This normal distribution calculator assists you to do to and fro calculations among cumulative probability and standard random variable. Also, you could now determine the area under the bell curve by subjecting this standard normal curve calculator. So tie your seat belts to go on a ride of normal distribution concept in more depth with us. Let's Continue!
In the context of statistical analysis:
“When data points are distributed closely around a central value with no bias to either side, this distribution is known as the normal distribution.”
Here are some key facts about the normal distribution:
To quickly determine these values, you can use our Mean, Median, Mode, Range Calculator.
The normal distribution is closely related to the standard deviation. Here are the key points to remember:
You can visualize this using a Standard Normal Distribution Calculator.
The whole statistics are represented by pictorial diagram as under:
It's a most generic form of the data distribution from which the normal distribution is itself dragged out.
“A special type of distribution of data in which the mean value becomes 0 and standard deviation becomes 1 is known as the standard deviation.”
Another name used for the phenomenon is z distribution that is calculated by z score. For a standard normal distribution, the overall area under a bell curve would be equal to 1. Also, you must convert the value of variable x into a z score.
The standard distribution contracts or expands the curve of a normal distribution. Below we have a table along with its pictorial representation that display the effect that we are actually discussing.
|
Curve |
Position or shape (relative to standard normal distribution) |
| A (M = 0, SD = 1) |
Standard normal distribution |
|
B (M = 0, SD = 0.5) |
Squeezed, because SD < 1 |
| C (M = 0, SD = 2) |
Stretched, because SD > 1 |
|
D (M = 1, SD = 1) |
Shifted right, because M > 0 |
| E (M = –1, SD = 1) |
Shifted left, because M < 0 |
You can also analyze these behaviors quickly using an online normal distribution calculator.
Several key formulas are used in normal distribution calculations:
The PDF gives the probability density at a specific value x:
$$ f(x) = \frac{1}{\sigma \sqrt{2\pi}} e^{-\frac{(x-\mu)^2}{2\sigma^2}} $$
For a standard normal distribution (mean = 0, standard deviation = 1):
$$ f(x) = \frac{1}{\sqrt{2\pi}} e^{-\frac{x^2}{2}} $$
The CDF calculates the probability that a random variable X is less than or equal to x:
$$ F(x;\mu,\sigma) = P(X \le x) = \frac{1}{\sigma \sqrt{2\pi}} \int_{-\infty}^{x} e^{-\frac{(t-\mu)^2}{2\sigma^2}} \, dt $$
The inverse CDF (or quantile function) gives the value of x for a given probability p:
$$ F^{-1}(p) = \mu + \sigma \, \Phi^{-1}(p) $$
Alternatively, using the error function:
$$ F^{-1}(p) = \mu + \sigma \sqrt{2} \, \mathrm{erf}^{-1}(2p-1), \quad p \in (0, 1) $$
All of these formulas are implemented in advanced normal distribution calculators to determine probabilities for events above or below the mean.
The standard normal distribution table (z-table) is used to calculate probabilities for z-scores. It allows you to determine the probability of a random variable being above or below a certain value relative to the mean. This is essential for hypothesis testing, confidence intervals, and statistical inference.
| z | 0 | 0.01 | 0.02 | 0.03 | 0.04 | 0.05 | 0.06 | 0.07 | 0.08 | 0.09 |
| 0 | 0 | 0.00399 | 0.00798 | 0.01197 | 0.01595 | 0.01994 | 0.02392 | 0.0279 | 0.03188 | 0.03586 |
| 0.1 | 0.03983 | 0.0438 | 0.04776 | 0.05172 | 0.05567 | 0.05962 | 0.06356 | 0.06749 | 0.07142 | 0.07535 |
| 0.2 | 0.07926 | 0.08317 | 0.08706 | 0.09095 | 0.09483 | 0.09871 | 0.10257 | 0.10642 | 0.11026 | 0.11409 |
| 0.3 | 0.11791 | 0.12172 | 0.12552 | 0.1293 | 0.13307 | 0.13683 | 0.14058 | 0.14431 | 0.14803 | 0.15173 |
| 0.4 | 0.15542 | 0.1591 | 0.16276 | 0.1664 | 0.17003 | 0.17364 | 0.17724 | 0.18082 | 0.18439 | 0.18793 |
| 0.5 | 0.19146 | 0.19497 | 0.19847 | 0.20194 | 0.2054 | 0.20884 | 0.21226 | 0.21566 | 0.21904 | 0.2224 |
| 0.6 | 0.22575 | 0.22907 | 0.23237 | 0.23565 | 0.23891 | 0.24215 | 0.24537 | 0.24857 | 0.25175 | 0.2549 |
| 0.7 | 0.25804 | 0.26115 | 0.26424 | 0.2673 | 0.27035 | 0.27337 | 0.27637 | 0.27935 | 0.2823 | 0.28524 |
| 0.8 | 0.28814 | 0.29103 | 0.29389 | 0.29673 | 0.29955 | 0.30234 | 0.30511 | 0.30785 | 0.31057 | 0.31327 |
| 0.9 | 0.31594 | 0.31859 | 0.32121 | 0.32381 | 0.32639 | 0.32894 | 0.33147 | 0.33398 | 0.33646 | 0.33891 |
| 1 | 0.34134 | 0.34375 | 0.34614 | 0.34849 | 0.35083 | 0.35314 | 0.35543 | 0.35769 | 0.35993 | 0.36214 |
| 1.1 | 0.36433 | 0.3665 | 0.36864 | 0.37076 | 0.37286 | 0.37493 | 0.37698 | 0.379 | 0.381 | 0.38298 |
| 1.2 | 0.38493 | 0.38686 | 0.38877 | 0.39065 | 0.39251 | 0.39435 | 0.39617 | 0.39796 | 0.39973 | 0.40147 |
| 1.3 | 0.4032 | 0.4049 | 0.40658 | 0.40824 | 0.40988 | 0.41149 | 0.41308 | 0.41466 | 0.41621 | 0.41774 |
| 1.4 | 0.41924 | 0.42073 | 0.4222 | 0.42364 | 0.42507 | 0.42647 | 0.42785 | 0.42922 | 0.43056 | 0.43189 |
| 1.5 | 0.43319 | 0.43448 | 0.43574 | 0.43699 | 0.43822 | 0.43943 | 0.44062 | 0.44179 | 0.44295 | 0.44408 |
| 1.6 | 0.4452 | 0.4463 | 0.44738 | 0.44845 | 0.4495 | 0.45053 | 0.45154 | 0.45254 | 0.45352 | 0.45449 |
| 1.7 | 0.45543 | 0.45637 | 0.45728 | 0.45818 | 0.45907 | 0.45994 | 0.4608 | 0.46164 | 0.46246 | 0.46327 |
| 1.8 | 0.46407 | 0.46485 | 0.46562 | 0.46638 | 0.46712 | 0.46784 | 0.46856 | 0.46926 | 0.46995 | 0.47062 |
| 1.9 | 0.47128 | 0.47193 | 0.47257 | 0.4732 | 0.47381 | 0.47441 | 0.475 | 0.47558 | 0.47615 | 0.4767 |
| 2 | 0.47725 | 0.47778 | 0.47831 | 0.47882 | 0.47932 | 0.47982 | 0.4803 | 0.48077 | 0.48124 | 0.48169 |
| 2.1 | 0.48214 | 0.48257 | 0.483 | 0.48341 | 0.48382 | 0.48422 | 0.48461 | 0.485 | 0.48537 | 0.48574 |
| 2.2 | 0.4861 | 0.48645 | 0.48679 | 0.48713 | 0.48745 | 0.48778 | 0.48809 | 0.4884 | 0.4887 | 0.48899 |
| 2.3 | 0.48928 | 0.48956 | 0.48983 | 0.4901 | 0.49036 | 0.49061 | 0.49086 | 0.49111 | 0.49134 | 0.49158 |
| 2.4 | 0.4918 | 0.49202 | 0.49224 | 0.49245 | 0.49266 | 0.49286 | 0.49305 | 0.49324 | 0.49343 | 0.49361 |
| 2.5 | 0.49379 | 0.49396 | 0.49413 | 0.4943 | 0.49446 | 0.49461 | 0.49477 | 0.49492 | 0.49506 | 0.4952 |
| 2.6 | 0.49534 | 0.49547 | 0.4956 | 0.49573 | 0.49585 | 0.49598 | 0.49609 | 0.49621 | 0.49632 | 0.49643 |
| 2.7 | 0.49653 | 0.49664 | 0.49674 | 0.49683 | 0.49693 | 0.49702 | 0.49711 | 0.4972 | 0.49728 | 0.49736 |
| 2.8 | 0.49744 | 0.49752 | 0.4976 | 0.49767 | 0.49774 | 0.49781 | 0.49788 | 0.49795 | 0.49801 | 0.49807 |
| 2.9 | 0.49813 | 0.49819 | 0.49825 | 0.49831 | 0.49836 | 0.49841 | 0.49846 | 0.49851 | 0.49856 | 0.49861 |
| 3 | 0.49865 | 0.49869 | 0.49874 | 0.49878 | 0.49882 | 0.49886 | 0.49889 | 0.49893 | 0.49896 | 0.499 |
| 3.1 | 0.49903 | 0.49906 | 0.4991 | 0.49913 | 0.49916 | 0.49918 | 0.49921 | 0.49924 | 0.49926 | 0.49929 |
| 3.2 | 0.49931 | 0.49934 | 0.49936 | 0.49938 | 0.4994 | 0.49942 | 0.49944 | 0.49946 | 0.49948 | 0.4995 |
| 3.3 | 0.49952 | 0.49953 | 0.49955 | 0.49957 | 0.49958 | 0.4996 | 0.49961 | 0.49962 | 0.49964 | 0.49965 |
| 3.4 | 0.49966 | 0.49968 | 0.49969 | 0.4997 | 0.49971 | 0.49972 | 0.49973 | 0.49974 | 0.49975 | 0.49976 |
| 3.5 | 0.49977 | 0.49978 | 0.49978 | 0.49979 | 0.4998 | 0.49981 | 0.49981 | 0.49982 | 0.49983 | 0.49983 |
| 3.6 | 0.49984 | 0.49985 | 0.49985 | 0.49986 | 0.49986 | 0.49987 | 0.49987 | 0.49988 | 0.49988 | 0.49989 |
| 3.7 | 0.49989 | 0.4999 | 0.4999 | 0.4999 | 0.49991 | 0.49991 | 0.49992 | 0.49992 | 0.49992 | 0.49992 |
| 3.8 | 0.49993 | 0.49993 | 0.49993 | 0.49994 | 0.49994 | 0.49994 | 0.49994 | 0.49995 | 0.49995 | 0.49995 |
| 3.9 | 0.49995 | 0.49995 | 0.49996 | 0.49996 | 0.49996 | 0.49996 | 0.49996 | 0.49996 | 0.49997 | 0.49997 |
| 4 | 0.49997 | 0.49997 | 0.49997 | 0.49997 | 0.49997 | 0.49997 | 0.49998 | 0.49998 | 0.49998 | 0.49998 |
This standard normal table calculator also uses z-score values to determine probabilities for normal distributions.
This normal distribution calculator allows you to quickly compute probabilities or values for the standard normal distribution in just a few steps:
A standard normal random variable is a normally distributed variable with a mean of 0 and a standard deviation of 1. It is always represented by the letter Z.
No. The Z-score indicates how many standard deviations a particular value is away from the mean. The standard deviation, on the other hand, measures the overall variability or spread of the dataset.
The normal distribution is used to calculate probabilities for a population. By transforming data into a standard normal distribution, we can determine the likelihood that a value falls above or below a certain point.
Some practical examples of the normal distribution include:
The normal distribution is a good model for many random variables because:
The normal distribution describes how the values of a variable are spread. It accurately models many natural and social phenomena, making it one of the most important probability distributions in statistics. For calculating precise probabilities and working with normal distributions, using a dedicated normal distribution calculator can save time and improve accuracy.
From the source of wikipedia: Normal distribution, Alternative parameterizations, Cumulative distribution functions, Quantile function, Properties, Symmetries and derivatives, From the source of khan academy: Qualitative sense of normal distributions, Empirical rule From the source of lumen learning: Z-Scores, The Empirical Rule
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