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This text provides an overview of the six layers of Earth's atmosphere and highlights the importance of the atmosphere in providing oxygen, protecting the planet, and regulating temperature. It also explains the greenhouse effect and the role of the magnetosphere.
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AtmosphereA mixture of gases:N2 78% O2 21% Ar 0.9% CO2 0.03%
What makes Earth unique is Oxygen.The presence of water and carbon dioxide is also important.
The atmosphere provides oxygen, protects the Earth from harsh solar and cosmic radiation, keeps most meteoroids from becoming meteorites, and keeps the Earth’s surface warm.
The atmosphere is relatively small, half below 5 km, 99% below 30 km.
Layers of atmosphere:Troposphere - below 15 kmStratosphere - 15 to 40-50 kmMesosphere - 50 to 90 kmThermosphere - above 90 kmExosphere - above 250 km
The troposphere is the area where convection occurs.This rising of warm air and sinking of cooler air is powered by the surface heat of the Earth.
These convection currents are responsible for all the weather on Earth.
The top of the troposphere is the tropopause. Above this, in the stratosphere, the air is still.
In the ozone layer the temperature increases as solar UV radiation is absorbed by O2, O3(ozone), and N2.
This absorption of UV radiation protects the Earth from its effects.
The ozone layer stretches into the mesosphere, although the term “stratosphere” is often used to refer to both the stratosphere and the mesosphere.
In the thermosphere, the temperature increases with altitude because the high-energy part of the Sun’s spectrum splits molecules into atoms and atoms into ions.
This ionization of the atmosphere is significant above about 100 km. This electrically conductive part of the atmosphere is called the ionosphere.
This ionosphereis part of the thermosphere and can actually reflect certain radio wavelengths. (AM)
The surface of the Earth absorbs much energy from the Sun and reradiates it. Most of this energy escapes into space, but infrared radiation is partially blocked by the carbon dioxide and water vapor in the atmosphere.
This partial blocking of solar radiation is called the greenhouse effect.
Warmed air rises and is replaced by air that has been cooled in the upper atmosphere. This produces a circulation pattern called a convection cell.
This rising and falling air affects atmospheric heating and also produces surface winds. Passenger aircraft tend to fly above these disturbances, in the lower stratosphere.
The magnetosphere is the region around the Earth influenced by the Earth’s magnetic field. This field is similar to that of a bar magnet roughly aligned with the spin axis of the Earth.
It was detected by satellites launched in the late 1950’s. It contains two doughnut-shaped zones of high energy particles (one about 3000 and the other 20 000 km above the Earth’s surface), called the Van Allen Belts. The radiation here is lethal.
The magnetic field is believed to be caused by rotating, conducting material (molten iron and nickel) flowing in the Earth’s outer core. This is called dynamo theory.
The high energy particles in the Van Allen Belts are collected from the solar wind and are trapped because they are charged particles (primarily protons and electrons).
These charged particles often escape near the poles, where the magnetic field intersects the atmosphere. They rip apart air particles, creating spectacular lights called the aurora.
In the north, these lights are called the aurora borealis (northern lights). In the south, they are called the aurora australis (southern lights).
Earth isn’t the only planet to have aurorae. The next three pictures are of aurorae on Saturn. Notice the strange hexagonal shape on the last image.