ATMOSPHERE SYSTEM


the atmosphere, or envelope of the earth's magnetic field, serves as “the largest membrane on earth.” Doctor and author Lewis Thomas made this very popular comparison in 1973. Like a cell membrane, the atmosphere filters out what is allowed to enter and leave, as do various light waves. Thomas was amazed at how images such as the famous "Earthrise" portrayed the barren face of the moon "and the overflowing sky coming from behind. It seemed a miracle that the Earth was alive when everything around it looked like that ... no. Most of us take the atmosphere lightly and do not usually think about how it is made or how it moves or changes. We recognize when bad weather distracts us or we appreciate it when we are outdoors. But 5 billion years ago it was built and that is how we and all other life cells are able to survive. The Intro Earth sphere is a unique pool that forms a protective barrier between outer space and living space, where all living things on earth are. Air is actually a mixture of gases in airplanes, tasteless, colorless, shapely, and so well-mixed that they often act as a single gas. The closest recipe to Earth is 99% nitrogen and oxygen, slightly less than 1% argon, and a small percentage of volume comes from small gases, such as carbon dioxide. But this staggering mixture begins to deviate as we reach the outer edges of the atmosphere.

To better study further, we can divide the universe into vertical layers or "spheres" using a few different features. The four most closely linked layers are the troposphere, stratosphere, mesosphere, and thermosphere, and they come from studying the atmosphere based on their thermal structure. Each layer has a different initial temperature drop or rise as we move into outer space. Temperature affects even the thickness of the layers. The closest layer of Earth where the whole climate and most of the air molecule - the troposphere - can extend anywhere from 8 to 16 miles [8 to 16 km] above the earth, depending on the season or latitude of your location on Earth. That sounds artificial, but in reality it is just physics: when air molecules cool, they accumulate, making the air thicker and thicker. So in winter or near poles, the troposphere is the thinnest. And it is heated where air atoms are scattered, as in tropical and subtropical regions. When we move to the stratosphere, the next layer, temperatures tend to spread and heat continuously.

Here we have the ozone layer, which is part of the atmosphere with the highest levels of ozone, one of the smallest gases in our recipe. The ozone layer, in turn, allows life-giving light to pass through, while filtering out harmful substances, such as ultraviolet rays. Absorption of UV radiation is what causes temperatures to rise in the stratosphere. Then the temperature dropped in the mesosphere and increased again in a surprisingly hot thermosphere where a few air cells circulating outside were about 1,100 degrees Celsius! In all, the atmosphere stretches for 300 miles [480 km] above the earth. Sounds like a lot, but the Earth's width is 12,756km. Compared to that, the atmosphere looks like ... an orange peel. This small layer of gas is very important for life, which is why it is so important to talk about it early in our journey to the visible world. Outside of space, there are no processes we will learn in the hydrosphere, lithosphere, and biosphere that will work. The energy from the Sun constantly passes through different layers of the atmosphere like waves, descending and being absorbed by the earth's surface to provide warmth and warmth of life. In fact, those “forces” are electromagnetic radiation, or different wavelengths.

Everything - the Sun, the Earth, our skin - is constantly emitting radiation. Extremely hot and high-energy objects, such as the Sun, emit large amounts of energy, such as short waves, or rays of the sun, in the form of light. Cool objects, such as the Earth, emit very long wavelengths, or radiation. With so much sunlight passing through the atmosphere, we could expect the temperature to rise above the heat, such as when you sit under a blanket and heat up enough to get rid of it. Fortunately, the Earth is not too hot because Earth and the atmosphere naturally balance shortwave solar energy with the energy of longwave being restored to space. This is the wind energy budget, which is achieved through three common types of energy transfer. The first type of energy transfer is the radiation we have been talking about, the most common of which is radiation.

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