optimum illuminance - traduzione in russo
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optimum illuminance - traduzione in russo

INTENSITY OF SUNLIGHT
Solar Constant; Solar Illuminance Constant; Solar illuminance constant
  • Solar irradiance spectrum at top of atmosphere, on a linear scale and plotted against [[wavenumber]].
  • A 1903 Langley bolograph with an erroneous solar constant of 2.54 calories/minute/square centimeter.

optimum illuminance      
оптимальная освещённость
optimal experiment         
EXPERIMENTAL DESIGN THAT IS OPTIMAL WITH RESPECT TO SOME STATISTICAL CRITERION
Optimum design; Optimum experiment; Optimal experiment; Optimum experimental designs; Model-oriented design of experiments; Optimal Design of Experiments; Alphabetic optimality; Optimal design of experiments; Optimal design of experiment; Optimum design of experiments; Optimum design of experiment; Optimal experimental design; Optimum experimental design; Optimal experimental designs; D-optimal design; E-optimal design; Optimal design model selection

математика

оптимальный эксперимент

acid phosphatase         
  • [[Reference ranges for blood tests]], showing acid phosphatase in red at left.
CLASS OF ENZYMES
Acid phosphatases; EC 3.1.3.2; Acid phosphomonoesterase; Acid monophosphatase; Acid phosphohydrolase; Acid phosphomonoester hydrolase; Uteroferrin; Acid nucleoside diphosphate phosphatase; Orthophosphoric-monoester phosphohydrolase (acid optimum); Phosphate-monoester phosphohydrolase (acid optimum)

медицина

кислая фосфатаза

Definizione

illuminance
[?'l(j)u:m?n?ns]
¦ noun Physics the amount of luminous flux per unit area.

Wikipedia

Solar constant

The solar constant (GSC) is a flux density measuring mean solar electromagnetic radiation (total solar irradiance) per unit area. It is measured on a surface perpendicular to the rays, one astronomical unit (au) from the Sun (roughly the distance from the Sun to the Earth).

The solar constant includes radiation over the entire electromagnetic spectrum. It is measured by satellite as being 1.361 kilowatts per square meter (kW/m2) at solar minimum (the time in the 11-year solar cycle when the number of sunspots is minimal) and approximately 0.1% greater (roughly 1.362 kW/m2) at solar maximum.

The solar "constant" is not a physical constant in the modern CODATA scientific sense; that is, it is not like the Planck constant or the speed of light which are absolutely constant in physics. The solar constant is an average of a varying value. In the past 400 years it has varied less than 0.2 percent. Billions of years ago, it was significantly lower.

This constant is used in the calculation of radiation pressure, which aids in the calculation of a force on a solar sail.

Traduzione di &#39optimum illuminance&#39 in Russo