To avoid making absolute measurements to determine film speed, it is convenient to refer to a group of film curves such
as those in Fig. 36(a). Curves positioned to the left of the chart require less exposure for a given density; those to the
right, more exposure. Thus, for a density of 2.0, film C in Fig. 36(a) is faster than film A, and both are faster than film B.
Their relative speed is calculated by determining the differences in log relative exposure and converting to the antilog.
Film B is the slowest film and requires a log relative exposure of 2.5 for a density of 2.0. Film B is chosen as the standard
and is assigned a speed of 100. Film A requires a log relative exposure of 1.9 for the same density. Subtracting 1.9 from
2.5 gives a difference of 0.6, for which the antilog is about 4, so the relative speed of film A is four times that of film B,
or has a relative speed of 400. Similarly, at a density of 2.0, film C requires a log relative exposure of 1.6. Subtracting 1.6
from 2.5 gives a log difference of 0.9, for which the antilog is about 8. Thus, film C is eight times faster than film B, or
has a relative speed of 800 at a density of 2.0.
Another advantage of using groups of characteristic curves is that the visual assessment of relative speeds can be easily
made. For example, although films A and B have similarly shaped curves running almost parallel, the curve for film C is
radically different. As calculated above, film C has a relative speed of 800 at a density of 2.0; however, at greater
densities, the relative speed of film C is lower than 800, and at lesser densities (down to a density of 1.0), the relative
speed of film C is greater than 800. Therefore, whenever relative speeds are used, the density at which they were
determined must be given.
Film gradient, also called film contrast, is a measure of the slope of the characteristic curve. If the difference is great,
the gradient (contrast) is said to be high. If the difference is slight, the gradient is said to be low. The contrast seen on a
radiograph is known as radiographic contrast and is composed of two factors:
•
Subject contrast, which is the result of variations in the amount of radiation absorbed by the testpiece
and which causes variations in radiation intensity impinging on the film
• Film gradient
(or film contrast), which is a measure of the response of the emulsion to the intensity of
impinging radiation and is a characteristic of a given film
Film gradient is determined from the characteristic curve by finding the slope of the curve at a given density. The slope of
the characteristic curve changes continuously over its entire length, as indicated in Fig. 36(a). The steeper the slope of the
curve over a range of relative exposures, the greater the difference in density and therefore the greater the resolution of
detail; thus, high gradient is important for good radiography.
In Fig. 36(b) tangents to a characteristic curve for a typical x-ray film have been drawn at two points, and the two
corresponding gradients (a/b and c/d) have been evaluated. Note that the gradient varies from 0.8 in the shallow portion of
the curve (called the toe) to 5 in the steeper portion of the curve.
Two regions of a testpiece that are slightly different in thicknesses will transmit slightly different intensities of radiation
to the film. On the characteristic curve, this would represent a small difference in the log relative exposure. For example,
assume that at a given kilovoltage the thinner section transmits 20% more radiation than the thicker section. The
difference in log relative exposure is 0.08 and is independent of tube current, exposure time, or source-to-film distance. In
the toe of the characteristic curve where, the gradient is only 0.8, the density difference is only 0.06, as indicated in Fig.
36(c). However, in the steeper portion of the curve where the gradient is 5, the density difference is 0.40. This effect of
film gradient is the main reason why it is best to use high exposures, obtaining the highest density that can be viewed on a
given illuminator for the greatest resolution of minor differences in transmitted radiation.
It is often more convenient to express gradient as an average over a given useful range of densities than for a single
density. This is a simple calculation in which the difference between the two densities is divided by the difference
between the log relative exposures for these densities; this ratio, known as the average gradient, is shown in Fig. 36(d).
Graininess. The silver halide grains that are contained in the emulsion of x-ray film are minute and can be seen only
with a high-power microscope, such as an electron microscope. Even though the emulsion on each side of the film is only
about 0.013 mm (0.0005 in.) thick, the grains are piled on top of each other in countless numbers. When the exposed-and-
processed radiograph is viewed, these small individual silver grains appear grouped together in relatively large masses.
This clumping, which is visible to the unaided eye or at low magnification, produces the visual impression called
graininess.