Skip to content

Commit 745fe49

Browse files
ctroupinTroupin Charles
andauthored
typos (AntSimi#53)
Co-authored-by: Troupin Charles <[email protected]>
1 parent 9643697 commit 745fe49

File tree

3 files changed

+20
-21
lines changed

3 files changed

+20
-21
lines changed

doc/custom_tracking.rst

Lines changed: 1 addition & 2 deletions
Original file line numberDiff line numberDiff line change
@@ -6,7 +6,6 @@ Customize tracking
66
Code my own tracking
77
********************
88

9-
To use your own tracking method, you just need to create a class which inherit
9+
To use your own tracking method, you just need to create a class which inherits
1010
from :meth:`py_eddy_tracker.observations.observation.EddiesObservations` and set this class in yaml file like
1111
we see in the previous topic.
12-

doc/grid_identification.rst

Lines changed: 5 additions & 5 deletions
Original file line numberDiff line numberDiff line change
@@ -8,7 +8,7 @@ Run the identification process for a single day
88
Shell/bash command
99
******************
1010

11-
Bash command will allow to process one grid, it will apply a filter and an identification.
11+
Bash command will allow you to process one grid, it will apply a filter and an identification.
1212

1313

1414
.. code-block:: bash
@@ -18,14 +18,14 @@ Bash command will allow to process one grid, it will apply a filter and an ident
1818
out_directory -v DEBUG
1919
2020
21-
Filter could be modify with options *--cut_wavelength* and *--filter_order*. You could also defined height between two isolines with *--isoline_step*, which could
21+
Filter could be modified with options *--cut_wavelength* and *--filter_order*. You could also define height between two isolines with *--isoline_step*, which could
2222
improve speed profile quality and detect accurately tiny eddies. You could also use *--fit_errmax* to manage acceptable shape of eddies.
2323

2424
An eddy identification will produce two files in the output directory, one for anticyclonic eddies and the other one for cyclonic.
2525

26-
In regional area which are away from the equator, current could be deduce from height, juste write *None None* inplace of *ugos vgos*
26+
In regional areas which are away from the Equator, current could be deduced from height, just write *None None* in place of *ugos vgos*
2727

28-
In case of **datacube**, you need to specify index for each layer (time, depth, ...) wiht *--indexs* option like:
28+
In case of **datacube**, you need to specify index for each layer (time, depth, ...) with *--indexs* option like:
2929

3030
.. code-block:: bash
3131
@@ -40,7 +40,7 @@ In case of **datacube**, you need to specify index for each layer (time, depth,
4040
Python code
4141
***********
4242

43-
If we want customize eddies identification, python module is here.
43+
If we want to customize eddies identification, the Python module is here.
4444

4545
Activate verbose
4646

doc/run_tracking.rst

Lines changed: 14 additions & 14 deletions
Original file line numberDiff line numberDiff line change
@@ -5,9 +5,9 @@ Tracking
55
Requirements
66
************
77

8-
Before to run tracking, you will need to run identification on every time step of the period(Period of your study).
8+
Before to run tracking, you will need to run identification on every time step of the period (period of your study).
99

10-
**Advice** : Before to run tracking, display some identification file allow to learn a lot
10+
**Advice** : Before to run tracking, displaying some identification file allows one to learn a lot
1111

1212
Default method
1313
**************
@@ -35,24 +35,24 @@ To run:
3535
3636
EddyTracking conf.yaml -v DEBUG
3737
38-
It will use default tracker:
38+
It will use the default tracker:
3939

40-
- No travel longer than 125 km between two observation
41-
- Amplitude and speed radius must be close to previous observation
42-
- In case of several candidate only closest is kept
40+
- No travel longer than 125 km between two observations
41+
- Amplitude and speed radius must be close to the previous observation
42+
- In case of several candidates only the closest is kept
4343

4444

4545
It will produce 4 files by run:
4646

47-
- A file of correspondances which will contains all the information to merge all identifications file
48-
- A file which will contains all the observations which are alone
49-
- A file which will contains all the short track which are shorter than **TRACK_DURATION_MIN**
50-
- A file which will contains all the long track which are longer than **TRACK_DURATION_MIN**
47+
- A file of correspondences which will contain all the information to merge all identifications file
48+
- A file which will contain all the observations which are alone
49+
- A file which will contain all the short tracks which are shorter than **TRACK_DURATION_MIN**
50+
- A file which will contain all the long tracks which are longer than **TRACK_DURATION_MIN**
5151

52-
Use python module
52+
Use Python module
5353
*****************
5454

55-
An example of tracking with python module is available in the gallery:
55+
An example of tracking with the Python module is available in the gallery:
5656
:ref:`sphx_glr_python_module_08_tracking_manipulation_pet_run_a_tracking.py`
5757

5858
Choose a tracker
@@ -67,7 +67,7 @@ With yaml you could also select another tracker:
6767
FILES_PATTERN: MY/IDENTIFICATION_PATH/Anticyclonic*.nc
6868
SAVE_DIR: MY_OUTPUT_PATH
6969
70-
# Number of timestep for missing detection
70+
# Number of timesteps for missing detection
7171
VIRTUAL_LENGTH_MAX: 3
7272
# Minimal time to consider as a full track
7373
TRACK_DURATION_MIN: 10
@@ -80,5 +80,5 @@ With yaml you could also select another tracker:
8080
# py_eddy_tracker.observations.observation.EddiesObservations
8181
CLASS: CheltonTracker
8282
83-
This tracker is like described in CHELTON11[https://doi.org/10.1016/j.pocean.2011.01.002].
83+
This tracker is like the one described in CHELTON11[https://doi.org/10.1016/j.pocean.2011.01.002].
8484
Code is here :meth:`py_eddy_tracker.featured_tracking.old_tracker_reference`

0 commit comments

Comments
 (0)