This raises a broader question about CF, perhaps thinking too far ahead.

Per my understanding, the terms in CF are chosen to maximize the 
interoperability of data sets that use them. The idea is that I can expect my 
sea_water_temperature or air_temperature to be pretty much the same as yours.

What is the mechanism by which the grand poobah of data set searching, or 
anyone else, can tell that the air_temperature of the BADC climate model is of 
the Martian atmosphere, not the Earth one?  My assumption has always been that 
the terms are describing _this planet's_ observables.

Presumably casual inspection will be likely to make obvious the distinction in 
many/most (all?) cases, so is that sufficient?  Or do we want the computer that 
finds a model with air_temperature to be able to understand which planet's air 
is being referred to, just from the variable name?

John

On Jan 25, 2011, at 06:49, <[email protected]> 
<[email protected]> wrote:

> Dear All,
> 
> At BADC we are preparing to archive some data generated by a group at Oxford 
> University who are working on a climate model of the Martian atmosphere.  The 
> data will be archived as CF-compliant netCDF files. Many of the model 
> variables are the same as those used in earth simulations, e.g., air 
> temperature, u and v wind components, surface atmospheric pressure, and for 
> all these we will use existing standard names.  However, there are a small 
> number of variables for which there are no existing standard names.  
> Therefore, we would like to propose the following new names:
> 
> carbon_dioxide_ice_amount; kg m-2
> This is the mass per unit area of frozen carbon dioxide on the Martian 
> surface.
> 
> atmosphere_optical_thickness_due_to_dust_dry_aerosol; 1
> This follows the pattern of the existing name 
> atmosphere_optical_thickness_due_to_dust_ambient_aerosol and is defined in an 
> analogous way.
> 
> aerocentric_longitude; degree
> 'Aerocentric longitude' is a widely used term within the Mars modelling 
> community and indicates the season within the Martian year according to the 
> sun's apparent motion relative to the planet's equator. Zero degrees is 
> defined as the northern hemisphere vernal equinox, i.e.,  the ascending node 
> of the apparent seasonal motion of the Sun on the planet's equator 
> [http://www.giss.nasa.gov/tools/mars24/help/notes.html]. Thus 90, 180 and 270 
> degrees indicate, respectively, the summer solstice, autumnal equinox and 
> winter solstice.
> 
> We would welcome comments on these proposals.
> 
> Best wishes,
> Alison
> 
> ------
> Alison Pamment                          Tel: +44 1235 778065
> NCAS/British Atmospheric Data Centre    Fax: +44 1235 446314
> STFC Rutherford Appleton Laboratory     Email: [email protected]
> R25, 2.22
> Harwell Oxford, Didcot, OX11 0QX, U.K.
> 
> 
> 
> -- 
> Scanned by iCritical.
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John Graybeal   <mailto:[email protected]> 
phone: 858-534-2162
System Development Manager
Ocean Observatories Initiative Cyberinfrastructure Project: 
http://ci.oceanobservatories.org
Marine Metadata Interoperability Project: http://marinemetadata.org   

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