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wradlib Documentation - Bitbucket

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<strong>wradlib</strong> <strong>Documentation</strong>, Release 0.1.1<br />

Now we have everything we need for the accumulation:<br />

accum_data = wrl.util.aggregate_in_time(data_R_depth, times, accum_times)<br />

wrl.vis.polar_plot(accum_data[0], title = ’Precipitation height 18.8.2006, 00:05-01:05 (Radarstation<br />

unit = ’mm’, colormap = ’spectral’, vmax = max(accum_data))<br />

wrl.vis.polar_plot(accum_data[1], title = ’Precipitation height 18.8.2006, 01:05-02:05 (Radarstation<br />

unit = ’mm’, colormap = ’spectral’, vmax = max(accum_data))<br />

.. image:: images/precip_movie.gif<br />

All raw data is provided by DWD<br />

2.6 Clutter correction<br />

Weather radar data with clutter (static and dynamic echos, not caused by precipitation) can be disastrously if used for<br />

hydrological rainfall-runoff modeling or related to attenuation correction of non-coherent radar data. So in most cases<br />

it is indispensable to detect and remove clutter bins from your radar data.<br />

The <strong>wradlib</strong> function histo_cut is an histogram based clutter identification algorithm. It classifies an (preferential<br />

yearly based) precipitation accumulation of radar data into 50 classes and removes iteratively framing classes which<br />

undercut 1% of the class with the highest frequency.<br />

In a first step you need an radar-image with an representative accumulation timespan, so that precipitation is distributed<br />

evenly over the image. As for example this philipinean image, where the scale extend shows us definitely the occurance<br />

of clutter:<br />

2.6. Clutter correction 29

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