Hit-accumulation clutter filter: HAC
By summing all polar bins in a scan with a uniquely-defined geoometry, the frequency of detection can be used as a criterion for determining whether a given bin is contaminated by clutter. Frequency of detection is thresholded hit accumulation, which is used to remove clutter and store it in a separate quality indicator field.
See references below.
Michelson D. and Henja A., 2013: OPERA WP3.6, Task #4. Implementation of hit-accumulation clutter filter in BALTRAD toolbox. EUMETNET OPERA Working document WD_2012_02p. 8 pp.
Scovell R., 2012: OPERA WP 3.6 Task #2 Evaluation of the Odyssey Clutter Removal Technique Using Radar vs. Gauge Comparisons Over the UK. EUMETNET OPERA Working document WD_2012_02f. 53 pp.
No optional ‘how’ attributes are required.
Polar scans (/what/object=SCAN) containing horizontal reflectivity (DBZH) are the basis for this algorithm, although other quantities can also be used. Polar volumes are also input; their scans are treated individually. No previous QC step need have been applied.
The algorithm has two steps:
The output reflectivities are the same data type as the input.
A quality field containing the filtered reflectivities is written. This field has the same data type as the original quantity.
The identifier for this algorithm, written to the quality indicator’s how/task attribute is “eu.opera.odyssey.hac”.