Data used in the analysis of Baltis Vallis, Venus

The files included in this data repository were used in the<br> analysis and figures of Conrad and Nimmo (2023) to determine<br> the characteristic wavelengths of the Baltis Vallis canale. Baltis Vallis is a ~7000 km long channel on the surface of<br> Venus that was altered over most of that length. The included files are in comma separated values format with<br> the first line giving the column disciptions. File Discriptions:<br> FordVenus720shape.txt = Spherical Harmonics Coefficients derived from Ford and Pettengil (1992)'s topography<br> BaltisVallis_LLT.csv = Baltis Vallis longitude, latitude, topography sampled from ArcGIS<br> BaltisVallis_Metrics_North.txt = % downhill and conformity factor as a funciton of maximum spherical harmonic degree. North source case<br> BaltisVallis_Metrics_South.txt = % downhill and conformity factor as a funciton of maximum spherical harmonic degree. South source case<br> Synthetic_Metric_Deviation.txt = Standard deviation of % downhill and conformity factor for our 1000 synthetic profiles.<br> BaltisVallis_Power_Spectrum.txt = Topographic power spectra of the topography presented in BaltisVallis_LLT.csv