The Brownian reflection principle gives, for ,
For a standard normal random variable , this is also . Thus the inverse-square Gaussian law of Brownian first passage is
In particular, is finite almost surely.
The Brownian motions are independent, so conditional on , the ordinate has the same distribution as , with a standard normal independent of the random time. By Brownian scaling and the hitting-time identity,
The last equality uses symmetry of and independence of : inserting the independent sign of does not change the distribution of the numerator. Therefore
For completeness, the ratio has density , where is the standard normal density. The scaled exit ordinate has density .

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