Model:CAM-CARMA

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CAM-CARMA

Introduction

History

Papers

CAM-CARMA Questionnaire

Contact Information

Model: CAM-CARMA
Contact person: Erik Larson (Model developer)
Institute: LASP/University of Colorado
City: Boulder
Country: USA
Email: larsonej@colorado.edu
2nd person involved: --
3rd person involved: --

Model Description

Model type: Modular model for the terrestrial.
Description: I am developing a recent adaptation of CAM 3.0 that has been converted to Titan by Friedson et al. at JPL. I am adding the aerosol microphysics from CARMA.

Technical information

Supported platforms: Mac OSX
Programming language: Fortran77, Fortran90
Model development started at: Model development still takes place.
To what degree will the model become available: Source code will be available
Current license type: --
Memory requirements: Large
Typical run time: varies greatly

Input / Output description

Input parameters: --
Input format: ASCII
Output parameters: --
Output format: Netcdf files
Post-processing software (if needed): No
Visualization software (if needed): Yes, IDL

Process description

Processes represented by model: CAM treats radiative transfer, tidal forcing from Saturn, a planetary boundary layer and surface interaction, thermal conduction in the soil and chemistry. The CARMA part of the code does the aerosol microphysics involving emission, coagulation and sedimentation.
Key physical parameters & equations: --
Length scale & resolution constraints: Currently there are only initial data sets for 10x15 degrees longitude and latitude. This model is meant for global scale dynamics.
Time scale & resolution constraints: I am running the model with dynamical time steps of 1800 seconds, but it only computes the radiative transfer every 200 timesteps.
Numerical limitations and issues : This is a large model that takes significant computing resources to spin up run.

Testing

Available calibration data sets: --
Available test data sets: --
Ideal data for testing: --

User groups

Currently or plans for collaborating with: I am collaborating with Jim Friedson and Bob West at JPL and Erika Barth at SWRI, as well as my adviser, Brian Toon.

Documentation

Key papers of the model:
  • James Friedson, A., etal., A global climate model of Titan’s atmosphere and surface. Planet. SpaceSci. (2009), doi:10.1016/j.pss.2009.05.006
Is there a manual available: yes
Model website if any: http://www.ccsm.ucar.edu/models/atm-cam/

Additional comments

Comments: --

Issues

Help

Input Files

Output Files

Download

Source