But you're making up the result when you say
it depends on convection so that you can then go on to suggest a rate of convection has an impact.
You really need to account for the vertical structure of temperature (the lapse rate), and if you want your model to get a number of basic things right you need to include spectrally grey absorbers — plus the additional mixing in the troposphere (which
depends on convection, and hence affects water vapour feedbacks) etc....
I agree that there needs to be included a relationship between dh and T and its going to be complex but I do nt agree that its going to
depend on your convection equation to any great extent.
Not exact matches
Place in oven (
convection bake setting is preferable) at 170 degrees for 35 — 60 minutes,
depending on how thin your layer is.
Place in the
convection oven and bake at 180o C / 360o F for 10 — 25 minutes
depending on if you like it al - dente or soft.
The major energy input to the climate system is radiation, not either
convection or conduction, and since the latter two
depend on temperature differences initially induced by radiation, they wouldn't be there
on their own.
Wouldn't the rate of upward moisture transport
depend primarily
on the distribution of
convection?
The ability of a band to shape the temperature profile of the whole atmosphere should tend to be maximum at intermediate optical thicknesses (for a given band width), because at small optical thicknesses, the amounts of emission and absorption within any layer will be small relative to what happens in other bands, while at large optical thicknesses, the net fluxes will tend to go to zero (except near TOA and, absent
convection, the surface) and will be insensitive to changes in the temperature profile (except near TOA), thus allowing other bands greater control over the temperature profile (
depending on wavelength — greater influence for bands with larger bandwidths at wavelengths closer to the peak wavelength — which will
depend on temperature and thus vary with height.
Studies with climate models have noted that the ITCZ width
depends on interactions between radiation and clouds (Voigt & Shaw 2015) and how the model represents sub-grid scale
convection (Kang et al. 2009), but a physical understanding of why the ITCZ width is affected by these processes is lacking.
Clouds too
depend on temperature, pressure,
convection and water vapor amounts.
Then, of course, you have the issues of conduction and
convection which
depend on details of the coupling to the hot plate and the surroundings.
1) The calculation of the GHE
depends on both radiative transfer and
convection.
The temperature of the troposphere (unlike the stratosphere)
depends on the surface temperature through
convection, so when that goes up due to the GHG IR enhancement, the troposphere warms in response.
But deep water production by
convection may be less,
depending on how much NADW is Arctic in origin and how much is simply recirculated Antarctic bottom water (extremely dense water, formed as brine under the sea ice around polynas offshore of Antarctica and sliding down the continental shelf into the depths without much mixing, creates a giant pool of dense water extending all the way up the bottom of the Atlantic to about 60 ° N).
Unfortunately, this can not be reliably predicted since it
depends on the chaotic behavior of the
convection layer of the sun...).
With
convection, the lapse rate is pretty well capped by the adiabatic lapse rate (somewhere between 5 - 10 K / km
depending on humidity), so surface warming is also severely limited.
The strength of the IR component is determined by laws of emission and absorption of radiation and
depend strongly
on the temperatures at various levels, but the total flux is maintained at the level required by stationarity by the
convection and transport of latent energy as long as the radiation alone is not sufficient.
For example, all estimates of government revenue and outgo
depend on some sort of economic model, which superficially have the same weaknesses as climate models: validation issues, adjustable parameters, some key processes (
convection, precipitation, human behavior) can't be reliably modeled.
Processes taken into account included (i) air mixing by pressure and temperature gradients down to a few meters below the surface (i.e., the so - called
convection zone); (ii) molecular diffusion in the open pore space and gravitational fractionation (entrainment toward the deeper firn
depends on concentration gradients, diffusivities, and molar mass); and (iii) a downward air flux in the open porosity zone due to bubble closure removing air from the open pores.