Ricco's Law
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Riccò's law, discovered by astronomer
Annibale Riccò Annibale Riccò (14 September 1844 – 23 September 1919) was an Italian astronomer. Biography He was born in Milan, Italy. In 1868 he was awarded a bachelor's degree from the '' Università di Modena'', then an engineering degree from the ' ...
, is one of several laws that describe a human's ability to visually detect targets on a uniform background. This law explains the visual relationship between a target
angular area In geometry, a solid angle (symbol: ) is a measure of the amount of the field of view from some particular point that a given object covers. That is, it is a measure of how large the object appears to an observer looking from that point. The poi ...
''A'' and target luminance increment \Delta L required for detection when that target is unresolved (that is, is too small in the field of view to make out different parts of it). The law is given by: :\mathrm \Delta L = \frac k where k is a constant (for a given background, see below). For constant background luminance L, the equation can be restated as :\Delta L / L = C = \frac K with a different constant K. The fraction \Delta L / L is referred to as Weber contrast ''C''. Riccò's law is applicable for regions where the target being detected is unresolved. The resolution of the human eye (the receptive field size) is approximately one arc-minute in the center (the fovea center) but the size increases in peripheral vision. Riccò's law is applicable for targets of angular area less than the size of the receptive field. This region is variable based on the amount of background
luminance Luminance is a photometric measure of the luminous intensity per unit area of light travelling in a given direction. It describes the amount of light that passes through, is emitted from, or is reflected from a particular area, and falls withi ...
. Riccò's law is based on the fact that within a receptive field, the light energy (or the number of photons per second) required to lead to the target being detected is summed over the area and is thus proportional to the luminance and to the area. Therefore, the contrast threshold required for detection is proportional to the signal-to-noise ratio multiplied by the noise divided by the area. This leads to the above equation. The "constant" ''K'' is actually a function of the background
luminance Luminance is a photometric measure of the luminous intensity per unit area of light travelling in a given direction. It describes the amount of light that passes through, is emitted from, or is reflected from a particular area, and falls withi ...
''B'' to which the eye is assumed to be adapted. It has been shown by
Andrew Crumey Andrew Crumey (born 1961) is a novelist and former literary editor of the Edinburgh newspaper ''Scotland on Sunday''. Life and career Crumey was born in Kirkintilloch, north of Glasgow, Scotland. He graduated with First Class Honours from the Uni ...
that for unconstrained vision (that is, observers could either look directly or at the target or avert their gaze) an accurate empirical formula for ''K'' is :K = (c_1B^+c_2)^2 where ''c1'', ''c2'' are constants taking different values for
scotopic In the study of human visual perception, scotopic vision (or scotopia) is the vision of the eye under low-light conditions. The term comes from Greek ''skotos'', meaning "darkness", and ''-opia'', meaning "a condition of sight". In the human eye, ...
and
photopic Photopic vision is the vision of the eye under well-lit conditions (luminance levels from 10 to 108  cd/m2). In humans and many other animals, photopic vision allows color perception, mediated by cone cells, and a significantly higher visua ...
vision. For low ''B'' this approximates to the De Vries-Rose Law for threshold contrast ''C'' :C\equiv\fracB \propto\frac 1. However, at very low background luminance (less than 10−5
candela per square metre The candela per square metre (symbol: cd/m2) is the unit of luminance in the International System of Units (SI). The unit is based on the candela, the SI unit of luminous intensity, and the square metre, the SI unit of area. The nit (symbol: n ...
) the threshold value for the
illuminance In photometry, illuminance is the total luminous flux incident on a surface, per unit area. It is a measure of how much the incident light illuminates the surface, wavelength-weighted by the luminosity function to correlate with human brightness ...
:\Delta I=A\Delta B is a constant (around 10−9
lux The lux (symbol: lx) is the unit of illuminance, or luminous flux per unit area, in the International System of Units (SI). It is equal to one lumen per square metre. In photometry, this is used as a measure of the intensity, as perceived by the ...
) and does not depend on ''B''. In that case :C=\fracB=\frac or :K=\fracB. At high ''B'' such as the daylight sky, Crumey's formula approaches an asymptotic value for ''K'' of or
lux The lux (symbol: lx) is the unit of illuminance, or luminous flux per unit area, in the International System of Units (SI). It is equal to one lumen per square metre. In photometry, this is used as a measure of the intensity, as perceived by the ...
per nit.From coefficients r4 or from coefficients a3 and a5.


Ricco's Areas

Ricco’s Areas are any areas of the retina where cells can detect a visual stimulus at threshold. The areas will change in location and size depending on the type of cells, the light conditions and the type of stimulus


See also

*
Spatial summation Summation, which includes both spatial summation and temporal summation, is the process that determines whether or not an action potential will be generated by the combined effects of excitatory and inhibitory signals, both from multiple simultane ...
* Weber's law *Bloch's law (termporal summation)


References

{{Reflist Photometry