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Add rtp3d.jl
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src/rtp3d.jl

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# rtp3d.jl — reduce a magnetic field anomaly grid to the pole via 2-D Fourier transform, given the
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# inclination/declination of the field and of the magnetization (port of Mirone/M.A.Tivey's
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# utils/rtp3d.m, 1992/1994). Can also isolate the X (north), Y (east) or Z (up) component instead
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# of doing a full RTP. The 2-D FFT is built from GMT.jl's own `fft1d` (GMT_FFT_1D), applied
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# row-wise then column-wise — no FFTW.jl, no in-house FFT (same convention as xyanalysis.jl's 1-D
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# case: everything Fourier goes through the GMT library).
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"""
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fout, k = rtp3d(f3d, incl_fld, decl_fld, incl_mag, decl_mag; component=0)
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Reduce a magnetic field anomaly map `f3d` to the pole, given the inclination/declination (degrees)
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of the ambient field (`incl_fld`, `decl_fld`) and of the magnetization (`incl_mag`, `decl_mag`).
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`component` selects an alternative output instead of the plain RTP: `1` = X/North, `2` = Y/East,
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`3` = Z/Up component. Default `0` is the RTP.
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Returns the transformed grid `fout` and the wavenumber array `k`.
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"""
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function rtp3d(f3d::Matrix{<:Real}, incl_fld::Real, decl_fld::Real, incl_mag::Real, decl_mag::Real;
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component::Integer=0)
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_rtp3d(Float64.(f3d), Float64(incl_fld), Float64(decl_fld), Float64(incl_mag), Float64(decl_mag), Int(component))
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end
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# Annotate all inputs because Julia recompiles everything if a single input type changes.
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function _rtp3d(f3d::Matrix{Float64}, incl_fld::Float64, decl_fld::Float64, incl_mag::Float64, decl_mag::Float64,
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component::Int)
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D2R = pi / 180
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incl_fld *= D2R; decl_fld *= D2R
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incl_mag *= D2R; decl_mag *= D2R
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ny, nx = size(f3d)
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x = collect((-0.5):(1/nx):(0.5 - 1/nx))
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y = collect((-0.5):(1/ny):(0.5 - 1/ny))
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X = Matrix{Float64}(undef, ny, nx)
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Y = Matrix{Float64}(undef, ny, nx)
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@inbounds for c = 1:nx, r = 1:ny
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X[r, c] = x[c]
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Y[r, c] = y[r]
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end
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k = 2pi .* sqrt.(X.^2 .+ Y.^2) # wavenumber array
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aux = atan.(Y, X) # auxiliary angle, computed once (as in the .m)
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# ------ geometric and amplitude factors
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Ob = sin(incl_fld) .+ im .* cos(incl_fld) .* sin.(aux .+ decl_fld)
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O = if (abs(incl_fld - incl_mag) > 0.03 || abs(decl_fld - decl_mag) > 0.03 || component != 0) # 0.03 rad is < 2 deg
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Om = sin(incl_mag) .+ im .* cos(incl_mag) .* sin.(aux .+ decl_mag)
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Ob .* Om
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else
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Ob .* Ob
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end
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if (component != 0) # X, Y or Z component instead of a plain RTP
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new_inc, new_dec = component == 1 ? (0.0, 0.0) :
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component == 2 ? (0.0, 90.0) :
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component == 3 ? (90.0, 0.0) : error("rtp3d: component must be 0, 1, 2 or 3")
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new_inc *= D2R; new_dec *= D2R
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O = O ./ ((sin(new_inc) .+ im .* (cos(new_inc) .* sin.(aux .+ new_dec)) .+ eps()) .* Om)
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end
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O = _fftshift2(O)
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mfin = sum(f3d) / length(f3d) # mean of the input field
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F = _fft2_gmt(complex.(f3d .- mfin))
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fout = real.(_ifft2_gmt(F ./ O))
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return fout, k
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end
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# ---- 2-D FFT/IFFT via GMT's own 1-D C FFT (GMT.fft1d -> GMT_FFT_1D), applied separably: each row
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# then each column. Mathematically identical to a native 2-D FFT since the DFT is separable.
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function _fft2_gmt(A::Matrix{<:Complex})
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ny, nx = size(A)
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B = Matrix{ComplexF64}(undef, ny, nx)
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@inbounds for r = 1:ny
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B[r, :] = GMT.fft1d(view(A, r, :))
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end
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C = Matrix{ComplexF64}(undef, ny, nx)
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@inbounds for c = 1:nx
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C[:, c] = GMT.fft1d(view(B, :, c))
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end
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return C
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end
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function _ifft2_gmt(A::Matrix{<:Complex})
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ny, nx = size(A)
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B = Matrix{ComplexF64}(undef, ny, nx)
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@inbounds for r = 1:ny
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B[r, :] = GMT.fft1d(view(A, r, :); inverse=true)
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end
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C = Matrix{ComplexF64}(undef, ny, nx)
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@inbounds for c = 1:nx
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C[:, c] = GMT.fft1d(view(B, :, c); inverse=true)
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end
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return C
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end
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# Same convention as AbstractFFTs' fftshift: circular shift by half (rounded down) each dimension.
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_fftshift2(A::Matrix{<:Complex}) = circshift(A, div.(size(A), 2))

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