heat budget - translation to ρωσικά
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heat budget - translation to ρωσικά

OVERVIEW ABOUT EARTH'S ENERGY BUDGET
Radiation budget; Heat budget; Earth's radiation balance; Earth Radiation Budget; Radiation Balance; Radiation balance; Radiative balance; RADIATIVE BALANCE; Earth radiation budget; Earth’s energy balance; Earth's energy balance; Earth's Energy Imbalance; Earth's heating rate; Earth's energy imbalance
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  • Schematic drawing of Earth's excess heat inventory as it relates to the planet's energy imbalance for two recent time periods.<ref name=EarthSysSciData_20200907 />
  • The rising accumulation of energy in the oceanic, land, ice, and atmospheric components of Earth's climate system since 1960.<ref name=EarthSysSciData_20200907 />
  • The growth in Earth's energy imbalance from satellite and [[in situ]] measurements (2005–2019). A rate of +1.0&nbsp;W/m<sup>2</sup> summed over the planet's surface equates to a continuous heat uptake of about 500&nbsp;[[terawatt]]s (~0.3% of the incident solar radiation).<ref name=GeophysResLtrs_20210615 /><ref name=em_20210622 />
  • The greenhouse effect traps infrared heat, and ultimately raises Earth's surface temperatures.
  • Animation of the orbits of NASA's 2011 fleet of Earth remote sensing observatories.
  • ''Outgoing'', longwave flux radiation at the top-of-atmosphere (26–27 Jan 2012). Heat energy radiated from Earth (in watts per square metre) is shown in shades of yellow, red, blue and white. The brightest-yellow areas are the hottest and are emitting the most energy out to space, while the dark blue areas and the bright white clouds are much colder, emitting the least energy.
  • CERES]] measurements (26–27 Jan 2012). Brightest white areas show the highest reflectivity (least absorption) of solar energy, while darkest blue areas show the greatest absorption.
  • imbalance]] (or rate of global heating; shown in figure as the "net absorbed" amount) grew from +0.6&nbsp;W/m<sup>2</sup> (2009 est.<ref name="WEB-NASA-EnergyBudgetPoster" />) to above +1.0&nbsp;W/m<sup>2</sup> in 2019<ref name=GeophysResLtrs_20210615 />.

heat budget         

общая лексика

тепловой баланс

radiation balance         

общая лексика

радиационный баланс

машиностроение

баланс лучистый

budget bill         
  • Budgeted revenues of governments in 2006
  • The financial crisis caused by the [[South Sea company]] led to the presentation of the government budget under Sir [[Robert Walpole]]. Painting by [[Edward Matthew Ward]].
GOVERNMENT DOCUMENT PRESENTING THE GOVERNMENT'S PROPOSED REVENUES AND SPENDING FOR A FISCAL YEAR
State budget; Government budgets; Budget Bill; Public budget; Finance bill; National budget; Budget Bills; City budget; Budget bill; Governmental budget; Governmental budgets; Supplementary budget; Parliamentary budget; Parliamentary budgets
бюджетный законопроект

Ορισμός

Heat
·noun Sexual excitement in animals.
II. Heat ·noun Fermentation.
III. Heat ·noun Animation, as in discourse; ardor; fervency.
IV. Heat ·noun Agitation of mind; inflammation or excitement; exasperation.
V. Heat ·Impf & ·p.p. Heated; as, the iron though heat red-hot.
VI. Heat ·vt To excite or make hot by action or emotion; to make feverish.
VII. Heat ·noun Utmost violence; rage; vehemence; as, the heat of battle or party.
VIII. Heat ·vt To excite ardor in; to rouse to action; to excite to excess; to inflame, as the passions.
IX. Heat ·vt To make hot; to communicate heat to, or cause to grow warm; as, to heat an oven or furnace, an iron, or the like.
X. Heat ·noun A single complete operation of heating, as at a forge or in a furnace; as, to make a horseshoe in a certain number of heats.
XI. Heat ·vi To grow warm or hot by the action of fire or friction, ·etc., or the communication of heat; as, the iron or the water heats slowly.
XII. Heat ·vi To grow warm or hot by fermentation, or the development of heat by chemical action; as, green hay heats in a mow, and manure in the dunghill.
XIII. Heat ·noun A violent action unintermitted; a single effort; a single course in a race that consists of two or more courses; as, he won two heats out of three.
XIV. Heat ·noun High temperature, as distinguished from low temperature, or cold; as, the heat of summer and the cold of winter; heat of the skin or body in fever, ·etc.
XV. Heat ·noun The sensation caused by the force or influence of heat when excessive, or above that which is normal to the human body; the bodily feeling experienced on exposure to fire, the sun's rays, ·etc.; the reverse of cold.
XVI. Heat ·noun Indication of high temperature; appearance, condition, or color of a body, as indicating its temperature; redness; high color; flush; degree of temperature to which something is heated, as indicated by appearance, condition, or otherwise.
XVII. Heat ·noun A force in nature which is recognized in various effects, but especially in the phenomena of fusion and evaporation, and which, as manifested in fire, the sun's rays, mechanical action, chemical combination, ·etc., becomes directly known to us through the sense of feeling. In its nature heat is a mode if motion, being in general a form of molecular disturbance or vibration. It was formerly supposed to be a subtile, imponderable fluid, to which was given the name caloric.

Βικιπαίδεια

Earth's energy budget

Earth's energy budget accounts for the balance between the energy that Earth receives from the Sun and the energy the Earth loses back into outer space. Smaller energy sources, such as Earth's internal heat, are taken into consideration, but make a tiny contribution compared to solar energy. The energy budget also accounts for how energy moves through the climate system. Because the Sun heats the equatorial tropics more than the polar regions, received solar irradiance is unevenly distributed. As the energy seeks equilibrium across the planet, it drives interactions in Earth's climate system, i.e., Earth's water, ice, atmosphere, rocky crust, and all living things. The result is Earth's climate.

Earth's energy budget depends on many factors, such as atmospheric aerosols, greenhouse gases, the planet's surface albedo (reflectivity), clouds, vegetation, land use patterns, and more. When the incoming and outgoing energy fluxes are in balance, Earth is in radiative equilibrium and the climate system will be relatively stable. Global warming occurs when earth receives more energy than it gives back to space, and global cooling takes place when the outgoing energy is greater. Multiple types of measurements and observations show a warming imbalance since at least year 1970. The rate of heating from this human-caused event is without precedent.

When the energy budget changes, there is a delay before average global surface temperature changes significantly. This is due to the thermal inertia of the oceans, land and cryosphere. Accurate quantification of these energy flows and storage amounts is a requirement within most climate models.

Μετάφραση του &#39heat budget&#39 σε Ρωσικά