Model:CAM-CARMA: Difference between revisions
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{{Model identity | |||
|Model type=Modular | |||
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{{Model identity2 | |||
|ModelDomain=Terrestrial | |||
|One-line model description=A GCM for Titan that incorporates aerosols | |||
|Extended model 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. | |||
}} | |||
{{Start model keyword table}} | |||
{{Model keywords | |||
|Model keywords=global climate | |||
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{{Modeler information | {{Modeler information | ||
|First name=Eric | |First name=Eric | ||
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|Town / City=Boulder | |Town / City=Boulder | ||
|Postal code=80309 | |Postal code=80309 | ||
|Country=United States | |||
|State=Colorado | |State=Colorado | ||
|Email address=larsonej@colorado.edu | |||
|Email address=larsonej@colorado.edu | |||
|Phone=3034928207 | |Phone=3034928207 | ||
}} | }} | ||
{{Model technical information | {{Model technical information | ||
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|Programming language=Fortran77, Fortran90 | |Programming language=Fortran77, Fortran90 | ||
|Does model development still take place?=Yes | |Does model development still take place?=Yes | ||
|DevelopmentCode=Active | |||
|DevelopmentCodeYearChecked=2020 | |||
|Model availability=As code | |Model availability=As code | ||
|Source code availability=Through | |Source code availability=Through web repository | ||
|Source web address=http://www.ccsm.ucar.edu/models/atm-cam/ | |||
|Program license type=Other | |Program license type=Other | ||
|Program license type other=-- | |Program license type other=-- | ||
|Memory requirements=large | |Memory requirements=large | ||
|Typical run time=varies greatly | |Typical run time=varies greatly | ||
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{{Process description model | {{Process description model | ||
|Describe processes represented by the 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. | |Describe processes represented by the 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. | ||
|Describe key physical parameters and equations=-- | |Describe key physical parameters and equations=-- | ||
|Describe length scale and resolution constraints=Currently there are only initial data sets for 10x15 degrees longitude and latitude. This model is meant for global scale dynamics. | |Describe length scale and resolution constraints=Currently there are only initial data sets for 10x15 degrees longitude and latitude. This model is meant for global scale dynamics. | ||
|Describe time scale and resolution constraints=I am running the model with dynamical time steps of 1800 seconds, but it only computes the radiative transfer every 200 timesteps. | |Describe time scale and resolution constraints=I am running the model with dynamical time steps of 1800 seconds, but it only computes the radiative transfer every 200 timesteps. | ||
|Describe any numerical limitations and issues=This is a large model that takes significant computing resources to spin up run. | |Describe any numerical limitations and issues=This is a large model that takes significant computing resources to spin up run. | ||
}} | }} | ||
{{Model testing}} | |||
{{Users groups model | {{Users groups model | ||
|Do you have current or future plans for collaborating with other researchers?=I am collaborating with Jim Friedson and Bob West at JPL and Erika Barth at SWRI, as well as my adviser, Brian Toon. | |Do you have current or future plans for collaborating with other researchers?=I am collaborating with Jim Friedson and Bob West at JPL and Erika Barth at SWRI, as well as my adviser, Brian Toon. | ||
}} | }} | ||
{{Documentation model | {{Documentation model | ||
|Manual model available=Yes | |Manual model available=Yes | ||
|Model website if any=http://www.ccsm.ucar.edu/models/atm-cam/ | |Model website if any=http://www.ccsm.ucar.edu/models/atm-cam/ | ||
}} | }} | ||
{{Additional comments model | {{Additional comments model | ||
|Comments=NOTICE: code is free available through CCSM UCAR website: | |||
| | http://www.ccsm.ucar.edu/models/atm-cam/ | ||
No need to register | |||
}} | }} | ||
{{CSDMS staff part | |||
|OpenMI compliant=No but possible | |||
|IRF interface=No but possible | |||
|CMT component=No but possible | |||
|CCA component=No but possible | |||
}} | |||
{{Start coupled table}} | |||
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<!-- Edit the part above to update info on other papers --> | <!-- Edit the part above to update info on other papers --> | ||
== | ==Introduction== | ||
== | == History == | ||
== | == References == | ||
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{{#ifexist:Template:{{PAGENAME}}-citation-indices|{{{{PAGENAME}}-citation-indices}}|}}<br> | |||
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== | == Issues == | ||
== | == Help == | ||
{{#ifexist:Model_help:{{PAGENAME}}|[[Model_help:{{PAGENAME}}]]|}} | |||
== | == Input Files == | ||
== Output Files == |
Latest revision as of 20:16, 16 September 2020
CAM-CARMA
Metadata
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Introduction
History
References
Nr. of publications: | 2 |
Total citations: | 2138 |
h-index: | 2 |
m-quotient: | 0.1 |
Featured publication(s) | Year | Model described | Type of Reference | Citations |
---|---|---|---|---|
Collins, W.D.; Rasch, P.J.; Boville, B.A.; Hack, J.J.; McCaa, J.R.; Williamson, D.L.; Kiehl, J.T.; Briegleb, B.; 2004. Description of the NCAR Community Atmosphere Model (CAM 3.0).. , , . (View/edit entry) | 2004 | CAM-CARMA |
Model overview | 2091 |
Friedson, A. James; West, Robert A.; Wilson, Eric H.; Oyafuso, Fabiano; Orton, Glenn S.; 2009. A global climate model of Titan's atmosphere and surface. Planetary and Space Science, 57, 1931–1949. 10.1016/j.pss.2009.05.006 (View/edit entry) | 2009 | CAM-CARMA |
Model overview | 47 |
See more publications of CAM-CARMA |