TaylorSwift
The name is in honor of physicist Sir Geoffrey Ingram Taylor. FFT-based (co)spectral analysis for eddy covariance time series.
TaylorSwift implements the standard micrometeorological workflow for computing power spectra and cospectra from high-frequency sonic anemometer and open-path gas analyser data, following Kaimal et al. (1972) conventions.
Features
- Spectral computation — double-rotation, linear detrending, Hamming-windowed FFT, logarithmic frequency binning, area-preserving normalization
- Spectral corrections — block-average, linear-detrend, first-order sensor response, sonic path averaging, sensor separation (Massman 2000; Horst 1997)
- Despiking — iterative UKDE despiking for raw time series (Metzger et al. 2012); rolling IQR, median-RLM, and EWMA methods via
CalcFlux - WPL density correction — Webb-Pearman-Leuning (1980) for open-path CO₂/H₂O fluxes
- Quality control — inertial-subrange slope fitting, stationarity test (Foken & Wichura 1996), Foken 9-class quality flags, ITC tests, outlier detection
- Physical constants — curated constants, surface-type enumerations, and roughness / displacement height helpers
- Flux pipeline — end-to-end
CalcFluxprocessor for IRGASON and KH-20 sensor suites with Polars/pandas compatibility - I/O — fast Campbell Scientific TOA5 reader and multi-file compiler (Polars backend)
- Plotting — publication-quality Kaimal-style spectral and cospectral figures
Installation
pip install taylorswift-spectra
The distribution is named taylorswift-spectra on PyPI (the shorter name was
already taken); the import name is unchanged:
import TaylorSwift
For development:
git clone https://github.com/inkenbrandt/TaylorSwift
cd TaylorSwift
pip install -e ".[dev]"
Quick start
import TaylorSwift as tswift
# --- Configure the site ---
config = tswift.SiteConfig(
z_measurement=3.0, # measurement height [m]
z_canopy=0.3, # canopy height [m]
sampling_freq=20.0, # Hz
averaging_period=30.0 # minutes
)
# --- Load a raw TOA5 file ---
df, meta = tswift.read_toa5("path/to/TOA5_mysite.dat")
# --- Process all 30-min intervals ---
results = tswift.process_file(df, config)
# --- Run quality control ---
results = tswift.run_qc(results)
# --- Plot ---
fig = tswift.plot_cospectra(results)
fig.savefig("cospectra.pdf")
Processing pipeline
TOA5 files
│
▼ tswift.read_toa5() / tswift.compile_toa5()
polars.DataFrame
│
▼ tswift.process_file()
│ ├─ double rotation (mean v = w = 0)
│ ├─ linear detrend
│ ├─ batched FFT (6 signals)
│ ├─ logarithmic frequency binning
│ └─ turbulence statistics (u*, L, z/L, H)
list[SpectralResult]
│
├──▶ corrections.apply_spectral_corrections() (optional)
├──▶ qc.run_qc()
└──▶ plotting.plot_cospectra() / plot_spectra() / plot_ogive()
Module overview
| Module | Contents |
|---|---|
core |
process_interval, process_file — the FFT cospectral pipeline |
cospectra |
SpectralResult, compute_cospectrum, compute_spectrum, log_bin, transfer functions, apply_spectral_corrections, compute_spectral_correction_factor |
config |
SiteConfig, InstrumentConfig, FluxConfig, ProcessingConfig |
io |
read_toa5, compile_toa5, scan_toa5_directory |
corrections |
wpl_correction, webb_pearman_leuning, shadow_correction, enrich_results_with_means |
despike |
ukde_despike, polars_ukde_despike, despike_dataframe, despike_med_mod, mad_outliers, rolling_sigma_filter |
data_quality |
fit_inertial_slope, stationarity_test, run_qc, QualityFlag, DataQuality, quality_filter |
rotations |
rotate_wind (double rotation), coord_rotation, rotate_velocities |
pipelines |
run_irga, run_kh20 — end-to-end flux pipelines for IRGASON and KH-20 |
plotting |
plot_cospectra, plot_spectra, plot_ogive, plot_summary_timeseries |
constants |
SurfaceType, Hemisphere, QualityThreshold, get_displacement_height, get_roughness_length, physical constants |
compat |
CalcFlux — backward-compatible wrapper around the legacy flux API |
Running tests
pytest
# or with coverage:
pytest --cov=TaylorSwift
References
- Kaimal, J.C. et al. (1972). Spectral characteristics of surface-layer turbulence. Quart. J. Roy. Meteor. Soc., 98, 563–589.
- Massman, W.J. (2000). A simple method for estimating frequency response corrections for eddy covariance systems. Agric. For. Meteorol., 104, 185–198.
- Webb, E.K., Pearman, G.I. & Leuning, R. (1980). Correction of flux measurements for density effects. Quart. J. Roy. Meteor. Soc., 106, 85–100.
- Foken, T. & Wichura, B. (1996). Tools for quality assessment of surface-based flux measurements. Agric. For. Meteorol., 78, 83–105.
- Foken, T. et al. (2004). Post-field data quality control. In Handbook of Micrometeorology (pp. 181–208). Springer.
- Metzger, S. et al. (2012). Eddy-covariance flux measurements with a weight-shift microlight aircraft. Atmos. Meas. Tech., 5, 1699–1717.
- Oke, T.R. (1987). Boundary Layer Climates (2nd ed.). Routledge.
- Stull, R.B. (1988). An Introduction to Boundary Layer Meteorology. Springer.
Metadata
Release files for taylorswift-spectra 0.2.2
For a detailed explanation of source distributions (sdists) and built distributions (wheels), please see the package formats documentation.
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| File | Size | Uploaded | |
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Built distribution (wheel)
| File | Interpreter | ABI | Platform | Reset |
|---|---|---|---|---|
| taylorswift_spectra-0.2.2-py3-none-any.whl | Python 3 | none | any | Details |
Total release size: 179.5 kB
Release files / taylorswift_spectra-0.2.2.tar.gz
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