First construct a centred Gaussian process on the countable dyadic set with covariance function . These consistent finite-dimensional normal distributions exist because, for coefficients ,
the Kolmogorov extension theorem realizes them on one probability space. Every increment has the normal distribution , so for every finite ,
Use the preceding estimate with , and . It yields an almost surely Hölder continuous extension from the dense dyadic set to . Approximate arbitrary times by dyadic times; continuity of the paths and of the Gaussian covariance function preserves all finite-dimensional laws. Disjoint increments are jointly Gaussian with zero cross-covariances, hence independent, with the required variances. Together with and continuity, this constructs Brownian motion.
For any , choose large enough. Taking a countable increasing sequence of exponents tending to gives simultaneous Hölder regularity of every order on a common probability-one set; the same argument on each compact time interval gives local Brownian Hölder regularity. This method does not give the endpoint exponent. In fact that endpoint fails: if a path had a finite -Hölder seminorm , all its adjacent normalized increments at level would have magnitude at most . These are independent standard normal random variables, so for a fixed integer the probability that their maximum is at most is . The event of a finite is contained in the union over of events with this bound at every level, each of probability zero. Thus Brownian paths are not -Hölder continuous on almost surely.

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