Related
This normal distribution calculator helps you easily convert between cumulative probabilities and standard scores. It also allows you to calculate the area under the bell curve using a standard normal curve. Get ready to explore the world of normal distribution in depth with us. Let’s dive in!
In statistical terms:
“A normal distribution occurs when data points cluster around a central value and spread symmetrically without skewness.”
Here are some essential aspects of the normal distribution:
For quick calculations of these values, try our Mean, Median, Mode, Range Calculator.
The shape of a normal distribution is influenced by the standard deviation. Important rules include:
Visualize this concept using our Standard Normal Distribution Calculator.
The standard normal distribution is the most basic form of normal distribution, used as a reference for other distributions.
“A standard normal distribution is a special case where the mean is 0 and the standard deviation is 1.”
It is also called a z distribution, and z scores are used to standardize values. The total area under its curve equals 1. To use it, you convert any value x into its corresponding z score.
The standardization affects the curve’s width and position. Below is a table demonstrating different scenarios:
| Curve | Effect on Shape/Position |
| A (M = 0, SD = 1) | Standard normal curve |
| B (M = 0, SD = 0.5) | Compressed, narrower curve |
| C (M = 0, SD = 2) | Expanded, wider curve |
| D (M = 1, SD = 1) | Shifted right, mean > 0 |
| E (M = –1, SD = 1) | Shifted left, mean < 0 |
You can experiment with these behaviors using an online normal distribution calculator.
Several formulas are central to calculating probabilities with normal distributions:
The PDF gives the likelihood of a specific value x occurring:
$$ f(x) = \frac{1}{\sigma \sqrt{2\pi}} e^{-\frac{(x-\mu)^2}{2\sigma^2}} $$
For mean = 0 and 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 ≤ x:
$$ F(x;\mu,\sigma) = P(X \le x) = \frac{1}{\sigma \sqrt{2\pi}} \int_{-\infty}^{x} e^{-\frac{(t-\mu)^2}{2\sigma^2}} dt $$
It gives the value x corresponding to a probability p:
$$ F^{-1}(p) = \mu + \sigma \, \Phi^{-1}(p) $$
Or using the error function:
$$ F^{-1}(p) = \mu + \sigma \sqrt{2} \, \mathrm{erf}^{-1}(2p-1), \quad 0 < p < 1 $$
These formulas are implemented in advanced calculators to determine probabilities above, below, or between values in a normal distribution.
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 |
| 2.9 | 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 uses z-scores to calculate probabilities for values in a normal distribution.
With this calculator, you can easily find probabilities or values for a standard normal distribution in a few simple steps:
A standard normal variable is a normal random variable with a mean of 0 and a standard deviation of 1. It is commonly denoted by Z.
No. A Z-score shows how far a particular value is from the mean in terms of standard deviations. The standard deviation measures the overall spread of the dataset.
The normal distribution allows us to calculate probabilities for values in a population. By converting data into the standard normal form, we can find the likelihood that a value falls above, below, or between certain points.
Examples of normal distribution in daily life include:
The normal distribution is widely used because:
The normal distribution describes how values of a variable are spread around the mean. It models numerous natural and social phenomena, making it a cornerstone of probability and statistics. Using a normal distribution calculator helps perform accurate probability calculations efficiently.
Sources include Wikipedia: Normal distribution, Alternative parameterizations, Cumulative distribution functions, Quantile function, Symmetries and properties, Khan Academy: Qualitative understanding of normal distributions, Empirical Rule , Lumen Learning: Z-Scores, The Empirical Rule
Related
Links
Home Conversion Calculator About Calculator Online Blog Hire Us Knowledge Base Sitemap Sitemap TwoEmail us at
Contact Us© Copyrights 2026 by Calculator-Online.net