Effective strip width (ESW) of a distance function is its
integral. That is, ESW is the area under the distance function from its
left-truncation limit (obj$w.lo
) to its right-truncation limit
(obj$w.hi
).
Under perfect detection, area under the detection function is the entire
half-width of
the strip transect (from obj$w.lo
to obj$w.hi
).
Under perfect detection, density is the number sighted targets
divided by area surveyed, where area surveyed is
obj$w.hi-obj$w.lo
times
total length of transects.
When detection is not perfect, less than the total half-width is
effectively covered. Buckland et al. (1993) show that the
denominator of the density estimator in this case involves total length of
surveyed transects times area under the detection function (i.e., this
integral). By analogy with the perfect detection case, this integral can
be viewed as the transect half-width that observers effectively
cover. In other words, a survey with imperfect detection and ESW equal to X
effectively covers the same area as a study with perfect detection out to a
distance of X.
The trapezoid rule is used to numerically integrate under the distance
function in obj
from obj$w.lo
to obj$w.hi
. Two-hundred
trapezoids are used in the approximation to speed calculations. In some
rare cases, two hundred trapezoids may not be enough. In these cases, the
code for this function can be sink
-ed to a file, inspected in a text
editor, modified to bump the number of trapezoids, and source
-d back
in.