Sentences with phrase «outer atmosphere into»

THE solar wind is a hurricane of charged particles that blows from the Sun's outer atmosphere into deep space at a million miles per hour.

Near the end of its life, a huge star blasts much of its bloated outer atmosphere into space — a torrent of gas equal to Earth's mass each year, racing outward at 10 million kilometers per hour.

Not exact matches

On Earth, the brightest auroras (the high - altitude glows often called the northern and southern lights) are generated when electrons in outer space near Earth are accelerated by large electrical potentials, or voltages, along the lines in our planet's magnetic field and slam into gas molecules in the upper atmosphere above polar regions.

The release of CO2 into the atmosphere contributes to the trapping of heat that would otherwise be emitted into outer space.

The radiation belts are two donut - shaped regions of highly energetic particles trapped in the Earth's magnetic field — the inner, located just above our atmosphere and extending 4,000 miles into space; and the outer, from 8,000 to 26,000 miles out — and are named for their discoverer (as are the probes), the late James A. Van Allen of the University of Iowa.

Most of the gas cascades back onto the sun, but a small fraction may escape into the outer atmosphere to feed the solar wind — a steady stream of particles that blows far into space.

Waves in the jet then transport material and energy into the outer atmosphere of the Sun and the wider Solar System.

Scientists suspect water on the surface of Mars evaporates, rises into the upper atmosphere, breaks into hydrogen and oxygen atoms, and is then swept into outer space by the solar wind.

The outer layers of the star — the stellar «atmosphere» — absorb this excess and swell outward into the characteristic distended figure of a red giant.

About every five minutes, spicules shoot red hot streams of charged particles into the corona, the outer layer of the solar atmosphere, at around 150 kilometres per second.

If the energy delivered to Earth by the Sun or by impacts (or both) were 40 % greater, the Earth would experience a runaway greenhouse.3 That is, more water would evaporate from Earth's surface, so too much heat trying to escape into outer space would be blocked by water vapor in the atmosphere.

In particular, both olive oil and oleic acid have been shown to increase trans - epidermal water loss (TEWL), which in scientific terms is the quantity of water that passes through the outer epidermis into the atmosphere.

The premise of Lindzen's hypothesis was that as the climate warms, the area in the atmosphere covered by high cirrus clouds will contract to allow more heat to escape into outer space, similar to the iris in a human eye contracting to allow less light to pass through the pupil in a brightly lit environment.

But that's actually an understatement by Gallup, since more than 97 % of the world's climatologists say that those carbon gases, which are given off by humans» burning of carbon - based fuels, are causing this planet's temperatures to rise over the long term, as those carbon gases accumulate in the atmosphere and also block the heat from being radiated back into outer space.

Greenhouse gases such as carbon dioxide accumulate in the atmosphere and trap heat that normally would exit into outer space.

About 30 percent of the sunlight that beams toward Earth is deflected by the outer atmosphere and scattered back into space.

The exosphere, the highest layer, is extremely thin and is where the atmosphere merges into outer space.

Air warmed at the surface naturally tends to rise above the majority of the (blocking) atmosphere and it can not descend until it has cooled by the emission of IR into the cool of outer space.

Greenhouse Effect As sunlight enters the Earth's atmosphere, some of the radiation from the sun is reflected back into outer space But, some of that radiation.

The evidence here comes from satellite measurements of infrared radiation escaping from the earth into outer space, from measurements of sunlight reflected from clouds and from measurements of the temperature the earth's surface or of the troposphere, the roughly 10 km thick layer of the atmosphere above the earth's surface that is filled with churning air and clouds, heated from below at the earth's surface, and cooled at the top by radiation into space.

It means how HIGH up in the atmosphere heat radiation occurs into outer space.