Open main menu
Home
Random
Recent changes
Special pages
Community portal
Preferences
About Wikipedia
Disclaimers
Incubator escapee wiki
Search
User menu
Talk
Dark mode
Contributions
Create account
Log in
Editing
Standard deviation
(section)
Warning:
You are not logged in. Your IP address will be publicly visible if you make any edits. If you
log in
or
create an account
, your edits will be attributed to your username, along with other benefits.
Anti-spam check. Do
not
fill this in!
===Rules for normally distributed data=== [[File:Standard deviation diagram.svg|thumb|Dark blue is one standard deviation on either side of the mean. For the normal distribution, this accounts for 68.27 percent of the set; while two standard deviations from the mean (medium and dark blue) account for 95.45 percent; three standard deviations (light, medium, and dark blue) account for 99.73 percent; and four standard deviations account for 99.994 percent. The two points of the curve that are one standard deviation from the mean are also the [[inflection point]]s.]] The [[central limit theorem]] states that the distribution of an average of many independent, identically distributed random variables tends toward the famous bell-shaped normal distribution with a [[probability density function]] of <math display="block">f\left(x, \mu, \sigma^2\right) = \frac{1}{\sigma\sqrt{2\pi}} e^{-\frac{1}{2}\left(\frac{x - \mu}{\sigma}\right)^2}</math> where {{mvar|μ}} is the [[expected value]] of the random variables, {{mvar|σ}} equals their distribution's standard deviation divided by {{math|{{var|n}}{{sup|{{frac|1|2}}}}}}, and {{mvar|n}} is the number of random variables. The standard deviation therefore is simply a scaling variable that adjusts how broad the curve will be, though it also appears in the [[normalizing constant]]. If a data distribution is approximately normal, then the proportion of data values within {{mvar|z}} standard deviations of the mean is defined by: <math display="block">\text{Proportion} = \operatorname{erf}\left(\frac{z}{\sqrt{2}}\right)</math> where <math>\textstyle\operatorname{erf}</math> is the [[error function]]. The proportion that is less than or equal to a number, {{mvar|x}}, is given by the [[cumulative distribution function]]:<ref>{{cite web |url= http://mathworld.wolfram.com/DistributionFunction.html |author= Eric W. Weisstein |title= Distribution Function |work=MathWorld |publisher=Wolfram |access-date= 30 September 2014}}</ref> <math display="block">\text{Proportion} \le x = \frac{1}{2}\left[1 + \operatorname{erf}\left(\frac{x - \mu}{\sigma\sqrt{2}}\right)\right] = \frac{1}{2}\left[1 + \operatorname{erf}\left(\frac{z}{\sqrt{2}}\right)\right].</math> If a data distribution is approximately normal then about 68 percent of the data values are within one standard deviation of the mean (mathematically, {{math|{{var|μ}} ± {{var|σ}}}}, where {{mvar|μ}} is the arithmetic mean), about 95 percent are within two standard deviations ({{math|{{var|μ}} ± 2{{var|σ}}}}), and about 99.7 percent lie within three standard deviations ({{math|{{var|μ}} ± 3{{var|σ}}}}). This is known as the ''[[68–95–99.7 rule]]'', or ''the empirical rule''. For various values of {{mvar|z}}, the percentage of values expected to lie in and outside the symmetric interval, {{math|{{var|CI}} {{=}} (−{{var|z}}{{var|σ}}, {{var|z}}{{var|σ}})}}, are as follows: [[File:Confidence interval by Standard deviation.svg|thumb|Percentage within(''z'')]] [[File:Standard deviation by Confidence interval.svg|thumb|''z''(Percentage within)]] {{anchor|Table}} {| class="wikitable" style="font-size: " |- ! rowspan=2 | Confidence <br />interval ! Proportion within ! colspan=2 | Proportion without |- ! Percentage ! Percentage ! Fraction |- | {{val|0.318639}}{{mvar|σ}} | 25% | 75% | 3 / 4 |- | {{val|0.674490}}{{mvar|σ}} | {{val|50}}% | {{val|50}}% | 1 / {{val|2}} |- | {{val|{{#expr:0.97792452561403 round 6}}}}{{mvar|σ}} | 66.6667% | 33.3333% | 1 / 3 |- | {{val|0.994458}}{{mvar|σ}} | 68% | 32% | 1 / 3.125 |- | 1{{mvar|σ}} | {{val|68.2689492}}% | {{val|31.7310508}}% | 1 / {{val|3.1514872}} |- | {{val|1.281552}}{{mvar|σ}} | 80% | 20% | 1 / 5 |- | {{val|1.644854}}{{mvar|σ}} | 90% | 10% | 1 / 10 |- | {{val|1.959964}}{{mvar|σ}} | 95% | 5% | 1 / 20 |- | 2{{mvar|σ}} | {{val|95.4499736}}% | {{val|4.5500264}}% | 1 / {{val|21.977895}} |- | {{val|2.575829}}{{mvar|σ}} | 99% | 1% | 1 / 100 |- | 3{{mvar|σ}} | {{val|99.7300204}}% | {{val|0.2699796}}% | 1 / 370.398 |- | {{val|3.290527}}{{mvar|σ}} | 99.9% | 0.1% | 1 / {{val|1000}} |- | {{val|3.890592}}{{mvar|σ}} | 99.99% | 0.01% | 1 / {{val|10000}} |- | 4{{mvar|σ}} | {{val|99.993666}}% | {{val|0.006334}}% | 1 / {{val|15787}} |- | {{val|4.417173}}{{mvar|σ}} | 99.999% | 0.001% | 1 / {{val|100000}} |- | {{val|4.5}}{{mvar|σ}} | {{gaps|99.999|320|465|3751%}} | {{gaps|0.000|679|534|6249%}} | 1 / {{val|147159.5358}}<br />6.8 / {{val|1000000}} |- | {{val|4.891638}}{{mvar|σ}} | {{val|99.9999}}% | {{val|0.0001}}% | 1 / {{val|1000000}} |- | 5{{mvar|σ}} | {{val|99.9999426697}}% | {{val|0.0000573303}}% | 1 / {{val|1744278}} |- | {{val|5.326724}}{{mvar|σ}} | {{val|99.99999}}% | {{val|0.00001}}% | 1 / {{val|10000000}} |- | {{val|5.730729}}{{mvar|σ}} | {{val|99.999999}}% | {{val|0.000001}}% | 1 / {{val|100000000}} |- | [[Six Sigma#Sigma levels|{{val|6}}{{mvar|σ}}]] | {{val|99.9999998027}}% | {{val|0.0000001973}}% | 1 / {{val|506797346}} |- | {{val|6.109410}}{{mvar|σ}} | {{val|99.9999999}}% | {{val|0.0000001}}% | 1 / {{val|1000000000}} |- | {{val|6.466951}}{{mvar|σ}} | {{val|99.99999999}}% | {{val|0.00000001}}% | 1 / {{val|10000000000}} |- | {{val|6.806502}}{{mvar|σ}} | {{val|99.999999999}}% | {{val|0.000000001}}% | 1 / {{val|100000000000}} |- | 7{{mvar|σ}} | {{gaps|99.999|999|999|7440%}} | {{val|0.000000000256}}% | 1 / {{val|390682215445}} |}
Edit summary
(Briefly describe your changes)
By publishing changes, you agree to the
Terms of Use
, and you irrevocably agree to release your contribution under the
CC BY-SA 4.0 License
and the
GFDL
. You agree that a hyperlink or URL is sufficient attribution under the Creative Commons license.
Cancel
Editing help
(opens in new window)