why is the east coast humid and west coast dr
Why Is The East Coast Humid And West Coast Dry? One of ...
In total approximately 70% of incoming radiation is absorbed by the atmosphere and the Earth’s surface while around 30% is reflected back to space and does not heat the surface.
Today, people use solar energy to heat buildings and water and to generate electricity. In 2015, solar energy accounted for just over 0.4 percent of U.S. energy consumption – less than one percent! The top producing solar energy states include many of the sunny, warm states in the western United States.
~50% of the incoming energy is absorbed by the earth’s surface i.e. the land and oceans. ~30% is directly reflected back to space by clouds, the earth’s surface and different gases and particles in the atmosphere (the earth’s albedo is 0.3 on average).
Only a part of solar radiation reaches the Earth’s surface: 34% of solar radiation is reflected into space by the atmosphere, by clouds and by the Earth’s surface itself. Of the remaining 66%, 19% is absorbed by water vapour, by clouds and by the ozone layer and only 47% on average is absorbed by the Earth’s surface.
All of the energy the sun releases does not reach Earth. One one-billionth of the Sun’s total energy output actually reaches the Earth. Of all the energy that does reach Earth, slightly less than 34 percent is reflected back to space by clouds. The Earth itself reflects another 66 percent back to space.
So for the six hours in the middle of a sunny day, an area the size of a small backyard swimming pool (48 m2) will receive about 288 kilowatts of energy. That’s nearly 10 times what the average US household uses in an entire day!
Solar energy is created by nuclear fusion that takes place in the sun. Fusion occurs when protons of hydrogen atoms violently collide in the sun’s core and fuse to create a helium atom. This process, known as a PP (proton-proton) chain reaction, emits an enormous amount of energy.
The atmosphere absorbs 16% (by air) plus 4% (by clouds) of the solar radiation arriving at the top of the atmosphere, and it absorbs 99% of the 105% of the longwave IR radiation emitted by the earth’s surface.
Most of the electromagnetic radiation that comes to the earth from the sun is invisible. Only a small portion comes as visible light. … Most of the solar radiation is absorbed by the atmosphere and much of what reaches the earth’s surface is radiated back into the atmosphere to become heat energy.
A total of 173,000 terawatts (trillions of watts) of solar energy strikes the Earth continuously. That’s more than 10,000 times the world’s total energy use. And that energy is completely renewable — at least, for the lifetime of the sun.
In terms of mass, you can think of the total energy output as about 4,000,000 tons every second. When the curvature of the Earth and the density of the luminosity that hits our planet is considered, we receive only about 4.5 pounds per second of that energy.
By mass the composition of the sun is 92.1% hydrogen and 7.9% helium. Various metals make up less than 0.1% of the mass of the sun. The temperature of the sun’s surface is about 10,340 degrees Fahrenheit (5,726 degrees Celsius).
25% on incoming sunlight is reflected by clouds, dust, and gases in the air. 5% is reflected by the surface back into the atmosphere.
The sun produces 1.23 x 10 ^ 35 Joules of energy in one year. To compare, a nuclear weapon only gives off 4.18 x 10 ^ 15 Joules of energy, which is less energy than the Sun produces in ONE SECOND.
Energy is made through the process of nuclear fusion. This is when two hydrogen nuclei join to make helium. This occurs in the sun’s core where there is very high pressure and temperature.
1. 7×1017 joule/second.
30% is directly reflected back i.e re-radiated towards space by clouds, the earth’s surface, and different gases and particles in the atmosphere (the earth’s albedo is 0.3 on average).
Of the light that reaches Earth’s surface, infrared radiation makes up 49.4% of while visible light provides 42.3% 9. Ultraviolet radiation makes up just over 8% of the total solar radiation.
Insolation refers to the average amount of longwave radiation emitted by the earth. Insolation is the flow rate of incoming solar energy, as measured at the top of the atmosphere.
In radiation, heat is transferred in the form of electromagnetic radiation, through the medium. We know that space is a vacuum, and also that the electromagnetic radiations can pass through a vacuum. Hence clearly, the sun’s heat reaches the earth through the process of radiation.
Only a part of solar radiation reaches the Earth’s surface: 34% of solar radiation is reflected into space by the atmosphere, by clouds and by the Earth’s surface itself. Of the remaining 66%, 19% is absorbed by water vapour, by clouds and by the ozone layer and only 47% on average is absorbed by the Earth’s surface.
The amount of sunlight that hits the Earth in one hour provides more power than the entire world consumes in one year [1]. … Each hour 430 quintillion Joules of energy from the sun hits the earth. 430 quintillion is the number 430 with 18 zeroes! In contrast, all humans combined use 410 quintillion Joules in a year.
All of the energy from the Sun that reaches the Earth arrives as solar radiation, part of a large collection of energy called the electromagnetic radiation spectrum. Solar radiation includes visible light, ultraviolet light, infrared, radio waves, X-rays, and gamma rays.
The Sun doesn’t have a solid surface like Earth and the other rocky planets and moons. … Although we call it the surface, the photosphere is actually the first layer of the solar atmosphere. It’s about 250 miles thick, with temperatures reaching about 10,000 degrees Fahrenheit (5,500 degrees Celsius).
5,778 K
As you can see, the amount reflected by the atmosphere (6%), clouds (20%) and the surface of the Earth (4%) is 30%. The gases in the atmosphere also absorbs 16%, and clouds absorb 3%. That is 49%. The reason the atmosphere is different from the clouds is the atmosphere is referring to gases in the atmosphere.
albedo. the percentage of incoming sunlight that a surface reflects.
How much of the sun’s incoming energy is reflected back out to space? About one-third of the sun’s incoming energy is reflected back out to space.
The solar energy reaching the earth is 12,211 gigawatt/hour. Using the measurement of the earth’s surface and the number of hours in a year, scientists conclude the earth receives 82 million quads of Btu energy from the sun each year. A “quad” is one quadrillion British Thermal Units (BTUs) of energy.
The sun’s energy is produced in its central region by the fusion of hydrogen nuclei into helium nuclei. What two forces in the sun interact to produce a stable structure? The sun remains stable because the inward pull of gravity balances the outward push of thermal pressure from nuclear fusion.
How does the sun release so much energy? Hydrogen particles smash into each other and produce helium. Every time this happens the sun releases energy as heat and light. This process is called fusion and you need tremendous heat and pressure for it to occur.
How does the Sun produce the energy that heats our planet? The core of the Sun has radioactive atoms that give off energy as they decay. Gas inside the Sun heats up when compressed, giving off large amounts of energy. Heat trapped by magnetic fields in the Sun is released as energy.
Each hour 430 quintillion Joules of energy from the sun hits the Earth. That’s 430 with 18 zeroes after it! In comparison, the total amount of energy that all humans use in a year is 410 quintillion Joules.
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