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wphase:documentation [2014/03/19 01:05]
wphase
wphase:documentation [2015/01/23 16:43]
wphase
Line 1: Line 1:
  
 ====== W-phase documentation ====== ====== W-phase documentation ======
 +
 +===== W-phase Index =====
 +  * [[wphase:​documentation|Documentation]]
 +  * [[wphase:​tutorial|Tutorial]]
 +  * [[wphase:​repository|Repository]]
 +  * [[wphase:​realtime|Real-time]]
 +  * [[wphase:​todo|Todo]]
 +  * [[wphase:​discussion|Discussion]]
  
 ===== Installation ===== ===== Installation =====
 +
 +==== Getting the code ====
 +
 +Currently, the W-phase package is hosted as a github repository. Ask Zacharie Duputel <​zacharie.duputel@unistra.fr>​ or Luis Rivera <​luis.rivera@unistra.fr>​ for access to the repository.
 +
 +Check out W-phase repository:
 +<​code>​
 +git clone https://​github.com/​eost/​wphase.git wphase_package
 +</​code>​
 +
 +To update your W-phase repository (pull changes)
 +<​code>​
 +cd /​to/​the/​wphase/​directory/​
 +git pull origin master
 +</​code>​
 +
 +
 +==== Dependencies ====
 +
 +The w-phase package have only been tested on Unix and Linux computers. You will need the following:
 +  - csh shell
 +  - gcc and gfortran
 +  - python2.7
 +  - You have to install pylab and basemap (matplotlib toolkit) to run some python scripts which make figures.
 +  - GMT4
 +
 +==== Building the code ====
  
 To install the code, we must first setup a few environment variables. If you use csh or tcsh: To install the code, we must first setup a few environment variables. If you use csh or tcsh:
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 ----- -----
  
-===== How to run the W-phase ​code =====+===== How to run W-phase ​ =====
  
 ==== Preparing directories,​ i_master and CMTSOLUTION ==== ==== Preparing directories,​ i_master and CMTSOLUTION ====
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 ----- -----
  
-==== Extracting data from (mini)SEED file(s) ​====+==== Extracting data from SEED ====
 Once the i_master and CMTSOLUTION files are created, we can extract waveforms and instrument response parameters and perform a rough screening by epicentral distance. This can be done using: ​ Once the i_master and CMTSOLUTION files are created, we can extract waveforms and instrument response parameters and perform a rough screening by epicentral distance. This can be done using: ​
 <​code>​${WPHASE_HOME}/​bin/​extract.csh</​code> ​ <​code>​${WPHASE_HOME}/​bin/​extract.csh</​code> ​
wphase/documentation.txt · Last modified: 2022/01/10 07:39 by wphase