photosphere
Prominences are large, bright features extending outward from the Sun's surface, while solar flares are sudden, intense bursts of energy. The corona is the Sun's outer atmosphere, solar wind is a stream of charged particles flowing from the Sun, chromospheres are the middle layer of the Sun's atmosphere, and photospheres are the Sun's visible surface. Collectively, these components make up the dynamic system of the Sun's structure and activity.
As Pluto moves away from the sun, it would experience a decrease in temperature and sunlight. This could impact its surface features, potentially leading to changes in its atmosphere and surface composition over long periods of time.
Surface of the sun is hotter.
The Sun exhibits several prominent features, including sunspots, which are cooler, darker areas on its surface caused by magnetic activity. Solar flares are intense bursts of radiation resulting from the release of magnetic energy, while prominences are large, loop-like structures of plasma extending outward from the Sun's surface. Additionally, the solar corona, which is the outer atmosphere of the Sun, can be seen during a total solar eclipse, showcasing its intricate structure and temperature variations.
The inner core is hotter then the sun's surface.
Scientists have discovered many features of the sunâ??s surface. Some of these features include a rigid iron surface, sunspots, prominences, and solar flares.
Photosphere- outer (gaseous) layer or surface of sun that we see Faculae- bright areas Sunspots- dark areas
The five surface features of the sun are sunspots, solar flares, prominences, faculae, and granulation. These features are caused by the dynamic processes occurring on the sun's surface due to its magnetic field and internal convective motion.
sunspots prominence solar flares solar winds
Sun spots on. Flares on and above. Solar wind above.
Some features that form on or above the sun's surface include sunspots, solar flares, prominences, and coronal loops. These features are related to the sun's magnetic field and can impact space weather and phenomena like the auroras on Earth.
Some features found on the surface of the sun include sunspots, which are temporary darker spots caused by magnetic activity, solar flares, which are sudden brightening events releasing energy, and prominences, which are huge arcs of gas that erupt from the surface. Additionally, the photosphere, chromosphere, and corona are distinct layers of the sun's atmosphere visible from the surface.
The major surface feature of the Sun is its photosphere, which is the visible surface that emits light and heat. The Sun's atmosphere includes the chromosphere, located just above the photosphere, and the corona, the outermost layer that extends into space. These layers exhibit features such as sunspots, solar flares, and prominences, which are all associated with the Sun's magnetic activity.
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.
Prominences occur in the chromosphere layer of the sun's atmosphere. They are large, bright, gaseous features that extend outward from the sun's surface.
No, there is no black dot in the middle of the Sun. The Sun is a bright, glowing ball of gas and does not have any visible surface features like a black dot.
Solar prominences are large looping structures of hot, glowing gas that extend from the Sun’s surface into the outer atmosphere, or corona. They can be seen during total solar eclipses or with special equipment that blocks out the brightness of the Sun. Prominences are caused by complex magnetic interactions within the Sun.