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{{For|the luminosity function in astronomy|Luminosity function (astronomy)}}
Going to a wine tasting can be a very enjoyable and pleasant knowledge. Even so, several men and women do not attend for fear of not knowing precisely how to act or what to do. There no great mystery to wine tastings, just a few issues you should remember.<br><br>As far as etiquette, generally the ladies are served prior to the gentlemen. Some wine tastings offer you you bottled waterUse this to rinse out your mouth between tastings so your palate is clean for the subsequent wineThere is usually unsalted and unflavored crackers and bread to help palate cleansing as well. You really should usually deal with the wine glass by the stem. This assists keep away from heating the wine with the warmth of your hands, therefore altering the taste. Steer clear of wearing strong perfumes and colognes to a wine tasting. 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You might be able to tell the age of a red wine by carrying out a rim test. Tilt the glass slightly towards the rim of the wine glass and look at the wine.  If the color of the red wine is much more of a purple, it is usually a younger wine. If the color of the red wine is brown, it is an older wine.<br><br>One more thing you might have observed people do ahead of they taste wine is swirl it slightly in the glass. This is to support open up the wine&quot;s flavor.  Remember that the wine might have been in a bottle anyplace from six months to several, a lot of years. When an individual swirls a wine, it helps release the flavors.  Just like when you happen to be cooking at house and stir the food to help blend the flavors.<br><br>The color of the wine is just a single aspect you will want to appear at when you attend a wine tasting.  You will also want to smell the wine.  Right after swirling, this is the subsequent step in the tasting methodYou have most likely seen men and women smell wine ahead of and wondered why they did it.  Smell plays a really critical element in what we taste.  Researchers have determined that maybe as significantly as 75% of what we taste is in fact based on what we smell very first. [http://avvocato-a-roma.info/blogs/beginning-wine-tasting/ Wisconsin Wine Tasting] contains further concerning the meaning behind it. You can smell your wine one of two techniques:  taking a small whiff to get an concept of how the wine smells, then a deeper whiff or take 1 deep whiffFollowing smelling the wine, take a minute to feel about the smell.   You do not want to quickly taste it after [http://Www.Smelling.net/ smelling] but give yourself time to discover exactly what you smelled.<br><br>Lastly, you will require to know is how to taste the wine correctly.  Your tongue has taste buds in both the front and back. These taste buds can detect bitter, salty, sweet, and sour flavors, but some are far more sensitive than other people are. There are three actions in tasting a wine:  the initial impression, the taste, and the aftertaste. The first impression happens when you take your first drink and the wine truly hits your taste buds. It should awaken your sense to the wine. After taking the 1st drink, you should swish the wine about your mouth for a handful of seconds to let all your taste buds discover the full flavor of the wine.  Feel about what the wine tastes like. Is it light or heavy?  Is the smooth or harsh?  The aftertaste is the sensation that remains in your mouth after swallowing the wine.  How lengthy did it last and was it pleasant?<br><br>Ahead of attending a wine tasting, it could support you really feel more confident to read about the different varieties of wines. This will give you a much better idea of what to appear for as far as flavor and taste. Next time you are invited to a wine tasting do not be afraid to goYou may possibly be missing a fantastic encounter!. 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[[Image:Luminosity.png|thumb|right|400px|[[Photopic vision|Photopic]] (black) and [[scotopic vision|scotopic]] (green) luminosity functions.<ref name="scvl" group=c/> The photopic includes the CIE 1931 standard<ref name="ciexyz31" group=c/> (solid), the Judd–Vos 1978 modified data<ref name="vljv" group=c/> (dashed), and the Sharpe, Stockman, Jagla & Jägle 2005 data<ref name="ssvl2" group=c/> (dotted). The horizontal axis is wavelength in [[Nanometre|nm]].]]
[[Image:Srgbspectrum.png|thumb|right|400px|]]
 
The '''luminosity function''' or '''luminous efficiency function''' describes the average [[spectral sensitivity]] of human visual perception of brightnessIt is based on subjective judgements of which of a pair of different-colored lights is brighter, to describe relative sensitivity to light of different wavelengths. It should not be considered perfectly accurate in every case, but it is a very good representation of visual sensitivity of the human eye and it is valuable as a baseline for experimental purposes.  
 
The CIE luminosity function <math>\overline{y}(\lambda)</math> or <math>V(\lambda)\,</math> is a standard function established by the [[Commission Internationale de l'Éclairage]] (CIE) and may be used to convert radiant energy into luminous (i.e., visible) energy. It also forms the central [[CIE 1931 color space#Color matching functions|color matching function]] in the [[CIE 1931 color space]].
 
== Details ==
 
There are two luminosity functions in common use. For everyday light levels, the [[photopic vision|photopic]] luminosity function best approximates the response of the human eye. For low light levels, the response of the human eye changes, and the [[scotopic vision|scotopic]] curve applies. The photopic curve is the CIE standard curve used in the CIE 1931 color space.
 
The [[luminous flux]] (or visible energy) in a light source is defined by the photopic luminosity function. The following equation calculates the total luminous flux in a source of light.
 
:<math>F=683.002\ \mathrm{lm/W}\cdot \int^\infin_0 \overline{y}(\lambda) J(\lambda) d\lambda</math>
 
where
:<math>F\,</math> is the luminous flux in [[lumen (unit)|lumen]]s,
:<math>J(\lambda)\,</math> is the [[spectral power distribution]] of the radiation (power per unit wavelength), in watts per metre.
:<math>\overline{y}(\lambda)</math> (also known as <math>V(\lambda)\,</math>) is the standard luminosity function (which is dimensionless).
:<math>\lambda\,</math> is wavelength in metres.
 
Formally, the integral is the [[inner product]] of the luminosity function with the light spectrum.<ref name="Charles2003"/> In practice, the integral is replaced by a sum over discrete wavelengths for which tabulated values of the luminosity function are available. The [[International Commission on Illumination|CIE]] distributes standard tables with luminosity function values at 5&nbsp;nm intervals from 380&nbsp;nm to 780&nbsp;nm.<ref name="CIEdocs" group=cie/>
 
The standard luminosity function is normalized to a peak value of unity at 555&nbsp;nm (see [[luminous coefficient]]). The value of the constant in front of the integral is usually rounded off to 683&nbsp;lm/W. The small excess fractional value comes from the slight mismatch between the definition of the lumen and the peak of the luminosity function. The lumen is defined to be unity for a radiant energy of 1/683 watt at a frequency of 540 THz, which corresponds to a standard air wavelength of 555.016&nbsp;nm rather than 555&nbsp;nm, which is the peak of the luminosity curve. The value of <math>\overline{y}(\lambda)</math> is 0.999997 at 555.016&nbsp;nm, so that a value of 683/0.999997 = 683.002 is the multiplicative constant.<ref name="Wyszecki2000"/>
The number 683 is connected to the modern (1979) definition of the [[candela]], the unit of [[luminous intensity]].<ref name="candela" group=cie/> This arbitrary number made the new definition give numbers equivalent to those from the old definition of the candela.
 
== Improvements to the standard ==
 
The CIE 1924 photopic <math>V(\lambda)</math> luminosity function,<ref name="CIE1926" group=cie/> which is included in the CIE 1931 color-matching functions as the ''y'' function, has long been acknowledged to underestimate the contribution of the blue end of the spectrum to perceived luminanceThere have been numerous attempts to improve the standard function, to make it more representative of human visionJudd in 1951,<ref name="Judd1975"/> improved by Vos in 1978,<ref name="Vos1978"/> resulted in a function known as CIE <math>V_M(\lambda)</math>.<ref name="Stiles1955"/>  More recently, Sharpe, Stockman, Jagla & Jägle (2005) developed a function consistent with the [http://www.cvrl.org/cones.htm Stockman & Sharpe cone fundamentals];<ref name="Sharpe2005"/> their curves are plotted in the figure above.
 
== Scotopic luminosity ==
 
For very low levels of intensity ([[scotopic vision]]), the sensitivity of the eye is mediated by rods, not cones, and shifts toward the [[violet (color)|violet]], peaking around 507&nbsp;nm for young eyes; the sensitivity is equivalent to 1699&nbsp;lm/W<ref name="Kohei2004"/> or 1700&nbsp;lm/W<ref name="Casimer1998"/> at this peak.   
 
The standard scotopic luminosity function or <math>V^\prime(\lambda)</math> was adopted by the CIE in 1951, based on measurements by Wald (1945) and by Crawford (1949).[http://www.cvrl.org/database/text/lum/scvl.htm]
 
== Color blindness ==
[[File:LuminosityCurve2.svg|right|thumb|400px|Protanopic (green) and deuteranopic (red) luminosity functions.<ref name="judd">{{cite book|last=Judd|first=Deane B.|title=Contributions to Color Science|year=1979|publisher=NBS|location=Washington D.C. 20234|url=http://books.google.ru/books?id=jgz_iI8NAzYC&pg=PA316|page=316}}</ref> For comparison, the standard photopic curve is shown in yellow.]]
[[Color blindness]] changes the sensitivity of the eye as a function of wavelength. For people with [[protanopia]], the peak of the eye's response is shifted toward the short-wave part of the spectrum (approximately 540&nbsp;nm), while for people suffering [[deuteranopia]], there is a slight shift in the peak of the spectrum, to about 560&nbsp;nm.<ref name="judd" /> People with protanopia have essentially no sensitivity to light of wavelengths more than 670&nbsp;nm.
 
Most [[mammals]] other than [[primates]] have the same luminosity function as people with protanopia. This makes it possible to study the nocturnal life of animals by illuminating the scene with long-wavelength red light that they can't see.<ref>{{cite journal|coauthors=I. S. McLennan & J. Taylor-Jeffs|title=The use of sodium lamps to brightly illuminate mouse houses during their dark phases|journal=Laboratory Animals|year=2004|volume=38|pages=384–392|pmid=15479553|doi= 10.1258/0023677041958927|url=http://la.rsmjournals.com/content/38/4/384.full.pdf}}</ref>
 
For older people with normal color vision, the [[crystalline lens]] may become slightly yellow due to [[cataract]]s, which moves the maximum of sensitivity to the red part of the spectrum and narrows the range of perceived wavelengths.
 
== See also ==
 
* [[A-weighting]], the sound equivalent
* [[Apparent brightness]]
* [[Color vision]]
* [[Quantum efficiency]], the image sensor equivalent
 
== References ==
 
{{reflist|3|refs=
<ref name="Charles2003">{{cite book
  | title    = Digital Video and HDTV: Algorithms and Interfaces
  | author    = Charles A. Poynton
  | publisher = Morgan Kaufmann
  | year      = 2003
  | isbn      = 1-55860-792-7
  | url      = http://books.google.com/?id=ra1lcAwgvq4C&pg=RA1-PA205&dq=luminance+dot-product
  }}</ref>
<ref name="Wyszecki2000">{{cite book
  | author    = Wyszecki, Günter and Stiles, W.S.
  | title    = Color Science - Concepts and Methods, Quantitative Data and Formulae
  | edition  = 2nd
  | publisher = Wiley-Interscience
  | year      = 2000
  | isbn      = 0-471-39918-3
  }}</ref>
<ref name="Judd1975">{{cite book
  | author    = Judd, Deane B. and Wyszecki, Günter
  | title    = Color in Business, Science and Industry
  | edition  = 3rd
  | publisher = John Wiley
  | year      = 1975
  | isbn      = 0-471-45212-2
  }}</ref>
<ref name="Vos1978">{{cite journal
  | author  = Vos, J. J.
  | title  = Colorimetric and photometric properties of a 2° fundamental observer
  | journal = Color Research and Application
  | year    = 1978
  | volume  = 3
  | issue  = 3
  | pages  = 125–128
  | doi    = 10.1002/col.5080030309
  }}</ref>
<ref name="Stiles1955">{{cite journal
  | author1 = Stiles, W. S.
  | author2 = Burch, J. M.
  | title  = Interim report to the Commission Internationale de l'Eclairage Zurich 1955, on the National Physical Laboratory's investigation of colour-matching
  | journal = Optica Acta
  | year    = 1955
  | volume = 2
  | pages  = 168–181
  | bibcode = 1955AcOpt...2..168S
   | doi    = 10.1080/713821039
  | issue  = 4
  }}</ref>
<ref name="Sharpe2005">{{cite journal
  | author1 = Sharpe, L. T.
  | author2 = Stockman, A.
  | author3 = Jagla, W.
  | author4 = Jägle, H.
  | year    = 2005
  | title  = A luminous efficiency function, V*(λ), for daylight adaptation
  | url    = http://calendar.arvo.org/5/11/3/Sharpe-2005-jov-5-11-3.pdf
  | journal = Journal of Vision
  | volume  = 5
  | number  = 11
  | pages  = 948–968
  | doi    = 10.1167/5.11.3
  }}</ref>
<ref name="Kohei2004">{{cite book
  | title    = Light Pollution Handbook
  | author1  = Kohei Narisada
  | author2  = Duco Schreuder
  | publisher = Springer
  | year      = 2004
  | isbn      = 1-4020-2665-X
  }}</ref>
<ref name="Casimer1998">{{cite book
  | title    = Handbook of Applied Photometry
  | author    = Casimer DeCusatis
  | publisher = Springer
  | year      = 1998
  | isbn      = 1-56396-416-3
  }}</ref>
}}
 
=== CIE documents ===
 
{{reflist|group=cie|refs=
<ref name="CIEdocs" group=cie>{{cite web
  | url  = http://www.cie.co.at/main/freepubs.html
  | title = CIE Free Documents for Download
  }}</ref>
<ref name="candela" group=cie>16th [[General Conference on Weights and Measures|Conférence générale des poids et mesures]] Resolution 3, CR, 100 (1979), and ''Metrologia'', '''16''', 56 (1980).</ref>
<ref name="CIE1926" group=cie>{{cite book
  | author    = CIE
  | title    = Commission internationale de l'Eclairage proceedings, 1924
  | publisher = Cambridge University Press, Cambridge
  | year      = 1926
  }}</ref>
}}
 
=== Curve data ===
{{reflist|group=c|refs=
<ref name="scvl">{{cite web
  | title      = CIE Scotopic luminosity curve (1951)
  | url        = http://www.cvrl.org/database/text/lum/scvl.htm
  | archiveurl  = http://web.archive.org/web/20081228115119/http://www.cvrl.org/database/text/lum/scvl.htm
  | archivedate = 2008-12-28
  }}</ref>
<ref name="ciexyz31">{{cite web
  | title      = CIE (1931) 2-deg color matching functions
  | url        = http://www.cvrl.org/database/text/cmfs/ciexyz31.htm
  | archiveurl  = http://web.archive.org/web/20081228084047/http://www.cvrl.org/database/text/cmfs/ciexyz31.htm
  | archivedate = 2008-12-28
  }}</ref>
<ref name="vljv">{{cite web
  | title      = Judd–Vos modified CIE 2-deg photopic luminosity curve (1978)
  | url        = http://www.cvrl.org/database/text/lum/vljv.htm
  | archiveurl  = http://web.archive.org/web/20081228083025/http://www.cvrl.org/database/text/lum/vljv.htm
  | archivedate = 2008-12-28
  }}</ref>
<ref name="ssvl2">{{cite web
  | title      = Sharpe, Stockman, Jagla & Jägle (2005) 2-deg V*(l) luminous efficiency function
  | url        = http://www.cvrl.org/database/text/lum/ssvl2.htm
  | archiveurl  = http://web.archive.org/web/20070927222337/http://www.cvrl.org/database/text/lum/ssvl2.htm
  | archivedate = 2007-09-27
  }}</ref>
}}
 
== External links ==
* [http://www.cvrl.org/lumindex.htm Color and Research Vision Laboratory - luminous efficiency data tables]
 
[[Category:Physical quantities]]
[[Category:Photometry]]

Latest revision as of 19:53, 19 November 2014

Going to a wine tasting can be a very enjoyable and pleasant knowledge. Even so, several men and women do not attend for fear of not knowing precisely how to act or what to do. There no great mystery to wine tastings, just a few issues you should remember.

As far as etiquette, generally the ladies are served prior to the gentlemen. Some wine tastings offer you you bottled water. Use this to rinse out your mouth between tastings so your palate is clean for the subsequent wine. There is usually unsalted and unflavored crackers and bread to help palate cleansing as well. You really should usually deal with the wine glass by the stem. This assists keep away from heating the wine with the warmth of your hands, therefore altering the taste. Steer clear of wearing strong perfumes and colognes to a wine tasting. If you have an opinion about the world, you will probably wish to discover about rate us. That might take away from not only your smell, but also that of the other guests. Also, avoid smoking, gum, and mints before and during a wine tasting to be in a position to get pleasure from the full flavor of the wine.

You can tell a lot about a wine just by hunting at its color. When you attend a wine tasting, the glasses really should usually be clear so you can get a great appear at the wine. The tables might also be covered with white tablecloths to support you see the wine"s color clearly. Do not let the wine name full you. For instance, white wines are not white in color. They may range from yellow to green to brown. Red wines range in color from pale red to a deep brownish red and frequently turn into lighter with age. Occasionally the color of a wine could indicate age or flavor. You might be able to tell the age of a red wine by carrying out a rim test. Tilt the glass slightly towards the rim of the wine glass and look at the wine. If the color of the red wine is much more of a purple, it is usually a younger wine. If the color of the red wine is brown, it is an older wine.

One more thing you might have observed people do ahead of they taste wine is swirl it slightly in the glass. This is to support open up the wine"s flavor. Remember that the wine might have been in a bottle anyplace from six months to several, a lot of years. When an individual swirls a wine, it helps release the flavors. Just like when you happen to be cooking at house and stir the food to help blend the flavors.

The color of the wine is just a single aspect you will want to appear at when you attend a wine tasting. You will also want to smell the wine. Right after swirling, this is the subsequent step in the tasting method. You have most likely seen men and women smell wine ahead of and wondered why they did it. Smell plays a really critical element in what we taste. Researchers have determined that maybe as significantly as 75% of what we taste is in fact based on what we smell very first. Wisconsin Wine Tasting contains further concerning the meaning behind it. You can smell your wine one of two techniques: taking a small whiff to get an concept of how the wine smells, then a deeper whiff or take 1 deep whiff. Following smelling the wine, take a minute to feel about the smell. You do not want to quickly taste it after smelling but give yourself time to discover exactly what you smelled.

Lastly, you will require to know is how to taste the wine correctly. Your tongue has taste buds in both the front and back. These taste buds can detect bitter, salty, sweet, and sour flavors, but some are far more sensitive than other people are. There are three actions in tasting a wine: the initial impression, the taste, and the aftertaste. The first impression happens when you take your first drink and the wine truly hits your taste buds. It should awaken your sense to the wine. After taking the 1st drink, you should swish the wine about your mouth for a handful of seconds to let all your taste buds discover the full flavor of the wine. Feel about what the wine tastes like. Is it light or heavy? Is the smooth or harsh? The aftertaste is the sensation that remains in your mouth after swallowing the wine. How lengthy did it last and was it pleasant?

Ahead of attending a wine tasting, it could support you really feel more confident to read about the different varieties of wines. This will give you a much better idea of what to appear for as far as flavor and taste. Next time you are invited to a wine tasting do not be afraid to go. You may possibly be missing a fantastic encounter!. Visit Site includes more about the meaning behind it.Cold Country Vines & Wines
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