Atmos

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Last updated 8:48 PM on 6/6/26
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44 Terms

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Layers of earths atmosphere

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Layers within earth’s troposphere and their adiabat

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Relationship between R and Ru (define both)

R = Ru/mu . R = specific gas constant [JK-1Kg-1], Ru = universal gas constant 8.31 [JK-1Mol-1]

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Energy (U) of different particle configurations and how to work out deg of freedom

Rotational, vibrational and Transverse modes

<p>Rotational, vibrational and Transverse modes </p>
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Define the mass mixing ratio

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Derive hydrostatic balance

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Derive adiabatic lapse rate

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Define potential temperature, theta

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Define convective stability and determine whether an air parcel is stable?

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Define CAPE?

Convective available potential energy

<p>Convective available potential energy </p>
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Clausius claperon and simplifying assumption

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Derive 2 species moist adiabatic lapse rate

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Relative and specific humidity definitions

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Radiance, I_nu definition

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Wien’s law

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Stefan boltzman equations for thick and thin atmosphere models

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Derive the swatszchild equation for radiative transfer and simplify

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Two stream equations

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Omega, beta and f in gfd

f = 2 omega sin(theta), where omega is 2pi/(3600×24), theta is latitude. Beta is df/dy. Potential vorticity (added beta term) can come out to d²u/dy²

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How to determine the stability of an atmosphere to convection?

dln(T)/dln(P) < R/cp (for stable)

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Geostrophic balance

-fu = 1/rho dP/dy and fv = 1/rho * dP/dy

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Angular momentum for calculations on earth

M = (omega*R*cos(theta) + u)*R*cos(theta)

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Rossby number and meaning

Ro = U/fL, where f = 2omegasin(theta). A small RO is strongly affected by coriolis (f) forces, whereas a large rossby number is not. Geostrophic balance occurs when Ro is low, cyclostrophic balance occurs when this is high.

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Dry adiabat + for diatomic

dln(T)/dln(p) = R / cp, for diatomic: R / cp = 7/2

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Schwartzmann eq

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