9b9a7b3f32
Now that the IPU3's Agc is derived from MeanLuminanceAgc we can delete all the unecessary bespoke functions. Reviewed-by: Jacopo Mondi <jacopo.mondi@ideasonboard.com> Reviewed-by: Stefan Klug <stefan.klug@ideasonboard.com> Signed-off-by: Daniel Scally <dan.scally@ideasonboard.com> Signed-off-by: Kieran Bingham <kieran.bingham@ideasonboard.com>
258 lines
8.0 KiB
C++
258 lines
8.0 KiB
C++
/* SPDX-License-Identifier: LGPL-2.1-or-later */
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/*
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* Copyright (C) 2021, Ideas On Board
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*
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* ipu3_agc.cpp - AGC/AEC mean-based control algorithm
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*/
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#include "agc.h"
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#include <algorithm>
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#include <chrono>
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#include <cmath>
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#include <libcamera/base/log.h>
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#include <libcamera/base/utils.h>
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#include <libcamera/control_ids.h>
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#include <libcamera/ipa/core_ipa_interface.h>
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#include "libipa/histogram.h"
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/**
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* \file agc.h
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*/
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namespace libcamera {
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using namespace std::literals::chrono_literals;
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namespace ipa::ipu3::algorithms {
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/**
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* \class Agc
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* \brief A mean-based auto-exposure algorithm
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*
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* This algorithm calculates a shutter time and an analogue gain so that the
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* average value of the green channel of the brightest 2% of pixels approaches
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* 0.5. The AWB gains are not used here, and all cells in the grid have the same
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* weight, like an average-metering case. In this metering mode, the camera uses
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* light information from the entire scene and creates an average for the final
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* exposure setting, giving no weighting to any particular portion of the
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* metered area.
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*
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* Reference: Battiato, Messina & Castorina. (2008). Exposure
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* Correction for Imaging Devices: An Overview. 10.1201/9781420054538.ch12.
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*/
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LOG_DEFINE_CATEGORY(IPU3Agc)
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/* Minimum limit for analogue gain value */
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static constexpr double kMinAnalogueGain = 1.0;
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/* \todo Honour the FrameDurationLimits control instead of hardcoding a limit */
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static constexpr utils::Duration kMaxShutterSpeed = 60ms;
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/* Histogram constants */
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static constexpr uint32_t knumHistogramBins = 256;
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Agc::Agc()
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: minShutterSpeed_(0s), maxShutterSpeed_(0s)
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{
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}
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/**
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* \brief Initialise the AGC algorithm from tuning files
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* \param[in] context The shared IPA context
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* \param[in] tuningData The YamlObject containing Agc tuning data
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*
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* This function calls the base class' tuningData parsers to discover which
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* control values are supported.
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*
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* \return 0 on success or errors from the base class
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*/
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int Agc::init(IPAContext &context, const YamlObject &tuningData)
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{
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int ret;
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ret = parseTuningData(tuningData);
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if (ret)
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return ret;
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context.ctrlMap.merge(controls());
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return 0;
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}
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/**
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* \brief Configure the AGC given a configInfo
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* \param[in] context The shared IPA context
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* \param[in] configInfo The IPA configuration data
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*
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* \return 0
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*/
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int Agc::configure(IPAContext &context,
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[[maybe_unused]] const IPAConfigInfo &configInfo)
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{
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const IPASessionConfiguration &configuration = context.configuration;
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IPAActiveState &activeState = context.activeState;
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stride_ = configuration.grid.stride;
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bdsGrid_ = configuration.grid.bdsGrid;
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minShutterSpeed_ = configuration.agc.minShutterSpeed;
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maxShutterSpeed_ = std::min(configuration.agc.maxShutterSpeed,
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kMaxShutterSpeed);
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minAnalogueGain_ = std::max(configuration.agc.minAnalogueGain, kMinAnalogueGain);
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maxAnalogueGain_ = configuration.agc.maxAnalogueGain;
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/* Configure the default exposure and gain. */
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activeState.agc.gain = minAnalogueGain_;
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activeState.agc.exposure = 10ms / configuration.sensor.lineDuration;
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context.activeState.agc.constraintMode = constraintModes().begin()->first;
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context.activeState.agc.exposureMode = exposureModeHelpers().begin()->first;
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/* \todo Run this again when FrameDurationLimits is passed in */
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setLimits(minShutterSpeed_, maxShutterSpeed_, minAnalogueGain_,
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maxAnalogueGain_);
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resetFrameCount();
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return 0;
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}
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Histogram Agc::parseStatistics(const ipu3_uapi_stats_3a *stats,
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const ipu3_uapi_grid_config &grid)
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{
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uint32_t hist[knumHistogramBins] = { 0 };
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rgbTriples_.clear();
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for (unsigned int cellY = 0; cellY < grid.height; cellY++) {
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for (unsigned int cellX = 0; cellX < grid.width; cellX++) {
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uint32_t cellPosition = cellY * stride_ + cellX;
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const ipu3_uapi_awb_set_item *cell =
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reinterpret_cast<const ipu3_uapi_awb_set_item *>(
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&stats->awb_raw_buffer.meta_data[cellPosition]);
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rgbTriples_.push_back({
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cell->R_avg,
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(cell->Gr_avg + cell->Gb_avg) / 2,
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cell->B_avg
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});
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/*
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* Store the average green value to estimate the
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* brightness. Even the overexposed pixels are
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* taken into account.
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*/
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hist[(cell->Gr_avg + cell->Gb_avg) / 2]++;
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}
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}
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return Histogram(Span<uint32_t>(hist));
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}
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/**
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* \brief Estimate the relative luminance of the frame with a given gain
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* \param[in] gain The gain to apply in estimating luminance
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*
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* The estimation is based on the AWB statistics for the current frame. Red,
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* green and blue averages for all cells are first multiplied by the gain, and
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* then saturated to approximate the sensor behaviour at high brightness
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* values. The approximation is quite rough, as it doesn't take into account
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* non-linearities when approaching saturation.
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*
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* The relative luminance (Y) is computed from the linear RGB components using
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* the Rec. 601 formula. The values are normalized to the [0.0, 1.0] range,
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* where 1.0 corresponds to a theoretical perfect reflector of 100% reference
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* white.
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*
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* More detailed information can be found in:
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* https://en.wikipedia.org/wiki/Relative_luminance
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*
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* \return The relative luminance of the frame
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*/
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double Agc::estimateLuminance(double gain) const
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{
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double redSum = 0, greenSum = 0, blueSum = 0;
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for (unsigned int i = 0; i < rgbTriples_.size(); i++) {
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redSum += std::min(std::get<0>(rgbTriples_[i]) * gain, 255.0);
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greenSum += std::min(std::get<1>(rgbTriples_[i]) * gain, 255.0);
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blueSum += std::min(std::get<2>(rgbTriples_[i]) * gain, 255.0);
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}
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double ySum = redSum * rGain_ * 0.299
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+ greenSum * gGain_ * 0.587
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+ blueSum * bGain_ * 0.114;
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return ySum / (bdsGrid_.height * bdsGrid_.width) / 255;
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}
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/**
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* \brief Process IPU3 statistics, and run AGC operations
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* \param[in] context The shared IPA context
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* \param[in] frame The current frame sequence number
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* \param[in] frameContext The current frame context
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* \param[in] stats The IPU3 statistics and ISP results
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* \param[out] metadata Metadata for the frame, to be filled by the algorithm
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*
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* Identify the current image brightness, and use that to estimate the optimal
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* new exposure and gain for the scene.
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*/
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void Agc::process(IPAContext &context, [[maybe_unused]] const uint32_t frame,
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IPAFrameContext &frameContext,
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const ipu3_uapi_stats_3a *stats,
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ControlList &metadata)
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{
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Histogram hist = parseStatistics(stats, context.configuration.grid.bdsGrid);
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rGain_ = context.activeState.awb.gains.red;
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gGain_ = context.activeState.awb.gains.blue;
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bGain_ = context.activeState.awb.gains.green;
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/*
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* The Agc algorithm needs to know the effective exposure value that was
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* applied to the sensor when the statistics were collected.
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*/
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utils::Duration exposureTime = context.configuration.sensor.lineDuration
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* frameContext.sensor.exposure;
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double analogueGain = frameContext.sensor.gain;
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utils::Duration effectiveExposureValue = exposureTime * analogueGain;
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utils::Duration shutterTime;
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double aGain, dGain;
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std::tie(shutterTime, aGain, dGain) =
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calculateNewEv(context.activeState.agc.constraintMode,
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context.activeState.agc.exposureMode, hist,
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effectiveExposureValue);
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LOG(IPU3Agc, Debug)
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<< "Divided up shutter, analogue gain and digital gain are "
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<< shutterTime << ", " << aGain << " and " << dGain;
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IPAActiveState &activeState = context.activeState;
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/* Update the estimated exposure and gain. */
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activeState.agc.exposure = shutterTime / context.configuration.sensor.lineDuration;
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activeState.agc.gain = aGain;
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metadata.set(controls::AnalogueGain, frameContext.sensor.gain);
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metadata.set(controls::ExposureTime, exposureTime.get<std::micro>());
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/* \todo Use VBlank value calculated from each frame exposure. */
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uint32_t vTotal = context.configuration.sensor.size.height
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+ context.configuration.sensor.defVBlank;
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utils::Duration frameDuration = context.configuration.sensor.lineDuration
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* vTotal;
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metadata.set(controls::FrameDuration, frameDuration.get<std::micro>());
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}
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REGISTER_IPA_ALGORITHM(Agc, "Agc")
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} /* namespace ipa::ipu3::algorithms */
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} /* namespace libcamera */
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