Photosphere
The photosphere is the visible surface of the Sun, which appears as granules (the tops of convection cells). The "supergranules" are a pattern into which the granules may be clumped, and can be considered either structurally part of the photosphere or part of the convection zone that lies directly beneath it. Some sources extend the term "supergranulation" to include both the photosphere and the chromosphere (which does not, however, use convection).
The granules in the photosphere are convection cells that transport heat from the interior of the Sun to its surface. They appear as bright areas surrounded by darker lanes and are typically about 1,000 kilometers in diameter. Granules are constantly forming, evolving, and disappearing as part of the Sun's dynamic atmosphere.
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The surface of the sun, known as the photosphere, has an average temperature of about 5,500 degrees Celsius and is covered in granules caused by convection currents. It also exhibits features like sunspots, faculae, and solar flares.
On the surface of the Sun, or its photosphere, you can find sunspots and granules. Sunspots are cooler, darker areas caused by magnetic activity, while granules are small, bright features resulting from convection currents in the Sun's plasma. Both phenomena contribute to the dynamic and ever-changing appearance of the Sun's surface.
Granules and supergranules are both structures found on the surface of the Sun, primarily related to solar convection. They are formed by the convective motions of plasma in the Sun's outer layer, with granules being smaller, typically about 1,000 kilometers in diameter, while supergranules are larger, measuring around 30,000 kilometers across. Both exhibit similar patterns of rising and sinking material, contributing to the dynamics of solar activity and influencing solar phenomena. Their study helps scientists understand solar processes and the Sun's overall behavior.
The photosphere is the visible surface of the Sun, which appears as granules (the tops of convection cells). The "supergranules" are a pattern into which the granules may be clumped, and can be considered either structurally part of the photosphere or part of the convection zone that lies directly beneath it. Some sources extend the term "supergranulation" to include both the photosphere and the chromosphere (which does not, however, use convection).
The granules in the photosphere are convection cells that transport heat from the interior of the Sun to its surface. They appear as bright areas surrounded by darker lanes and are typically about 1,000 kilometers in diameter. Granules are constantly forming, evolving, and disappearing as part of the Sun's dynamic atmosphere.
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The surface of the sun, known as the photosphere, has an average temperature of about 5,500 degrees Celsius and is covered in granules caused by convection currents. It also exhibits features like sunspots, faculae, and solar flares.
Granules are small convective cells on the Sun's surface caused by rising hot gas and sinking cool gas. Spicules are small jets of gas that shoot upward from the Sun's surface. Together, these features create the granulated texture seen on the Sun's surface.
Because it covered 25% of the world and was so widespread that the sun was always shining on some part of it.
On the surface of the Sun, or its photosphere, you can find sunspots and granules. Sunspots are cooler, darker areas caused by magnetic activity, while granules are small, bright features resulting from convection currents in the Sun's plasma. Both phenomena contribute to the dynamic and ever-changing appearance of the Sun's surface.
Those are called granules. Granules are small convection cells on the surface of the sun, caused by hot gas rising and cooler gas sinking. They are typically about 1000 kilometers in diameter and last for about 5 to 10 minutes.
The grainieness is caused by convective cells at the sun's sufrace. Hooter material rises up at the centers of these "grains" (called granules) while less hot material sinks around their edges. Each granule is several hundred miles across.
A Partial Solar Eclipse will happen most often because it is more likely for part of the sun to be covered up by the moon than the whole moon covering the entire sun.A Partial Solar Which_occurs_more_often_a_partial_solar_eclipse_or_a_total_solar_eclipsewill happen most often because it is more likely for part of the sun to be covered up by the moon than the whole moon covering the entire sun. Also you don't really hear about Total Eclipses do you ?Hope I HelpedRead more: Which_occurs_more_often_a_partial_solar_eclipse_or_a_total_solar_eclipseA Partial Solar Which_occurs_more_often_a_partial_solar_eclipse_or_a_total_solar_eclipsewill happen most often because it is more likely for part of the sun to be covered up by the moon than the whole moon covering the entire sun. Also you don't really hear about Total Eclipses do you ?Hope I HelpedRead more: Which_occurs_more_often_a_partial_solar_eclipse_or_a_total_solar_eclipseA Partial Solar Which_occurs_more_often_a_partial_solar_eclipse_or_a_total_solar_eclipsewill happen most often because it is more likely for part of the sun to be covered up by the moon than the whole moon covering the entire sun. Also you don't really hear about Total Eclipses do you ?Hope I HelpedRead more: Which_occurs_more_often_a_partial_solar_eclipse_or_a_total_solar_eclipsePartial Solar Eclipse will happen most often because it is more likely for part of the sun to be covered up by the moon than the whole moon covering the entire sun. Also you don't really hear about A Partial Solar Eclipse will happen most often because it is more likely for part of the sun to be covered up by the moon than the whole moon covering the entire sun. Also you don't really hear about
The bright markings are "faculae" (plural of facula). However, I wouldn't say that they produce the grainy texture. I think the "granulation" is there even without the faculae.