All variables are provided using two different input as velocity fields;; GlobEkmanDt : MULTIOBS_GLO_PHY_REP_015_004 downloaded from E.U. Copernicus Marine Environment Monitoring Service (CMEMS, http://marine.copernicus.eu/). This was produced by combining the altimetry derived geostrophic velocities and modeled Ekman surface currents. It had a spatial resolution of 0.25¡ and a temporal resolution of one day. ;; GloryS12 : GLOBAL_REANALYSIS_PHY_001_030 downloaded from E.U. Copernicus Marine Environment Monitoring Service (CMEMS, http://marine.copernicus.eu/). It was obtained by a NEMO model assimilating altimetry and other observations. It had a spatial resolution of 1/12¡ and a temporal resolution of 1 day;; ;; All variables are provided as mean and 25, 50 and 75percentiles of all virtual particlesintroduced in the stadium defined by the start and end position of each station;; For all lagrangian diagnostics, advective times (Days backward) of 5, 10, 15,20, 30 and 60 days were used;; ;; Variable label is constructed to reflect the variable_VelocityFieldSource(_AdvectiveTime)_MeanOrPercentile;; ;; variable;description;unit OA;Label of the OA station;nd lon_start;longitude (start of the station position);decimal degree lon_end;longitude (end of the station position);decimal degree lat_start;latitude (start of the station position);decimal degree lat_end;latitude (end of the station position);decimal degree datetime_start;date-time stamp (start of the station);iso UTC datetime_end;date-time stamp (end of the station);iso UTC Uabs;Absolute velocity;m s-1 Ekin;Kinetic energy;m2 .s-2 Vorticity;Vorticity;d-1 OW;Okubo-Weiss;d-2 Ftle;Finite-Time Lyapunov Exponents;d-1 EulerDiverg;Eulerian Divergence;d-1 LagrDiverg;Lagrangian Divergence;d-1 RetentionTime;Retention Time;d Betw;Lagrangian betweenness;nd