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Gibbs SeaWater Oceanographic Package of TEOS-10

Project description

(This python module is incomplete and should be used with caution!)

https://badge.fury.io/py/gsw.png https://api.travis-ci.org/ocefpaf/python-gsw.png?branch=master http://bottlepy.org/docs/dev/_static/Gittip.png

Python implementation of the Thermodynamic Equation Of Seawater - 2010 (TEOS-10)

This module is an python alternative to the gsw MatlabTM toolbox. The table below shows some function names in the gibbs library and the corresponding function names in the seawater library.

TEOS-10 vs. EOS-80

Variable

SeaWater (EOS 80)

Gibbs SeaWater (GSW TEOS 10)

Absolute Salinity

NA

gsw.SA_from_SP(SP,p,long,lat)

Conservative Temperature

NA

gsw.CT_from_t(SA,t,p)

density (i.e. in situ density)

sw.dens(SP,t,p)

gsw.rho_CT(SA,CT,p), or gsw.rho(SA,t,p)

potential density

sw.pden(SP,t,p,pr)

gsw.rho_CT(SA,CT,pr)

potential temperature

sw.ptmp(SP,t,p,pr)

gsw.pt_from_t(SA,t,p,pr)

\(\sigma_0\), using \(\theta_o\) = sw.ptmp(SP,t,p,0)

sw.dens(SP, \(\theta_o\), 0) -1000 kg m\(^{-3}\)

gsw.sigma0_CT(SA,CT)

\(\sigma_2\), using \(\theta_2\) = sw.ptmp(SP,t,p,2000)

sw.dens(SP,\(\theta_2\), 2000) -1000 kg m\(^{-3}\)

gsw.sigma2_CT(SA,CT)

\(\sigma_4\), using \(\theta_4\) = sw.ptmp(SP,t,p,2000)

sw.dens(SP,\(\theta_4\), 4000) -1000 kg m\(^{-3}\)

gsw.sigma2_CT(SA,CT)

specific volume anomaly

sw.svan(SP,t,p)

gsw.specvol_anom_CT(SA,CT,p)

dynamic height anomaly

-sw.gpan(SP,t,p)

gsw.geo_strf_dyn_height(SA,CT,p,delta_p,interp_style)

geostrophic velocity

sw.gvel(ga,lat,long)

gsw.geostrophic_velocity(geo_str,long,lat,p)

N\(^2\)

sw.bfrq(SP,t,p,lat)

gsw.Nsquared(SA,CT,p,lat)

pressure from height (SW uses depth, not height)

sw.pres(-z,lat)

gsw.p_from_z(z,lat)

height from pressure (SW outputs depth, not height)

z = -sw.dpth(p,lat)

gsw.z_from_p(p,lat)

in situ temperature from pt

sw.temp(SP,pt,p,pr)

gsw.pt_from_t(SA,pt,pr,p)

sound speed

sw.svel(SP,t,p)

gsw.sound_speed(SA,t,p)

isobaric heat capacity

sw.cp(SP,t,p)

gsw.cp(SA,t,p)

adiabatic lapse rate*

sw.adtg(SP,t,p)

gsw.adiabatic_lapse_rate(SA,t,p)

SP from cndr, (PSS 78)

sw.salt(cndr,t,p)

gsw.SP_from_cndr(cndr,t,p)

cndr from SP, (PSS 78)

sw.cndr(SP,t,p)

gsw.cndr_from_SP(SP,t,p)

distance

sw.dist(lat,long,units)

gsw.distance(long,lat,p)

gravitational acceleration

sw.g(lat,z)

gsw.grav(lat,p)

Coriolis parameter

sw.f(lat)

gsw.f(lat)

Note that the SW and GSW functions output the adiabatic lapse rate in different units, being K (dbar):math:^{-1} and K Pa\(^{-1}\) respectively.

Authors

  • Bjørn Ådlandsvik

  • Eric Firing

  • Filipe Fernandes

Thanks

  • Bjørn Ådlandsvik - Testing unit and several bug fixes.

  • Eric Firing - Support for masked arrays, re-write of deltaSA.

  • Trevor J. McDougall (and all of SCOR/IAPSO WG127) for making available the Matlab version of this software.

Acknowledgments

  • SCOR/IAPSO WG127 for the original MatlabTM code.

Caveats

  • This python module is incomplete and should be used with caution.

  • The database used in _delta_SA comes from the MatlabTM gsw version.

Changelog

Version 3.0.3

  • Fixed NumPy 1.8.1 indexing bug.

Version 3.0

  • New repository with TEOS-10 code (version 3 only).

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