Model:WACCM-EE: Difference between revisions
From CSDMS
No edit summary |
m Text replacement - "{{End headertab}}" to "{{End headertab}} {{{{PAGENAME}}_autokeywords}}" |
||
| (29 intermediate revisions by 2 users not shown) | |||
| Line 1: | Line 1: | ||
{{Model identity | |||
|Model type=Modular | |||
}} | |||
{{Model identity2 | |||
|ModelDomain=Climate | |||
|One-line model description=GCM for deep paleoclimate studies | |||
|Extended model description=I am developing a GCM based on NCAR's WACCM model to studied the climate of the ancient Earth. WACCM has been linked with a microphysical model (CARMA). Some important issues to be examined are the climate of the ancient Earth in light of the faint young Sun, reducing chemistry of the early atmosphere, and the production and radiative forcing of Titan-like photochemical hazes that likely enshrouded the Earth at this time. | |||
}} | |||
{{Start model keyword table}} | |||
{{Model keywords | |||
|Model keywords=paleoclimate | |||
}} | |||
{{End a table}} | |||
{{Modeler information | {{Modeler information | ||
|First name=Eric | |First name=Eric | ||
| Line 8: | Line 21: | ||
|Postal code=80309 | |Postal code=80309 | ||
|State=Colorado | |State=Colorado | ||
|Country= | |Country=United States | ||
|Email address=eric.wolf@colorado.edu | |Email address=eric.wolf@colorado.edu | ||
|Phone=240-461-8336 | |Phone=240-461-8336 | ||
}} | }} | ||
{{Model technical information | {{Model technical information | ||
| Line 33: | Line 34: | ||
|Source web address=http://www.cesm.ucar.edu/working_groups/WACCM/ | |Source web address=http://www.cesm.ucar.edu/working_groups/WACCM/ | ||
|Program license type=GPL v2 | |Program license type=GPL v2 | ||
|Memory requirements=1GB for input data | |Memory requirements=1GB for input data | ||
|Typical run time=1.5 days per model year on 8 processor mac | |Typical run time=1.5 days per model year on 8 processor mac | ||
}} | }} | ||
{{Input - Output description | {{Input - Output description | ||
| Line 53: | Line 47: | ||
|Visualization software needed?=Yes | |Visualization software needed?=Yes | ||
|If above answer is yes=IDL | |If above answer is yes=IDL | ||
}} | }} | ||
{{Process description model | {{Process description model | ||
| Line 63: | Line 54: | ||
|Describe time scale and resolution constraints=The model takes about 4-6 model years to reach equilibrium. The modeled time period is from the Archean Earth (3.8 - 2.5 Ga) | |Describe time scale and resolution constraints=The model takes about 4-6 model years to reach equilibrium. The modeled time period is from the Archean Earth (3.8 - 2.5 Ga) | ||
|Describe any numerical limitations and issues=Dynamics, chemistry, RT, microphysical, and slab ocean model are all coupled, thus the model runs slowly. | |Describe any numerical limitations and issues=Dynamics, chemistry, RT, microphysical, and slab ocean model are all coupled, thus the model runs slowly. | ||
}} | }} | ||
{{Model testing | {{Model testing | ||
| Line 71: | Line 59: | ||
|Describe available test data sets=I have numerous data sets produced by an 8 processor Mac and a local unix cluster to confirm the model is initialized correctly. | |Describe available test data sets=I have numerous data sets produced by an 8 processor Mac and a local unix cluster to confirm the model is initialized correctly. | ||
|Describe ideal data for testing=Cassini data describing Titan photochemical haze. Laboratory work constraining haze properties. | |Describe ideal data for testing=Cassini data describing Titan photochemical haze. Laboratory work constraining haze properties. | ||
}} | }} | ||
{{Users groups model | {{Users groups model | ||
|Do you have current or future plans for collaborating with other researchers?=Yes, I plan on collaborating with others in particular when it comes time to rework the model chemistry modules. | |Do you have current or future plans for collaborating with other researchers?=Yes, I plan on collaborating with others in particular when it comes time to rework the model chemistry modules. | ||
}} | }} | ||
{{Documentation model | {{Documentation model | ||
|Manual model available=Yes | |Manual model available=Yes | ||
|Model website if any=CCSM | |Model website if any=CCSM | ||
}} | }} | ||
{{Additional comments model | {{Additional comments model | ||
| Line 99: | Line 74: | ||
http://www.cesm.ucar.edu/working_groups/WACCM/ | http://www.cesm.ucar.edu/working_groups/WACCM/ | ||
}} | }} | ||
{{CSDMS staff part | |||
|OpenMI compliant=No but possible | |||
|CCA component=No but possible | |||
|IRF interface=No but possible | |||
|CMT component=No but possible | |||
}} | |||
{{Start coupled table}} | |||
{{End a table}} | |||
{{End headertab}} | |||
{{{{PAGENAME}}_autokeywords}} | |||
<!-- Edit the part above to update info on other papers --> | <!-- Edit the part above to update info on other papers --> | ||
==Introduction== | ==Introduction== | ||
| Line 112: | Line 93: | ||
== History == | == History == | ||
== | == References == | ||
<br>{{AddReferenceUploadButtons}}<br><br> | |||
{{#ifexist:Template:{{PAGENAME}}-citation-indices|{{{{PAGENAME}}-citation-indices}}|}}<br> | |||
{{Include_featured_references_models_cargo}}<br> | |||
== Issues == | == Issues == | ||
== Help == | == Help == | ||
{{#ifexist:Model_help:{{PAGENAME}}|[[Model_help:{{PAGENAME}}]]|}} | |||
== Input Files == | == Input Files == | ||
== Output Files == | == Output Files == | ||
Latest revision as of 20:16, 16 September 2020
WACCM-EE
Metadata
|
|
|
Introduction
History
References
| Nr. of publications: | 1 |
| Total citations: | 188 |
| h-index: | 1 |
| m-quotient: | 0.06 |
| Featured publication(s) | Year | Model described | Type of Reference | Citations |
|---|---|---|---|---|
|
Bardeen, C. G.; Toon, O. B.; Jensen, E. J.; Marsh, D. R.; Harvey, V. L.; 2008. Numerical simulations of the three-dimensional distribution of meteoric dust in the mesosphere and upper stratosphere. Journal of Geophysical Research, 113, D17202. 10.1029/2007JD009515 (View/edit entry) | 2008 | WACCM-EE |
Model overview | 188 |
| See more publications of WACCM-EE |
