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18 Sentences With "greenhouse effects"

How to use greenhouse effects in a sentence? Find typical usage patterns (collocations)/phrases/context for "greenhouse effects" and check conjugation/comparative form for "greenhouse effects". Mastering all the usages of "greenhouse effects" from sentence examples published by news publications.

"I am very worried about greenhouse effects," said a professor.
"I am very worried about greenhouse effects," Dr. Yanagisawa said.
Ceppi added that clouds also have their own greenhouse effects and can act as a blanket in the same way as greenhouse gases.
The brief required Elemental to use glass, Aravena told me, without providing enough money for a proper curtain wall to mitigate heat and greenhouse effects.
Propane can be used as a coolant in small air-conditioners at a fraction of the climate impact of HFCs, and ammonia is an industrial coolant with no greenhouse effects.
I was so mad about this release date I wanted to blame climate change on Calvin Harris, but obviously this song was just released too early and climate change is the longstanding result of human activity exacerbating greenhouse effects.
The weather is hot and humid with an average of over 30 °C year round. The oil well flares produce large amounts of carbon dioxide (CO2), which produces greenhouse effects which make the place even hotter. Precipitation is low during most of the year but the rain is heavy during the wet season.
Meteorology For Scientists and Engineers. A technical companion book with Ahrens' Meteorology Today, Brooks/Cole, Belmont CA, ., p. 400. Planetary equilibrium temperature differs from the global mean temperature and surface air temperature, which are measured observationally by satellites or surface-based instruments, and may be warmer than an equilibrium temperature due to greenhouse effects.
Other theories that explain the growing carbon rift (but exclude capitalism as a contributing factor) are the Chaotic Solar System theory, the claim that carbon is wrongly blamed for the greenhouse effects of water vapor and that the sun is causing global warming. These together are referred to as Non- Consensus views, and lack reliable scientific evidence.
The Earth was formed approximately 4.5 billion years ago. As it cooled and a crust and oceans formed, its atmosphere transformed from being dominated by hydrogen to one composed mostly of methane and ammonia. Over the next billion years, the metabolic activity of life transformed the atmosphere into a mixture of carbon dioxide, nitrogen, and water vapor. These gases changed the way that light from the sun hit the Earth's surface and greenhouse effects trapped heat.
Since the atmospheres, albedo and greenhouse effects of super-Earths are unknown, the surface temperatures are unknown and generally only an equilibrium temperature is given. For example, the black-body temperature of the Earth is 255.3 K (−18 °C or 0 °F ). It is the greenhouse gases that keep the Earth warmer. Venus has a black-body temperature of only 184.2 K (−89 °C or −128 °F ) even though Venus has a true temperature of 737 K (464 °C or 867 °F ).
Other studies of zircons found in Australian Hadean rock point to the existence of plate tectonics as early as 4 billion years ago. If true, that implies that rather than a hot, molten surface and an atmosphere full of carbon dioxide, early Earth's surface was much as it is today. The action of plate tectonics traps vast amounts of CO2, thereby reducing greenhouse effects, and leading to a much cooler surface temperature, and the formation of solid rock and liquid water.
Given the large spread in the masses of planets within a circumstellar habitable zone, coupled with the discovery of super-Earth planets which can sustain thicker atmospheres and stronger magnetic fields than Earth, circumstellar habitable zones are now split into two separate regions—a "conservative habitable zone" in which lower-mass planets like Earth can remain habitable, complemented by a larger "extended habitable zone" in which a planet like Venus, with stronger greenhouse effects, can have the right temperature for liquid water to exist at the surface.
But the anthropogenic greenhouse effects and changing insolation patterns may have unpredictable long-term effects. Reductions of glacial ice on land masses can cause isotatic rebounds and may affect earthquakes and volcanism over a wide range. Rising sea levels can also affect patterns, and was seen in Indonesia, simply drilling a gas well in the wrong place may have touched off a mud volcano and there are some signs that this may precede a new caldera formation for a volcano. Over the very long term, the change in temperature of the Earth's crust on geothermal and volcanic processes is unknown.
Adequate cooling of the surface typically takes place when it loses more energy by infrared radiation than it receives as solar radiation from the sun, which is especially the case on clear nights. Poor thermal conductivity restricts the replacement of such losses from deeper ground layers, which are typically warmer at night. Preferred objects of dew formation are thus poor conducting or well isolated from the ground, and non- metallic, while shiny metal coated surfaces are poor infrared radiators. Preferred weather conditions include the absence of clouds and little water vapor in the higher atmosphere to minimize greenhouse effects and sufficient humidity of the air near the ground.
The model's output is kilogram of CO2 produced per Megawatt hour of delivered energy. Scenario 33 for example, which concerns the production of heat from wood chips produced from UK small roundwood produced from bringing neglected broadleaf forests back into production, shows that burning oil releases 377 kg of CO2 while burning woodchip releases 1501 kg of CO2 per MW h delivered energy. On the other hand, scenario 32 in that same reference, which concerns production of heat from wood chips that would otherwise be made into particleboard, releases only 239 kg of CO2 per MW h delivered energy. Therefore the relative greenhouse effects of biomass energy production very much depends on the usage model.
Artist's depiction of the life cycle of a Sun-like star, starting as a main- sequence star at lower left then expanding through the subgiant and giant phases, until its outer envelope is expelled to form a planetary nebula at upper right. The faint young Sun paradox or faint young Sun problem describes the apparent contradiction between observations of liquid water early in Earth's history and the astrophysical expectation that the Sun's output would be only 70 percent as intense during that epoch as it is during the modern epoch. The issue was raised by astronomers Carl Sagan and George Mullen in 1972. Proposed resolutions of this paradox have taken into account greenhouse effects, changes to planetary albedo, astrophysical influences, or combinations of these suggestions.
Tidal heating experienced by planets in the habitable zone of red dwarfs less than 30% of the mass of the Sun may cause them to be "baked out" and become "tidal Venuses." Combined with the other impediments to red dwarf habitability, this may make the probability of many red dwarfs hosting life as we know it very low compared to other star types. There may not even be enough water for habitable planets around many red dwarfs; what little water found on these planets, in particular Earth- sized ones, may be located on the cold night side of the planet. In contrast to the predictions of earlier studies on tidal Venuses, though, this "trapped water" may help to stave off runaway greenhouse effects and improve the habitability of red dwarf systems.

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