WHICH LAYER OF THE SUN IS VISIBLE DURING A TOTAL SOLAR ECLIPSE

The setting of the sunlight is composed of several layers, mostly the photospbelow, the chromosphere and also the corona. It"s in these outer layers that the sun"s power, which has bubbled up from the sun"s internal layers, is detected as sunlight.

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The lowest layer of the sun"s setting is the photosphere. It is about 300 miles (500 kilometers) thick. This layer is where the sun"s energy is released as light. Since of the distance from the sunlight to Earth, light reaches our world in around eight minutes.


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Image of the solar corona, taken by the SECCHI outer coronagraph (COR2) on the STEREO Ahead observatory on June 8, 2010 at 01:09:35 UT. Click to enbig. (Image credit: NASA/STEREO)

The photospbelow is noted by bappropriate, bubbling granules of plasma and darker, cooler sunspots, which emerge once the sun"s magnetic area breaks through the surconfront. Sunspots appear to move throughout the sun"s disk. Observing this motion led astronomers to realize that the sunlight rotates on its axis. Due to the fact that the sunlight is a bevery one of gas through no solid develop, various regions rotate at various rates. The sun"s equatorial areas turn in around 24 days, while the polar areas take even more than 30 days to make a complete rotation.


The photospright here is additionally the source of solar flares: tongues of fire that extend hundreds of countless miles over the sun"s surface. Solar flares create bursts of X-rays, ultraviolet radiation, electromagnetic radiation and also radio waves.


The following layer is the chromosphere. The chromospbelow emits a reddish glow as super-heated hydrogen burns off. But the red rim have the right to only be checked out throughout a full solar eclipse. At various other times, light from the chromospright here is typically too weak to be seen versus the brighter photospbelow.


The chromospright here may play a duty in conducting warmth from the internal of the sunlight to its outera lot of layer, the corona. "We check out particular kinds of solar seismic waves channeling upwards into the lower environment, dubbed the chromospbelow, and also from tright here, right into the corona," Junwei Zhao, a solar scientist at Stanford College in Stanford, The golden state, and also lead writer on a recent study that tracked waves from sunspots, said in a statement. "This research gives us a brand-new viewpoint to look at waves that deserve to contribute to the energy of the atmosphere."

The third layer of the sun"s environment is the corona. It have the right to just be viewed throughout a full solar eclipse too. It shows up as white streamers or plumes of ionized gas that flow outward right into room. Temperatures in the sun"s corona deserve to acquire as high as 3.5 million degrees Fahrenheit (2 million levels Celsius). As the gases cool, they become the solar wind.

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Why the corona is up to 300 times hotter than the photospright here, despite being farther from the solar core, has continued to be a irreversible mystery.


"That"s a little of a puzzle," Jeff Brosius, a kosid.org scientist at Catholic College in Washington, D.C., and NASA"s Goddard kosid.org Flight Center in Greenbelt, Maryland also, said in a statement. "Things normally get cooler farther ameans from a warm source. When you"re roasting a marshmallow you move it closer to the fire to prepare it, not farther amethod."

Recent research suggests that tiny explosions well-known as nanoflares may aid push the temperature up by giving sporadic bursts getting to up to 18 million F (10 million C).

"The explosions are referred to as nanoflares bereason they have one-billionth the power of a regular flare," Jim Klimchuk, a solar scientist at NASA"s Goddard kosid.org Flight Center in Maryland also, shelp in a statement. "Despite being tiny by solar standards, each packs the wallop of a 10-megaton hydrogen bomb. Millions of them are going off eexceptionally second across the sun, and jointly they warm the corona."

Giant super-tornados might also play a function in heating the sun"s external layer. These solar twisters are a mix of warm flowing gas and tangled magnetic field lines, inevitably moved by nuclear reactions in the solar core.

"Based on the detected events, we estimate that at leastern 11,000 swirls are present on the sunlight at all times," Sven Wedemeyer-Böhm, a solar scientist of the University of Oslo in Norway and lead writer of the team that identified tornados on the sun, told kosid.org.