convective zone - translation to russian
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convective zone - translation to russian

(OF A STAR) LAYER WHICH IS UNSTABLE TO CONVECTION. ENERGY IS PRIMARILY OR PARTIALLY TRANSPORTED BY CONVECTION IN SUCH A REGION
Convective zone
  • An illustration of the structure of the [[Sun]] and a [[red giant]] star, showing their convective zones. These are the granular zones in the outer layers of the stars.

convective zone         
конвективная зона
bathypelagic         
  • Layers of the pelagic zone
  • carbon fixation]].
PART OF THE PELAGIC ZONE THAT EXTENDS FROM A DEPTH OF 1000 TO 4000 METERS (3300 TO 13000 FEET) BELOW THE OCEAN SURFACE. IT LIES BETWEEN THE MESOPELAGIC ABOVE, AND THE ABYSSOPELAGIC BELOW
Bathypelagic; Bathypelagic Zone; Bathyal zone; Bathyal Zone; Bathyal; Midnight zone; Midnight Zone; Bathypelagic realm; Scary Zone; The Scary Zone; Dark zone

общая лексика

батипелагический

нефтегазовая промышленность

глубоководный

bathyal         
  • Layers of the pelagic zone
  • carbon fixation]].
PART OF THE PELAGIC ZONE THAT EXTENDS FROM A DEPTH OF 1000 TO 4000 METERS (3300 TO 13000 FEET) BELOW THE OCEAN SURFACE. IT LIES BETWEEN THE MESOPELAGIC ABOVE, AND THE ABYSSOPELAGIC BELOW
Bathypelagic; Bathypelagic Zone; Bathyal zone; Bathyal Zone; Bathyal; Midnight zone; Midnight Zone; Bathypelagic realm; Scary Zone; The Scary Zone; Dark zone

геология

батиаль

батиальная зона (зона Мирового океана между мелководной и глубоководной зонами)

батиальный

Definition

ЧАСОВЫЕ ПОЯСА
см. Поясное время.

Wikipedia

Convection zone

A convection zone, convective zone or convective region of a star is a layer which is unstable due to convection. Energy is primarily or partially transported by convection in such a region. In a radiation zone, energy is transported by radiation and conduction.

Stellar convection consists of mass movement of plasma within the star which usually forms a circular convection current with the heated plasma ascending and the cooled plasma descending.

The Schwarzschild criterion expresses the conditions under which a region of a star is unstable to convection. A parcel of gas that rises slightly will find itself in an environment of lower pressure than the one it came from. As a result, the parcel will expand and cool. If the rising parcel cools to a lower temperature than its new surroundings, so that it has a higher density than the surrounding gas, then its lack of buoyancy will cause it to sink back to where it came from. However, if the temperature gradient is steep enough (i.e. the temperature changes rapidly with distance from the center of the star), or if the gas has a very high heat capacity (i.e. its temperature changes relatively slowly as it expands) then the rising parcel of gas will remain warmer and less dense than its new surroundings even after expanding and cooling. Its buoyancy will then cause it to continue to rise. The region of the star in which this happens is the convection zone.

What is the Russian for convective zone? Translation of &#39convective zone&#39 to Russian