Sentences with phrase «higher surface pressure»

Higher surface pressure at the pole pushes winds and polar storms into lower latitudes.
You correctly note that planets with thicker atmospheres and higher surface pressure usually have higher surface temperature, but this happens because atmospheres usually contain GHGs.
Climate change can also turn down the thermostat as a team led by Dr Michael Grose from CISRO in Tasmania in collaboration with CPDN's David Karoly and Mitchell Black discovered when they examined an unusual high surface pressure anomaly off the south coast of Australia in August 2014.
I can see how the anomalous westerlies and high surface pressure could contribute to warmer SSTs north of 20N in the Atlantic during El nino episodes, but to say it weakens the trade winds in the tropical belt is incorrect, most especially during the summer months when the Azores - Bermuda High is farther north.
Semipermanent anticyclones (high surface pressures), which tend to develop on the eastern sides of the world's ocean basins, result in alongshore surface wind stresses.

Not exact matches

The process of fracking involves vertical and horizontal drilling, often for more than 10,000 feet below the surface, followed by the injection of millions of gallons of water, chemicals and sand at high pressures.
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Last summer Gov. Andrew Cuomo lifted the official moratorium on the controversial drilling technique, which involves shooting a high pressure mixture of water and chemicals into the shale rock deep below the Earth's surface.
Hydrofracking relies on a high - pressure blend of chemicals, sand and water pumped deep underground to break up gas - bearing rock formations, freeing gas to rise up the well to the surface.
Diamonds form at high temperatures and pressures, crystallizing in pockets rich in the mineral carbonate before being carried to the surface with erupting magma (SN: 4/30/16, p. 8).
Scientists aren't sure why the blob formed, though many blame a ridge of high pressure that brought sunnier weather and less mixing of surface water with colder, deeper water.
«Titan's atmosphere is made up mainly of nitrogen and methane, with 50 % higher pressure at its surface than on Earth,» said Andrew Coates (UCL Mullard Space Science Laboratory), who led the study.
If a planet consists of a lot of gas, the atmospheric pressure on the surface may be so high that water is not able to keep its liquid form.
Materials with a surface area above 2,800 square meters per gram excelled at absorbing carbon dioxide at pressures of 30 bar, but the advantages of such high surface area diminished at lower pressures.
When pressure is higher, it better shields the surface from radiation.
Another disadvantage is the high levels of radiant heat energy produced by high - pressure sodium lamps; up to 75 % of the energy from HPS lamps that is not converted to light is emitted as radiant heat energy, causing the surface of the lamps to reach temperatures as high as 450 °C.
The wavenumber - 5 pattern is a ring of five high - and low - pressure systems in the atmosphere that circles the Earth's surface above the midlatitudes, or the temperate zone, running in a direction opposite to the flow of the jet stream.
On Proxima Centauri b, the model indicates that high stellar wind pressure would cause the atmosphere to escape and prevent atmosphere from lasting long enough to give rise to surface - based life as we know it.
Without the extraordinarily dry surface and the anomalous high - pressure conditions in the lowest level of the atmosphere occurring at the same time, the extreme, persistent hot spells wouldn't have occurred, says paper co-author Diego Miralles, a climate hydrologist at Ghent University in Belgium.
Together with his daughter Wendy and other colleagues at the Geophysical Laboratory of the Carnegie Institution for Science in Washington DC, he was using the device to test materials at pressures many millions of times higher than those at the Earth's surfacehigher even than in our planet's core — by squeezing them between two tiny diamond jaws.
Green explained that at 300 - 700 kilometers depth, the pressure and temperature are so high that rocks in this deep interior of the planet can not break by the brittle processes seen on Earth's surface.
A group of Japanese researchers led by Osaka University has proposed that substances heated with high - power lasers produce an ultrahigh pressure plasma state, comparable with those found at the centers of stars, and that the surface tension of the plasma can push back light.
At that boundary, atmospheric pressures 100,000 times higher than those at Earth's surface strip protons and electrons from the planet's hydrogen.
The bottom of that zone, deep in the seafloor mud, is where the temperature gets too high, toward Earth's hot interior; the top of the zone is where the pressure gets too low, moving toward the surface.
The analysis of high - frequency surface air temperature, mean sea - level pressure, wind speed and direction and cloud - cover data from the solar eclipse of 20 March 2015 from the UK, Faroe Islands and Iceland, published today (Monday 22 August 2016), sheds new light on the phenomenon.
A second study, led by Hailan Wang of NASA's Goddard Space Flight Center, used different model simulations and came to a similar conclusion: While a warming sea surface did make it more likely that a high - pressure ridge could form, the signal was not strong enough to explain its extreme nature.
But under the high - pressure conditions at the neutron star's surface, it would be transformed into a material made of pure neutrons, which some scientists believe would have a jelly - like consistency.
Also, the pressure exerted on the water is so high that hydrogen bond interactions with the graphene surface are overcome by the attractive van der Waals atomic interaction that draws together the graphene planes.
Thus, if a parcel of air from the surface rises (because of wind flowing up the side of a mountain, for example), it undergoes an expansion, from higher to lower pressure.
This allows magma and hydrothermal fluids originating in the mantle to intrude into Lusi's sediments, which triggers massive reactions and creates gas that generates high pressure below Earth's surface.
El Niño causes higher sea level pressure, warmer air temperature and warmer sea surface temperature in west Antarctica that affect sea ice distribution.
«One gram of MOF has a surface area of up to 10,000 square meters onto which it is possible to compact gas molecules into MOF pores like so many bees on a honeycomb without the high pressures and low temperatures usually required for compressed gas storage,» Yaghi says.
«When a comet impacts a planetary surface, it creates very high pressures and temperatures.
«Our speculation is that because of all the high antibiotic pressure, those are the only bugs that can survive, and they probably are coming in from surfaces in the NICU.»
Recharge ponds are constructed surface basins that allow water to collect and seep through the soil; injection wells use high - pressure pumps to actively push water down into aquifers.
InSAR uses a highly accurate radar to measure the change in distance between the satellite and ground surface, allowing the team to show that injecting water into the wells at high pressure caused ground uplift near the shallower wells, the release said.
Pressure - sensitive adhesives tend to flow out on materials having a high surface energy — for instance, metals, glass and plastics such as acrylic, polycarbonate and nylon.
The wavenumber - 5 pattern refers to a sequence of alternating high - and low - pressure systems (five of each) that form a ring circling the northern midlatitudes, several miles above the surface.
Normally, the reaction happens too slowly to be useful, but injecting carbon dioxide into the rock at high pressure would speed things up considerably; the formation of magnesium carbonate could cause the rock to expand and crack, with the increased surface area spurring the reaction to continue.
Given that some microbes can withstand temperatures as high as 122 °C and pressures about 3000 times higher than at Earth's surface, Plümper calculates that life could survive up to 10 kilometres beneath the seabed.
After the researchers analyzed the inclusions — each just 15 to 40 microns wide, or one - sixth to two - fifths of the diameter of a human hair — they found the inclusions contained the entire range of minerals one would expect of a volcanic rock called basalt that originally formed at the planet's surface and then crystallized under extreme high pressures and temperatures.
Beneath its thick atmosphere, the surface of Venus is much hotter and at a higher pressure than that of our planet, making its land surface hard to interpret.
Titan's surface pressure is a bit higher than our planet — standing on the moon would feel similar to standing 15 feet underwater here on Earth.
The higher sea level near the western ocean boundary creates a west - east pressure difference in the ocean, that results in the equatorial undercurrent flowing from west to east below the surface.
There, many kilometers deep, the carbonate rocks will be exposed to very high pressures and temperatures, converting the carbonate rocks back to the silicates and expelling CO2 and water — these gases will then find their ways to the surface through explosive volcanoes near the plate subduction boundaries.
While the large atmospheric pressure at the surface and the high altitude of the Venusian cloud layer appears to exclude the possibility of cloud - to - ground lightning (Gurnett et al. 2001; Aplin 2006), several authors have suggested that lightning discharges above, between or within clouds may occur (Borucki 1982; Russell & Scarf 1990; Gurnett et al. 2001).
Using these steady - states, we find that if volatile cycling is either solely dependent on temperature or seafloor pressure, exoplanets require a high abundance (more than 0.3 % of the total mass) of water to have fully inundated surfaces.
However, extreme events may require the combined effect of increased prevailing winds and tropical storms guided by the strengthened blocking high pressure and nurtured by the unusually warm late - Eemian tropical sea surface temperatures (Cortijo et al., 1999), which would favor more powerful tropical storms (Emanuel, 1987).
Typically, the snout, margins, sides, and surface ice are below the pressure - melting point, while thicker ice higher up in the accumulation area is warm - based [3].
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