Comments (6)
Yaml file for identification is an old one it will be removed at next realease. If you grid is a regular one you could use eddyid, but it can process only one file by command and only is first time step if you several in one.
To process a time series create a bash or somethings like that.
If your roms are unregular look at a previous closed issue.
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Issue #5
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Thanks a lot for swift reply!
Exactly what I needed for ROMS.
I was thinking about bash script and looping with date variable but then I might endup with bunch of daily files for Cyclonic and Anticyclonic outputs. If I want to make analysis for example on life duration of individual eddies I need to aggregate those daily outputs and have some dimension and then take/find ID of that particular eddy that might change from file to file, or there is already tool/script available?
Cheers
Ivica
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Regarding ROMS inputs, I have already rotated and at collapsed to rho coordinates both u_eastward and v_northward components (Rutgers ROMS have the option). So, according to your #5, all I should do is just to make that speed norm aware of units (change units)? I could do it quickly using NCO ncrename for velocity unit attributes and put them to "meter second^-1"?
Cheers
Ivica
from py-eddy-tracker.
Thanks a lot for swift reply!
Exactly what I needed for ROMS.
I was thinking about bash script and looping with date variable but then I might endup with bunch of daily files for Cyclonic and Anticyclonic outputs. If I want to make analysis for example on life duration of individual eddies I need to aggregate those daily outputs and have some dimension and then take/find ID of that particular eddy that might change from file to file, or there is already tool/script available?Cheers
Ivica
Atlas is produced in two step, identification first and tracking after. For tracking you must used EddyTracking with a yaml file, and also choose method to track.
To subset atlas you could use eddysubsetter. You could also take a look at the gallery from documentation.
from py-eddy-tracker.
Regarding ROMS inputs, I have already rotated and at collapsed to rho coordinates both u_eastward and v_northward components (Rutgers ROMS have the option). So, according to your #5, all I should do is just to make that speed norm aware of units (change units)? I could do it quickly using NCO ncrename for velocity unit attributes and put them to "meter second^-1"?
Cheers
Ivica
I think you need just to have correct units. Speed norm was needed in previous case, because u/v used another dimensions than h.
from py-eddy-tracker.
Related Issues (20)
- Request for help HOT 3
- Bug with matplotlib 3.8
- py_eddy_tracker.dataset.grid issue HOT 6
- pixel position of grid HOT 4
- Lifetime average HOT 3
- The function in the library tried to use Numba to speed up the computation, but received an array of type numpy.ma.MaskedArray that is not supported by Numba. HOT 2
- error about eddy_identification function HOT 2
- Eddies detected on land HOT 6
- Eddy kinetic energy of different types of eddies and its calculation HOT 1
- about from py_eddy_tracker.dataset.grid import RegularGridDataset HOT 1
- Eddy detection issue HOT 3
- batch identification of eddies over multiple days from a single netCDF file HOT 14
- Request for help: No extrema found in contour of xxx pixels in level xxx HOT 6
- Issue reading NEMO UnRegularGrid HOT 2
- grid_count and grid_stat error HOT 2
- The boundary cannot be closed normally, and the longitude and latitude of some points are wrongγ HOT 6
- How to store the eddy tracking results HOT 4
- Data is Empty
- Data is Empty HOT 1
- Cartopy projection HOT 1
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