what function does the sun's convective zone perform
ef8fe22c273d9060e239a3ed248682e4
How the Sun Works The convective zone, which is the final 30 percent of the sun's radius, is dominated by convection currents that carry the energy outward to the surface. These convection currents are rising movements of hot gas next to falling movements of cool gas, and it looks kind of like glitter in a simmering pot of water.fter covering the core, it's time to extend outward in the sun's structure. Next up are the radiative and convective zones. The radiative zone extends outward from the core, accounting for 45 percent of the sun's radius. In this zone, the energy from the core is carried outward by photons, or light units.
2e74ccb433a1855b4879ea58203b99ad
Solar flare Solar flares affect all layers of the solar atmosphere (photosphere, chromosphere, and corona), when the plasma medium is heated to tens of millions kelvins, while the cosmic-ray-like electrons, protons, and heavier ions are accelerated to near the speed of light.
b05dcfd5acb3dd39a282c3e312a7e6f4
- The Malmedy massacre was a war crime in which 80 American prisoners of war were murdered by their German captors during World War II.The massacre was committed on 17 December 1944, by members of Kampfgruppe Peiper (part of the 1st SS Panzer Division), a German combat unit, during the Battle of the Bulge.2] [3] The route followed by Kampfgruppe Peiper. The crossroads of Baugnez where the Malmedy massacre happened is surrounded by a circle. Hitler 's plans for the Battle of the Bulge gave the main goal (breaking through Allied lines) to the 6th SS Panzer Army, commanded by General Sepp Dietrich.
9a557dea3616d2789d01ec4f53fca546
Earthâs Sun: Facts About the Sunâs Age, Size and History Although it only makes up roughly 2 percent of the sun's volume, it is almost 15 times the density of leadand holds nearly half of the sun's mass. Next is the radiative zone, which extends from the core to 70 percent of the way to the sun's surface, making up 32 percent of the sun's volume and 48 percent of its mass.he solar atmosphere above that consists of the photosphere, chromosphere, a transition region and the corona. Beyond that is the solar wind, an outflow of gas from the corona. The core extends from the sun's center to about a quarter of the way to its surface.
e0cf4a689bbf213d5ae36f50a1fcf9ba
- The convective zone of the sun resides beneath the Photosphere and Chromosphere (the visible surface) and above the radiative zone which surrounds the core. It is within the c … onvective zone that energy is primarily transferred outwards via convection.toms in this zone absorb energy and emit the energy as radiation. In this manner, the energy created in the core is transported through the radiation zone. After the radiation zone, the energy is transported through convection to be released at the surface of sun. 2 people found this useful.
cf12003da30bbc1715d406ac666d2dae
- The sun shines because the fusion reactions taking place there release a tremendous amount of energy. And light, which is electromagnetic energy, is released in great quantiti … es. The brightness of the sun speaks to the amount of power it generates.he sun shines because the fusion reactions taking place there release a tremendous amount of energy. And light, which is electromagnetic energy, is released in great quantiti … es. The brightness of the sun speaks to the amount of power it generates.
9efd159a6a7823dfb5a739a97af2b6a2
The ozone layer and its effect on ultraviolet light The ozone layer and its effect on ultraviolet light. The Earth is surrounded by a thick atmosphere which provides us with the air we beathe, keeps the planet warm and also protects us from harmful radiation from space. One of the most important types of damaging radiation is ultra violet radiation from the Sun. The part of the atmosphere that filters out a lot of the ultra violet radiation is called the ozone layer – a region of the atmosphere between about 15 and 40 km above the Earth's surface. The ultra violet radiation from the Sun is divided into three regions depending on the wavelength of the radiation.
732b795ca9c5b0e202d284144477b4b2
- The Sun is the main source of energy for convection in the atmosphere and the oceans.    The Sun, heat radiated form the Sun is the main source of energy  driving convec…tion in the atmosphere and oceans. There is also a  small input form geothermal energy. ãã¤Leeziitha XD.
ed2e0eac9d27d4dc27b922c5ef049567
Taibon Agordino Taibon Agordino. Taibon Agordino is a comune (municipality) in the province of Belluno in the Italian region of Veneto, located about 100 kilometres (62 mi) north of Venice and about 25 kilometres (16 mi) northwest of Belluno. As of 31 December 2004, it had a population of 1,790 and an area of 90.4 square kilometres (34.9 sq mi).
80c32084e847209bd175da85bb943f25
- 1 The Sun has six layers. 2  The centre of the Sun is its core which produces all the Sun’s energy. 3  Around the core is the radiative zone, which carries the energy out from the core. 4  It takes about 170,000 years for the Sun’s energy to move from the core through the radiative zone to the next layer, the connective zone.
cbba7f49c71e3013a5c406ea127d008d
Sun path Sun path. Solar altitude over a year; latitude on northern hemisphere. Sun path polar chart for any location at the latitude of Rotterdam. Sun path refers to the apparent hourly and seasonal motion of the Sun across the sky (and the length of daylight) as the Earth rotates and orbits the Sun. The relative position of the Sun is a major factor in the heat gain of buildings and in the performance of solar energy systems.
5c1cee61a1dafc92c5fc48857631f213
- Convection Zone Moving from a distance of approximately 200,000 Km (125,000 mi) lies the Convective Zone of the Sun. This zone is not dense enough to use radiative transfer of energy, instead, it uses thermal convection zones, in other words, it boils. Energy is carried through thermal columns to the surface of the sun and creates areas that we see as solar granulation and super granulation.
6d946dd2188052de58ec96cbd8e78521
Temperature of the Sun Temperature of the Sun. The Sun provides all the heat and energy needed in the Earth as well as the entire solar system. It also generates tremendous energy in the form of light and heat.It is this energy which powers the entire solar system.emperature of the Sun. The Sun provides all the heat and energy needed in the Earth as well as the entire solar system. It also generates tremendous energy in the form of light and heat.
f397e45615a3e87051e05ac0aae5618d
Sunlight Sunlight is a portion of the electromagnetic radiation given off by the Sun, in particular infrared, visible, and ultraviolet light.On Earth, sunlight is filtered through Earth's atmosphere, and is obvious as daylight when the Sun is above the horizon.When the direct solar radiation is not blocked by clouds, it is experienced as sunshine, a combination of bright light and radiant heat. Ultraviolet C or (UVC) range, which spans a range of 100 to 280 nm. 2  The term ultraviolet refers to the fact that the radiation is at higher frequency than violet light (and, hence, also invisible to the human eye).
1b057550864e0070d038ac2dc84d0b60
The Sun's Radiative Zone The Sun's radiative zone is the section of the solar interior between the innermost core and the outer convective zone. In the radiative zone, energy generated by nuclear fusion in the core moves outward ...more.any other stars also have radiative zones. The Sun's radiative zone extends from the core outward to about 70% of the Sun's radius. In a smaller (than the Sun) star that is cooler than our Sun, the convective zone tends to be larger, extending deeper into the star's interior.
9e36507edc4d15badf0580a143996f29
Solar Radiation and the Earth's Energy Balance. The energy that drives the climate system comes from the Sun. When the Sun's energy reaches the Earth it is partially absorbed in different parts of the climate system. The absorbed energy is converted back to heat, which causes the Earth to warm up and makes it habitable.
03e694ccdf55e0791690ef5b55fd2e7d
What Lives where? The epipelagic zone. The epipelagic zone (or the sunlight zone) is the only layer of the oceans where photosynthesis takes place. The importance of photosynthesis: photosynthesis is a process of sunlight and carbon dioxide gas converting into oxygen gas and food. Most of the oxygen is created by phytoplankton which are called autotrophs.
aa034c35121eb10648f0827281843ca3
The Sun But for Earth and the other planets that revolve around it, the sun is a powerful center of attention. It holds the solar system together; pours life-giving light, heat, and energy on Earth; and generates space weather.The sun is a big star.ut for Earth and the other planets that revolve around it, the sun is a powerful center of attention. It holds the solar system together; pours life-giving light, heat, and energy on Earth; and generates space weather.
addc599635f57d16f89c5c81d22a312b
- The Sun's radiative zone is the section of the solar interior between the innermost core and the outer convective zone. In the radiative zone, energy generated by nuclear fusi … on in the core moves outward as electromagnetic radiation. In other words, the energy is conveyed by photons.toms in this zone absorb energy and emit the energy as radiation. In this manner, the energy created in the core is transported through the radiation zone. After the radiation zone, the energy is transported through convection to be released at the surface of sun. 2 people found this useful.
13a8a8a9d92d3ee9579c51b883967bd6
What does the photosphere do? The photosphere of the sun is the thin layer from which most of the light produced from the sun is emitted.
cf3ffd92b1de6280c39959a0060546b4
Astronomy The sun and its atmosphere consist of several zones or layers. From the inside out, the solar interior consists of:1  the core (the central region where nuclear reactions consume hydrogen to form helium. 2  These reactions release the energy that ultimately leaves the surface as visible light. ),he sun and its atmosphere consist of several zones or layers. From the inside out, the solar interior consists of:
dce6a2e12c7440fa1651e6db24f981d0
13. The Self-Sustaining Dynamo in the Earth's Core The Sun's Magnetism. The rotation of the Sun around its axis, therefore, does not by itself contribute to its magnetism. What is important in this case is that the Sun does not rotate like a solid ball.Its equator has a shorter rotation period than higher latitudes-- about 25 days for the equator, 27 days for latitude 40 degrees (the Earth meanwhile moves some distance around the Sun, so from here the period seems to be 27 and 29 days).hat is important in this case is that the Sun does not rotate like a solid ball. Its equator has a shorter rotation period than higher latitudes-- about 25 days for the equator, 27 days for latitude 40 degrees (the Earth meanwhile moves some distance around the Sun, so from here the period seems to be 27 and 29 days).
9a089c560fa88f4547bba9016fd6a962
Radiation zone A radiation zone, radiative zone or radiative region is a layer of a star's interior where energy is primarily transported toward the exterior by means of radiative diffusion and thermal conduction, rather than by convection. Energy travels through the radiation zone in the form of electromagnetic radiation as photons. radiation zone, radiative zone or radiative region is a layer of a star's interior where energy is primarily transported toward the exterior by means of radiative diffusion and thermal conduction, rather than by convection. Energy travels through the radiation zone in the form of electromagnetic radiation as photons.
3df843a447af6b676922a9d0d19f1944
Earth's orbit Because of the axial tilt of the Earth in its orbit, the maximum intensity of sun rays hits the earth 23.4 degrees north of equator at the June Solstice (at the Tropic of Cancer), and the maximum intensity of sun rays hits the earth 23.4 degrees south of equator at the December Solstice (at the Tropic of Capricorn).
ad1a46a8c7e73bfca0b970e7de1fad79
How does the ozone layer protect Earth from radiation? The ozone layer acts as a filter for the shorter wavelength and highly hazardous ultraviolet radiation (UVR) from the sun, protecting life on Earth from its potentially harmful effects. When the sky is clear, there is an inverse relationship between stratospheric ozone and solar UVR measured at the Earth’s surface.
4a0649a3da2490d292da48031699b967
- The sun and other stars do show periods of slightly higher than normal activity, detectable in our sun by an increase in sunspot activity. During sunspot activity, more energy reaches the Earth. The sun spends about a quarter of its time in a state with very few sunspots.