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Warning

The new MARS client with the MIR interpolation library is currently in BETA, and it is meant for tests only. Do not use it for any operational purpose.

You can try the new MIR-enabled MARS client with:

No Format
mars -m

You are encouraged to test this new version of the MARS client and report back any issues to advisory@ecmwf.int.


MIR stands for Meteorological Interpolation and Regridding and is a interpolation and regridding tool and library. This new piece of software is replacing the veteran EMOSLIB when it comes to perform those operations in MARS.  Beyond this, MIR’s flexible design facilitates scalability improvements and additional features. These include efficiency gains, a high degree of user configurability, and support for a wider range of grids than in the current package.

Table of Contents

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You can try the new MIR-enabled MARS client with:

No Format
mars -m

You are encouraged to test this new version of the MARS client and report back any issues to advisory@ecmwf.int.

Questions and Answers

Why are you changing?

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MIR will also compute distance in 3D whereas EMOSLIB computes distances on the 2D lat-lon grid. Consequently, different nearest points may be selected for the interpolation methods, and the nearest neighbour method should improve as a result.

See Distance metrics for more details.

Parameter classification

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MIR does not support the 12-point interpolation method, used by EMOSLIB for rotated grids. Therefore, the default interpolation method used is the linear. Rotated spherical harmonics are not supported in MIR or EMOSLIB.

Known Issues