Files
dwarf-go/dwarfctl/internal/odometry/rotation.go
Jacquin Antoine d319ef6b4a Improve odometry with rotation estimation, daemon stability, and RTSP fixes
- Add rotation estimation via log-polar phase correlation (EstimateRotation,
  rotateGray) — de-rotate before translation to avoid aliasing
- Track cumulative field rotation in Tracker, reject low-confidence frames
- Extract RTSP grabber into internal/rtspgrab module
- Daemon: pause odometry during slew (motion blur), auto-resume after settle
  delay, add /pause and /resume HTTP endpoints, switch shooting mode before
  opening camera, use ReqOpenCamera with rtsp_encode_type=1
- WebSocket heartbeat (ping/pong every 10s) to prevent idle disconnects
- FFmpeg low-latency flags (-fflags nobuffer, -probesize, -analyzeduration)
- Add SendRaw API for custom payloads, increase daemon HTTP timeout to 60s

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2026-07-13 23:00:30 +02:00

188 lines
5.2 KiB
Go

package odometry
import (
"math"
"math/cmplx"
)
// EstimateRotation estimates the rotation angle (in degrees) between two
// grayscale matrices using the log-polar phase correlation method:
//
// 1. Compute the magnitude spectra |F1|, |F2| (rotation in spatial domain =
// rotation in frequency domain).
// 2. Apply a high-pass filter to suppress the DC-dominated center.
// 3. Resample to log-polar coordinates: rotation becomes a shift along the
// angular axis, scale becomes a shift along the log-radius axis.
// 4. Phase-correlate in log-polar space → the peak along the angular axis
// gives the rotation angle.
//
// Returns the rotation angle in degrees (positive = counter-clockwise rotation
// of the scene from g1 to g2), and a confidence in [0,1].
func EstimateRotation(g1, g2 [][]float64, rows, cols int) (angleDeg float64, conf float64) {
// 1. FFT both images.
a := windowedComplex(g1, rows, cols)
b := windowedComplex(g2, rows, cols)
fft2(a, false)
fft2(b, false)
// 2. Magnitude spectra with high-pass filtering.
magA := make([][]float64, rows)
magB := make([][]float64, rows)
cy, cx := float64(rows)/2, float64(cols)/2
maxR := math.Min(cy, cx)
for i := 0; i < rows; i++ {
magA[i] = make([]float64, cols)
magB[i] = make([]float64, cols)
for j := 0; j < cols; j++ {
// Shift zero-frequency to center (fftshift).
si := i
sj := j
if i < rows/2 {
si = i + rows/2
} else {
si = i - rows/2
}
if j < cols/2 {
sj = j + cols/2
} else {
sj = j - cols/2
}
ma := cmplx.Abs(a[si][sj])
mb := cmplx.Abs(b[si][sj])
// High-pass: suppress frequencies near DC.
dist := math.Sqrt(float64((float64(i)-cy)*(float64(i)-cy)) + float64((float64(j)-cx)*(float64(j)-cx)))
hp := 1.0 - math.Exp(-(dist*dist)/(2*(maxR*0.1)*(maxR*0.1)))
magA[i][j] = ma * hp
magB[i][j] = mb * hp
}
}
// 3. Resample magnitude spectra to log-polar coordinates.
nAngles := 256 // angular resolution
nRadii := 128 // radial resolution
lpA := logPolarResample(magA, rows, cols, nAngles, nRadii, maxR)
lpB := logPolarResample(magB, rows, cols, nAngles, nRadii, maxR)
// 4. Phase-correlate in log-polar space.
dx, dy, confRaw := phaseCorrelationFloat(lpA, lpB, nAngles, nRadii)
// dy is the shift along the angular axis → rotation angle.
// Each row in lpA/lpB corresponds to 360/nAngles degrees.
angleDeg = -float64(dy) * 360.0 / float64(nAngles)
// Wrap to [-180, 180)
for angleDeg < -180 {
angleDeg += 360
}
for angleDeg >= 180 {
angleDeg -= 360
}
_ = dx // log-radius shift (scale change) — not used for rotation-only estimation
conf = confRaw
return angleDeg, conf
}
// logPolarResample converts a Cartesian matrix to log-polar coordinates.
// The output has nAngles rows (angular samples) and nRadii columns (log-radius
// samples). This transforms a rotation in Cartesian space into a cyclic shift
// along the angular (row) axis.
func logPolarResample(mag [][]float64, rows, cols, nAngles, nRadii int, maxR float64) [][]float64 {
out := make([][]float64, nAngles)
cy, cx := float64(rows)/2, float64(cols)/2
logMinR := math.Log(2.0)
logMaxR := math.Log(maxR)
rStep := (logMaxR - logMinR) / float64(nRadii-1)
for a := 0; a < nAngles; a++ {
theta := 2 * math.Pi * float64(a) / float64(nAngles)
out[a] = make([]float64, nRadii)
for r := 0; r < nRadii; r++ {
radius := math.Exp(logMinR + float64(r)*rStep)
y := cy + radius*math.Sin(theta)
x := cx + radius*math.Cos(theta)
// Bilinear interpolation.
y0 := int(math.Floor(y))
x0 := int(math.Floor(x))
fy := y - float64(y0)
fx := x - float64(x0)
y0 = clampInt(y0, 0, rows-1)
x0 = clampInt(x0, 0, cols-1)
y1 := clampInt(y0+1, 0, rows-1)
x1 := clampInt(x0+1, 0, cols-1)
v := (1-fy)*(1-fx)*mag[y0][x0] +
(1-fy)*fx*mag[y0][x1] +
fy*(1-fx)*mag[y1][x0] +
fy*fx*mag[y1][x1]
out[a][r] = v
}
}
return out
}
// phaseCorrelationFloat is a float-based phase correlation (same algorithm as
// phaseCorrelation but operates on float64 matrices instead of complex, using
// its own internal FFT buffers).
func phaseCorrelationFloat(g1, g2 [][]float64, rows, cols int) (dx, dy, conf float64) {
a := windowedComplex(g1, rows, cols)
b := windowedComplex(g2, rows, cols)
fft2(a, false)
fft2(b, false)
r := make([][]complex128, rows)
for i := 0; i < rows; i++ {
r[i] = make([]complex128, cols)
for j := 0; j < cols; j++ {
cross := cmplx.Conj(a[i][j]) * b[i][j]
mag := cmplx.Abs(cross)
if mag > 1e-12 {
r[i][j] = cross / complex(mag, 0)
}
}
}
fft2(r, true)
px, py, peak := 0, 0, math.Inf(-1)
mean := 0.0
for i := 0; i < rows; i++ {
for j := 0; j < cols; j++ {
v := real(r[i][j])
mean += v
if v > peak {
peak = v
px, py = j, i
}
}
}
mean /= float64(rows * cols)
dx = float64(signedShift(px, cols))
dy = float64(signedShift(py, rows))
// Sub-pixel refinement.
dx += parabola(at2(r, py, px-1, cols), peak, at2(r, py, px+1, cols))
dy += parabola(at2(r, py-1, px, rows), peak, at2(r, py+1, px, rows))
denom := peak - mean
if denom > 1 {
denom = 1
}
if denom < 0 {
denom = 0
}
conf = denom
return dx, dy, conf
}
func clampInt(v, lo, hi int) int {
if v < lo {
return lo
}
if v > hi {
return hi
}
return v
}