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author | Aaron LI <aly@aaronly.me> | 2017-11-03 13:15:43 +0800 |
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committer | Aaron LI <aly@aaronly.me> | 2017-11-03 13:15:43 +0800 |
commit | eb2fdf35f276a88158ed2620c28cb3ae7cc4e272 (patch) | |
tree | 0784883d917b3f9fe5d5eee07536188e4ea02f9f /astro | |
parent | 075c628a8c3c429b246744996781e5e58218a76c (diff) | |
download | atoolbox-eb2fdf35f276a88158ed2620c28cb3ae7cc4e272.tar.bz2 |
astro/calc_psd.py: Also plot the additional pixel-based frequency axis
Diffstat (limited to 'astro')
-rwxr-xr-x | astro/calc_psd.py | 21 |
1 files changed, 20 insertions, 1 deletions
diff --git a/astro/calc_psd.py b/astro/calc_psd.py index a18e755..50344aa 100755 --- a/astro/calc_psd.py +++ b/astro/calc_psd.py @@ -194,7 +194,26 @@ class PSD: title="Radial (Azimuthally Averaged) Power Spectral Density", xlabel=r"k [%s$^{-1}$]" % self.pixel[1], ylabel="Power") - return ax + + if self.pixel[1] != "pixel": + # Add an additional X axis for pixel-based frequencies + ax2 = ax.twiny() + ax2.set_xscale(ax.get_xscale()) + pix_ticks = np.logspace(-4, 0, num=5) # [pixel^-1] + ax2.set_xticks(pix_ticks) + ax2.set_xticklabels([r"10$^{%d}$" % ep + for ep in np.log10(pix_ticks)]) + x1_min, x1_max = ax.get_xlim() + x2_min, x2_max = x1_min*self.pixel[0], x1_max*self.pixel[0] + ax2.set_xlim(x2_min, x2_max) + ax2.set_xlabel(r"k [pixel$^{-1}$] (1 pixel = %.2f %s)" % + self.pixel) + ax2.grid(False) + # Raise title position to avoid overlapping + ax.title.set_position([0.5, 1.1]) + return (ax, ax2) + else: + return ax def open_image(infile): |