Strategies for modelling seismic refraction/wide-angle reflection traveltim
es to obtain 2-D velocity and interface structure are presented along with
methods for assessing the reliability of the results. Emphasis is placed on
using inverse methods, but a discussion of arrival picking and classificat
ion, data uncertainties, traveltime reciprocity, crooked line geometry and
the selection of a starting model is also applicable to trial-and-error for
ward modelling. The most important advantages of an inverse method are the
ability to derive simpler models for the appropriate level of fit to the da
ta, and the ability to assess the final model in terms of resolution, param
eter bounds and non-uniqueness. Given the unique characteristics of each da
ta set and the local earth structure, there is no single approach to modell
ing wide-angle data that is best. This paper describes the best modelling s
trategies according to (1) the model parametrization, (2) the inclusion of
prior information, (3) the complexity of the earth structure, (4) the chara
cteristics of the data, and (5) the utilization of coincident seismic refle
ction data. There are two natural end-member inversion styles: (1) a regula
r, fine-grid parametrization when seeking a minimum-structure model, and (2
) an irregular grid, minimum-parameter model when considering certain forms
of prior information. The former style represents the 'pure' tomography ap
proach. The latter style is closer to automated forward modelling, and can
be applied best with a parameter-selective algorithm, that is, one that all
ows any subset of model parameters to be selected for inversion. If there i
s strong lateral heterogeneity in the near-surface only, layer stripping wo
rks well. If there is complexity at all depths, all model parameters should
be determined simultaneously after careful construction of a starting mode
l that allows the appropriate rays to be traced to all pick locations. The
lateral spacing of model nodes to use will depend on the type of inversion
and whether detailed prior information is included, but a general guideline
based on model resolution when seeking a minimum-parameter model is a mode
l node spacing equal to the shot spacing (receiver spacing for typical mari
ne data), except perhaps in the upper layers where about half this may be n
ecessary; node spacing is not an issue when using smoothing constraints, pr
ovided it is small enough to resolve the earth structure of interest. Trave
ltimes picked from pre-stack, unmigrated or migrated coincident reflection
data can be (1) used to develop the starting model, (2) inverted simultaneo
usly with the wide-angle data, or (3) inverted after modelling the wide-ang
le data to constrain interfaces that 'float' within the velocity model. Mod
el assessment establishes the reliability of the final model. Presenting mo
del statistics, traveltime fits, ray diagrams and resolution kernels is use
ful, but can only indirectly address this issue. Direct model assessment te
chniques that derive alternative models that satisfactorily fit the real da
ta are the best means of establishing the absolute bounds on model paramete
rs and whether a particular model feature is required by the data.