satdump/src-core/common/image/earth_curvature.cpp
2023-12-13 22:05:03 -05:00

99 lines
No EOL
5.1 KiB
C++

#include "earth_curvature.h"
#include <cmath>
namespace image
{
namespace earth_curvature
{
const float EARTH_RADIUS = 6371.0f;
/*
This was mostly based off the following document :
https://web.archive.org/web/20200110090856if_/http://ceeserver.cee.cornell.edu:80/wdp2/cee6150/Monograph/615_04_GeomCorrect_rev01.pdf
*/
template <typename T>
Image<T> correct_earth_curvature(Image<T> &image, float satellite_height, float swath, float resolution_km, float *foward_table)
{
float satellite_orbit_radius = EARTH_RADIUS + satellite_height; // Compute the satellite's orbit radius
int corrected_width = round(swath / resolution_km); // Compute the output image size, or number of samples from the imager
float satellite_view_angle = swath / EARTH_RADIUS; // Compute the satellite's view angle
float edge_angle = -atanf(EARTH_RADIUS * sinf(satellite_view_angle / 2) / ((cosf(satellite_view_angle / 2)) * EARTH_RADIUS - satellite_orbit_radius)); // Max angle relative to the satellite
float *correction_factors = new float[corrected_width]; // Create a LUT to avoid recomputing on each row
// Generate them
for (int i = 0; i < corrected_width; i++)
{
float angle = ((float(i) / float(corrected_width)) - 0.5f) * satellite_view_angle; // Get the satellite's angle
float satellite_angle = -atanf(EARTH_RADIUS * sinf(angle) / ((cosf(angle)) * EARTH_RADIUS - satellite_orbit_radius)); // Convert to an angle relative to earth
correction_factors[i] = image.width() * ((satellite_angle / edge_angle + 1.0f) / 2.0f); // Convert that to a pixel from the original image
}
Image<T> output_image(corrected_width, image.height(), image.channels()); // Allocate output image
if (foward_table != nullptr)
for (int i = 0; i < (int)image.width(); i++)
foward_table[i] = -1;
for (int channel = 0; channel < image.channels(); channel++)
{
int channel_offset = channel * (image.width() * image.height());
int channel_offset_output = channel * (output_image.width() * output_image.height());
// Process each row
#pragma omp parallel for
for (int row = 0; row < (int)image.height(); row++)
{
for (int i = 0; i < corrected_width; i++)
{
#if 1
// printf("%d %f %f %d %d\n", i, correction_factors[i], fmod(correction_factors[i], 1), (int)correction_factors[i], (int)correction_factors[i] + 1);
int currPixel = correction_factors[i];
int nextPixel = correction_factors[i] + 1;
float fractionalPx = fmod(correction_factors[i], 1);
if ((size_t)nextPixel >= image.width())
nextPixel = image.width() - 1;
int px1 = image[channel_offset + row * image.width() + currPixel];
int px2 = image[channel_offset + row * image.width() + nextPixel];
int px = px1 * (1.0 - fractionalPx) + px2 * fractionalPx;
output_image[channel_offset_output + row * corrected_width + i] = px;
if (foward_table != nullptr)
foward_table[currPixel] = i;
#else
int pixel_to_use = correction_factors[i]; // Input pixel to use, will get rounder automatically
output_image[channel_offset_output + row * corrected_width + i] = image[channel_offset + row * image.width() + pixel_to_use]; // Copy over that pixel!
if (foward_table != nullptr)
foward_table[pixel_to_use] = i;
#endif
}
}
}
if (foward_table != nullptr)
{
float last_val = 0;
for (int i = 0; i < (int)image.width(); i++)
{
if (foward_table[i] == -1)
foward_table[i] = last_val;
last_val = foward_table[i];
}
}
// Maybe we could do some more smoothing after the fact?
// Will see later.
delete[] correction_factors;
return output_image;
}
template Image<uint8_t> correct_earth_curvature<uint8_t>(Image<uint8_t> &, float, float, float, float *);
template Image<uint16_t> correct_earth_curvature<uint16_t>(Image<uint16_t> &, float, float, float, float *);
}
}