.. index:: ! rotsmoother .. include:: ../module_supplements_purpose.rst_ *********** rotsmoother *********** |rotsmoother_purpose| Synopsis -------- .. include:: ../../common_SYN_OPTs.rst_ **gmt rotsmoother** [ *table* ] [ |-A| ] [ |-C| ] [ |-N| ] [ |-S| ] [ |-T|\ *ages* ] [ |SYN_OPT-V| ] [ |-W| ] [ |-Z| ] [ |SYN_OPT-b| ] [ |SYN_OPT-d| ] [ |SYN_OPT-e| ] [ |SYN_OPT-f| ] [ |SYN_OPT-h| ] [ |SYN_OPT-i| ] [ |SYN_OPT-o| ] [ |SYN_OPT-s| ] [ |SYN_OPT-:| ] [ |SYN_OPT--| ] |No-spaces| Description ----------- **rotsmoother** reads a table of total reconstructions and computes mean rotations (and optionally covariance matrices) for sub-groups of rotations based on rotation age (or all of the rotations). Required Arguments ------------------ *table* Name of a rotation table containing (*lon lat time angle* [*weight*]) values. Optional Arguments ------------------ .. _-A: **-A** Use opening angles as a proxy for time. Suitable when no time can be assigned to the rotations. In this case, input is expected to contain *lon lat angle* [*weight*] records and |-T| settings refer to angles instead of time. [Default expects *lon lat time angle* [*weight*] and |-T| refers to time]. .. _-C: **-C** Compute covariance matrix for each mean rotation. This is done by converting each finite rotation to a quaternion, determining the mean quaternion (rotation) and the consider all rotations as perturbation to the mean rotation. From these perturbations we determine the covariance matrix. .. _-N: **-N** Ensure all poles are in northern hemisphere [Default ensures positive opening angles]. .. _-S: **-S** Ensure all poles are in southern hemisphere [Default ensures positive opening angles]. .. _-T: **-T**\ *ages* Sets the desired groups of ages. For a single time append the desired time and all rotations are used to compute a single mean rotation. For an equidistant range of reconstruction ages give **-T**\ *start*\ /\ *stop*\ /\ *inc* or **-T**\ *start*\ /\ *stop*\ /\ *npoints*\ **+n**. For an non-equidistant set of reconstruction ages please pass them via the first column in a file, e.g., **-T**\ *agefile*. The ages we read or generate becomes the bin-boundaries and we output the average time of all rotations inside each bin. .. |Add_-V| replace:: |Add_-V_links| .. include:: /explain_-V.rst_ :start-after: **Syntax** :end-before: **Description** .. _-W: **-W** Expect weights in last column for a weighted mean rotation [no weights]. .. _-Z: **-Z** Report negative opening angles [positive]. .. |Add_-bi| replace:: [Default is 2 input columns]. .. include:: ../../explain_-bi.rst_ .. |Add_-bo| replace:: [Default is same as input]. .. include:: ../../explain_-bo.rst_ .. |Add_-d| unicode:: 0x20 .. just an invisible code .. include:: ../../explain_-d.rst_ .. |Add_-e| unicode:: 0x20 .. just an invisible code .. include:: ../../explain_-e.rst_ .. |Add_-f| unicode:: 0x20 .. just an invisible code .. include:: ../../explain_-f.rst_ .. |Add_-h| unicode:: 0x20 .. just an invisible code .. include:: ../../explain_-h.rst_ .. include:: ../../explain_-icols.rst_ .. include:: ../../explain_-ocols.rst_ .. include:: ../../explain_-s.rst_ .. include:: ../../explain_colon.rst_ .. include:: ../../explain_-n.rst_ .. include:: ../../explain_help.rst_ .. include:: explain_geodetic.rst_ Examples -------- To smooth rotation groups in increments of 3 Myr and ensure northern hemisphere poles, try:: gmt rotsmoother rotations.txt -N -T3/3/30 -V > rot_means.txt To smooth all rotations and compute a single mean rotation (assigned to time = 5) with corresponding covariance matrix, try:: gmt rotsmoother rotations.txt -C -T5 -V > rot_means_cov.txt See Also -------- :doc:`backtracker`, :doc:`gmtpmodeler`, :doc:`grdpmodeler`, :doc:`grdspotter`, :doc:`hotspotter`, :doc:`originater`, :doc:`rotconverter`