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In this note, we combine the two approaches of Billingsley (1998) andCs\H{o}rg\H{o} and R\'ev\'esz (1980), to provide a detailed sequential anddescriptive for creating s standard Brownian motion, from a Brownian motionwhose time space is the class of non-negative dyadic numbers. By adding theproof of Etemadi's inequality to text, it becomes self-readable and serves asan independent source for researches and professors.

A direct construction of the Standard Brownian Motion