J.H. Michell solved in 1898 the problem of a thin ship moving steadily forward in a calm sea, and was able, in spite of the
total absence of computing equipment, to evaluate with 2-figure accuracy the triple integral for the resulting inviscid drag
force or wave resistance. Michell’s formulation allowed in principle determination of the actual ship-wave pattern, but this
task was not completed
... [Show full abstract] for the whole wave field for about another century. Far-field waves can be computed with only marginally
more difficulty than wave resistance, and some such computations appeared a few decades ago, but even then there are subtleties
and fine details such as very short diverging waves that are difficult to capture with adequate accuracy. Waves near the ship
are an order of magnitude harder to compute. We have produced very fast code for both near and far fields, that can determine
a finely detailed pattern in about an hour on an inexpensive PC, a task that J.H. Michell would no doubt have carried out
himself if he had such a device on his desk in 1898. A feature that Michell might not have included is an empirical dissipation
factor for the far-field waves, incorporating an eddy viscosity coefficient which damps out some of the shortest diverging
waves. Results are given for a destroyer hull where agreement with experiment is reasonable, and in particular is not necessarily
worse than that for codes incorporating features such as nonlinearity and full viscous effects.