared lines). Intense magnetic fields on the surface of the Sun inhibit convection in some areas, causing these areas to have lower temperatures than others and causing the appearance of dark spots known as sunspots (lower right)
Science Photo Library features Science and Medical images including photos and illustrations
Media ID 9228975
© CARLOS CLARIVAN/SCIENCE PHOTO LIBRARY
Arrow Arrows Astrophysical Astrophysics Core Coronal Mass Ejection Cosmological Cosmology Current Currents Cutaway Ejecting Ejections Flare Flares Flaring Fusion Internal Layer Layers Loop Loops Photosphere Prominence Prominences Solar Solar System Star Surface Universe Coronal Loops Section Sectioned Sunspot Sunspots
EDITORS COMMENTS
This photo print, titled "Solar Structure" offers a mesmerizing glimpse into the intricate workings of our magnificent Sun. Created by artist Carlos Clarivan, this cutaway computer artwork unveils the hidden layers and processes that occur within our star. At the very core of the Sun, hydrogen atoms undergo nuclear fusion, transforming into helium atoms while releasing an immense amount of heat and light energy in the form of photons. These radiant energies then traverse through the inner region known as the radiative zone, depicted in a vibrant yellow hue. Moving further outwards lies the outer convection zone layer, represented by a striking orange shade. In this awe-inspiring illustration against a black background, we witness solar plasma rising in thermal columns towards the visible surface called photosphere. Simultaneously, it falls back to its interior through convection currents illustrated by squared lines. However, areas with intense magnetic fields inhibit convection and exhibit lower temperatures compared to others – these are what we know as sunspots. Carlos Clarivan's artwork beautifully captures not only these dark spots but also showcases various other celestial phenomena such as flares, loops, prominences, and coronal mass ejections (CMEs). With meticulous detail and precision in every stroke and arrow used throughout this piece; it serves as a stunning reminder of both our place within our solar system and the vast wonders that lie beyond its boundaries.
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