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This table provides the values we've been using and explanation of what each quantity means.


 ne30ne120 before 8/10/16ne120 after 8/10/16Explanation
dtime30 min15 min15 minTimestep used for most physics processes and for coupling between physics and dynamics
se_nsplit246*dtime/se_nsplit = time between vertical remaps of the semi-Lagrangian vertical coordinate.
se_qsplit111

dtime/(se_nsplit*se_qsplit) = timestep used for tracer advection

(this should always be 1)

se_rsplit4332*

dtime/(se_nsplit*se_qsplit*se_rsplit) = timestep used for dynamics calculations

For ne30, dt_dyn = 360s is probably stable, but we usually use 300s

For ne120, dt_dyn = 90s is probably stable, but we usually use 75s.

hypervis_subcycle344dtime/(se_nsplit_se_qsplit*se_rsplit*hypervis_subcycle) = timestep used for hyperviscosity calculation
hypervis_subcycle_q111dtime/(se_nsplit_se_qsplit*se_rsplit*hypervis_subcycle_q) = timestep used for hyperviscosity calculation in tracer advection (namelist_definition.xml indicates that only '1' is supported in CAM?)
cld_macmic_num_steps63*3Number of times the code surrounding macrophysics + microphysics is subcycled. This means that dtime/cld_macmic_num_steps = timestep used for macrophysics and microphysics.
clubb_timestep300 sec300 sec300 secI'm not sure what this means or how it relates to cld_macmic_num_steps
IRADSW2 steps4 steps (1 hr)4 steps (1 hr)How frequently to compute SW radiation (in multiples of dtime). Radiation tendencies are taken from previous steps for steps when radiation is not recalculated. I think some scaling is made to account for zenith angle changes?
IRADLW2 steps4 steps4 stepsHow frequently to compute LW radiation (in multiples of dtime). Radiation tendencies are taken from previous steps for steps when radiation is not recalculated.   


*since AV1C-04*suggest to use 

 

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