efficient illuminance - definição. O que é efficient illuminance. Significado, conceito
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O que (quem) é efficient illuminance - definição

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-market hypothesis         
  • Replication of Figure 5 of Martineau (2021), see also Ball and Brown (1968)
  • [[Daniel Kahneman]]
  • 0-393-32535-0}}. p.254.</ref>
ECONOMIC THEORY THAT ASSET PRICES FULLY REFLECT ALL AVAILABLE INFORMATION, SO THAT IT IS IMPOSSIBLE TO "BEAT THE MARKET" CONSISTENTLY ON A RISK-ADJUSTED BASIS
Efficient Markets Hypothesis; Efficient markets theory; Efficient markets; Efficient Markets Theory; Efficient markets hypothesis; Efficient market theory; Market efficiency; Efficient market; Semi-strong form; Inefficient markets; Efficient Market Hypothesis; Hypothesis of market efficiency; Efficient market hypothesis; Efficient capital markets; Market stability; Efficient-market theory
The efficient-market hypothesis (EMH) is a hypothesis in financial economics that states that asset prices reflect all available information. A direct implication is that it is impossible to "beat the market" consistently on a risk-adjusted basis since market prices should only react to new information.
Centrum pro efektivní dopravu         
ORGANIZATION
User:Thisusernameisalreadytaken/Centre for Efficient Transport; Centre for Efficient Transport; Centrum pro Efektivni Dopravu; Centrum pro Efektivní Dopravu
The Centre for Efficient Transport (Centrum pro efektivní dopravu, abbreviated CEDOP) is a Czech-based think tank that advocates the development of public and rail transport. p.
Score (statistics)         
GRADIENT OF THE LIKELIHOOD FUNCTION
Efficient score
In statistics, the score (or informant) is the gradient of the log-likelihood function with respect to the parameter vector. Evaluated at a particular point of the parameter vector, the score indicates the steepness of the log-likelihood function and thereby the sensitivity to infinitesimal changes to the parameter values.

Wikipédia

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.