This results in the need for a high-sensitivity light receiver or a changeable amount of light illuminating the scattering volume. The next problem is to balance the capacity of the scattering volume. If the scattering volume is too small, then the small number of big particles flowing through the light beam causes the measured signal
to be unstable. On the other hand, selleck compound a large scattering volume capacity leads to decreasing angular resolution, or else requires a larger instrument (see Petzold 1972). Another problem is to obtain as wide a range of angles as possible. When light is scattered into small forward angles it is difficult to distinguish between the scattered light and the illuminating beam. That is why the so-called small angle problem can be solved by using a separate instrument. This was the way chosen by Petzold (1972), and nowadays this can be done on a modern instrument (see Slade & Boss 2006). On the IDH activation other hand, when the light receiver moves close to 180° it shades the illuminating beam and limits the
range of measurement. Because of these limitations a typical polar nephelometer can measure the VSF from 5° or 6° to about 170°. This is the range covering at least 50% of the scattered light. a review of many known constructions will be found in Jonasz & Fournier (2007). The largest range of scattering angles was obtained with a prototypical version of the Multispectral Volume Scattering Meter Thalidomide (MVSM) (see Lee & Lewis 2003). Because this instrument uses a rotational prism of special shape, the unusual range from 0.5° to 179° with a 0.25° step was obtained. Unfortunately, because of the uniqueness of measurements made with the MVSM, the variability of VSFs is still poorly known. That is why even partial information
about the scattering properties of sea water is very valuable. There are a few optical properties of a medium that can be calculated from the VSF. The first is the scattering coefficient, which describes the fraction of light that changes direction per unit of length of its propagation. Operationally, it is the VSF integrated over all directions. But nowadays in sea water the scattering coefficient is usually obtained as the difference between the attenuation and absorption coefficients (measured by ac-9 or ac-s (WET Labs)). Another of these properties is the backscattering coefficient bb, which is the VSF integrated over the backward hemisphere. Knowledge of bb is very important because of its relation to remote sensing reflectance ( Gordon et al. 1988). The above difficulties persuaded researchers to look for a simplified method of obtaining these values. The first such attempt was by Jerlov (1953), who tried to establish a link between the scattering coefficient b and scattering into the 45° angle. His dependence turned out to be erroneous, however, because at least 50% of the light is scattered into angles smaller than 5°.
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