All,

Only trivial thing: "aerocentric_longitude" should be "areocentric_longitude" ("RE" instead of "ER").

I think it's the first time to use the word "longitude" to represent a coordinate in space, like in ecliptic longitude or galactic longitude. I'm not inventing other wording, so my suggestion is to modify the description:

"Longitude is positive eastward; its units of degree_east (or equivalent) indicate this explicitly. In a latitude-longitude system defined with respect to a rotated North Pole, the standard name of grid_longitude should be used instead of longitude. Grid longitude is positive in the grid-eastward direction, but its units should be plain degree."

Best Regards,
--
Eizi TOYODA
http://www.google.com/profiles/toyoda.eizi

----- Original Message ----- From: <[email protected]>
To: <[email protected]>; <[email protected]>
Sent: Tuesday, January 25, 2011 11:49 PM
Subject: [CF-metadata] Standard names for Martian climate model data


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.



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