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The existing FAULTDIST result always considered every fault in the main grid. Users with many faults need to compute distance fields against a named subset, so this adds a Fault Distance Results collection under each view's Faults node. Each entry holds a multiselect of faults and a name (FAULTDIST1, FAULTDIST2, ...) and publishes the result into the Generated cell-result category. The per-cell BVH-based distance loop was extracted from RigFaultDistanceResultCalculator into a reusable utility that accepts the subset of faults to include; the original all-faults entry point delegates to the same utility and keeps the static-native FAULTDIST behavior unchanged.
36 lines
1.2 KiB
C++
36 lines
1.2 KiB
C++
/////////////////////////////////////////////////////////////////////////////////
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//
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// Copyright (C) 2026- Equinor ASA
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//
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// ResInsight is free software: you can redistribute it and/or modify
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// it under the terms of the GNU General Public License as published by
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// the Free Software Foundation, either version 3 of the License, or
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// (at your option) any later version.
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//
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// ResInsight is distributed in the hope that it will be useful, but WITHOUT ANY
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// WARRANTY; without even the implied warranty of MERCHANTABILITY or
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// FITNESS FOR A PARTICULAR PURPOSE.
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//
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// See the GNU General Public License at <http://www.gnu.org/licenses/gpl.html>
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// for more details.
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//
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/////////////////////////////////////////////////////////////////////////////////
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#pragma once
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#include <QString>
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#include <vector>
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class RigEclipseCaseData;
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class RigFault;
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//==================================================================================================
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///
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//==================================================================================================
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class RigSelectedFaultDistanceResultCalculator
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{
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public:
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static void compute( RigEclipseCaseData* caseData, const QString& resultName, const std::vector<const RigFault*>& selectedFaults );
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};
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