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3.1.5  WHPT (Walley                                                        Dikerogammarus haemobaphes


            Hawkes Paisley Trigg)
            indices for older data sets



            WHPT is a development of BMWP. Like BMWP, it is
            expressed as an ASPT and Ntaxa. The main differences
            are that it includes more families, particularly of Diptera.
            BMWP-composite families are considered as separate
            families, each with their own index values, and different
            abundances of each taxon also have their own index
            values. This not only improves its accuracy, but allows it to
            respond to subtle pressures around the Good-Moderate
            status boundary that affect abundances before the
            taxonomic composition changes.


            WHPT was derived from an analysis of invertebrate data
            and BMWP-ASPT values from a very large data set of   Variations of the standard WHPT indices have been devised
            approximately 100,000 samples collected and analysed   so that it can be estimated from older data analysed to the
            by standard RIVPACS procedures (see Chapter 2). In its   level required for BMWP indices (ie RIVPACS Taxon level
            standard form, it is the basis for the UK’s river invertebrate   TL1), without records for abundance or the additional families
            (general degradation) status classification. Both the   used by WHPT but not by BMWP. Whereas the standard
            standard form of WHPT and the classification are   abundance-related version of WHPT ASPT can only be
            described in detail in Chapter 3.                 calculated from standard RIVPACS samples, the presence-
                                                              only version described below is suitable for samples
                                                              collected by other methods.

                                                              If abundance data is not available or the sample has not been
              WHPT – Walley Hawkes                            collected by standard RIVPACS methods you can estimate

              Paisley Trigg indices                           WHPT ASPT by using index values for the presence of taxa
                                                              termed ‘presence only’ or in RICT2 ‘non Ab’ index values.
                                                              Index values have also been devised for BMWP composite
              WHPT indices were developed from BMWP indices,   families (termed ‘CompFam’ in RICT2). These are listed
              which they replace. The most common form of WHPT   in the paper by Paisley et al. (2014)   and included on the
                                                                                         (41)
              uses abundance data but versions of WHPT have   WHPT calculator spreadsheet. These forms of WHPT ASPT
              been devised for use with older data sets without   are more accurate than BMWP ASPT, but they are not as
              abundance data or identified to the level used for   accurate as the abundance-related version of WHPT using
              BMWP indices. WHPT indices are more precise and   distinct (rather than composite) taxa and they must not be
              more accurate than BMWP and are therefore better   used to determine WFD status class. Being on the same
              able to detect nutrient and other mild pressures.  scale, these forms of WHPT ASPT are comparable with
                                                              the standard form of WHPT ASPT, but WHPT NTaxa is only
                                                              comparable if it is based on the same group of taxa.



























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