efficient illuminance - traducción al ruso
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efficient illuminance - traducción al ruso

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.

efficient illuminance      
действующая освещённость
efficient score         
GRADIENT OF THE LIKELIHOOD FUNCTION
Efficient score

математика

эффективный вклад

inefficiency         
DEGREE TO WHICH A PROCESS MINIMIZES WASTE OF RESOURCES
Inefficiency; Inefficient; Effeciency; Highly efficient; Inefficiencies

[ini'fiʃ(ə)nsi]

общая лексика

неэффективность

недостаточность

нераспорядительность

антоним

efficiency

Смотрите также

coefficient of inefficiency

существительное

общая лексика

неспособность

неумение

недейственность

неэффективность

неспособность, неумелость

неэффективность, недейственность

Definición

Inefficient
·adj Not efficient; not producing the effect intended or desired; inefficacious; as, inefficient means or measures.
II. Inefficient ·adj Incapable of, or indisposed to, effective action; habitually slack or remiss; effecting little or nothing; as, inefficient workmen; an inefficient administrator.

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.

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