Dataset from "Constraining Martian regolith and vortex parameters from combined seismic and meteorological measurements"

The table provided below (in CSV format) includes derived data obtained from the raw data of the InSight SEIS and APSS experiments. For the raw data, we acknowledge:

InSight Mars SEIS Data Service. (2019). SEIS raw data, Insight Mission. IPGP, JPL, CNES, ETHZ, ICL, MPS, ISAE-Supaero, LPG, MFSC. https://doi.org/10.18715/SEIS.INSIGHT.XB_2016

The dataset in this table was used to produce Figures 6, 7, 11 and 12 of the following paper:

N. Murdoch, A. Spiga, R. Lorenz, R.F. Garcia, C. Perrin, R. Widmer-Schnidrig, S. Rodriguez, N. Compaire, N. H. Warner, D. Mimoun, D. Banfield, P. Lognonné and W.B. Banerdt. Constraining Martian regolith and vortex parameters from combined seismic and meteorological measurements. Journal of Geophysical Research: Planets.

The table provides derived vortex parameters of all vortices studied in this paper. The columns of the table contain the following properties of every vortex event: Sol, UTC date and time, Local Mean Solar Time (LMST), Observed pressure deficit \(\Delta P_{obs}\) (determined from the fit to the Ellehoj et al. (2010) model after filtering in the 0.02 - 0.3 Hz frequency band), Observed pressure drop encounter duration \(\tau\) (FWHM determined from the fit to the Ellehoj et al. (2010) model after filtering in the 0.02 - 0.3 Hz frequency band), the Ellehoj et al. (2010) model goodness of fit to the vortex pressure data (after filtering in the 0.02 - 0.3 Hz frequency band), Mean background wind speed \(v\), Standard deviation of background wind speed \(\sigma_v\), Maximum radial tilt \(\theta_{obs}\), Azimuth at maximum radial tilt (i.e. at closest approach) \(\alpha_{obs}\), Mean miss distance \(x\) (i.e. when \(S = v\)), \(\eta \) (defined as \(E/(1-\nu^2) \)), Mean \(\zeta\) (i.e. when \(S = v\)). For further details about these parameters please see the paper cited above.