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Science 123
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Spring 2026
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Atmospheric Stability
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Parcel Thermodynamics (video)
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Ideal Gas Law : relating temperature, pressure and density
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$P = 2.87\rho T$
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$T = am_wv^2$ temperature is directly related to the kinetic energy of the molecules
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$P = \frac{\mbox{force}}{\mbox{area}} \sim \frac{\mbox{mass} \times \mbox{velocity} \times \mbox{frequency}}{\mbox{area}}$ exerted on the "walls" of the parcel
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$\rho = \frac{\mbox{mass}}{\mbox{volume}}$
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Potential Temperature $\Theta = T\left(\frac{1000}{P} \right)^{R/C_p}$ is used to determine the temperature
of the parcel as it moves off the surface of the earth into lower pressure $P$ with no phase change of water within the parcel.
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Figure of $\theta$ as a function of altitude and latitude.
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adiabatic process - no exchange of energy between the parcel and its environment.
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Potential temperature, $\theta$, is conserved when no moisture phase change occurs within the parcel.
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rising parcel of air cools - molecular KE is decreased as the parcel constituents expand the parcels by pushing against the parcel "walls"
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sinking parcel of air warms - molecular KE is increased as the parcel walls contract and impart energy to the parcel constituents
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Equivalent Potential Temperature, $\Theta_e$, accounts for difference of pressure and the thermal energy "potential" of the parcel due to the mass of water vapor of the parcel.
The formula is
$\Theta_e = T_e\left(\frac{1000}{P} \right)^{R/C_p} = \left(T + \frac{L_v}{C_p} \cdot W \right) \left(\frac{1000}{P} \right)^{R/C_p}$
where $L_v$ is the latent heat of vaporization (condensation), $C_p$ is the heat capacity of dry air, and $W$ is the mixing ratio of the parcel in kg/kg or gm/gm.
The quantity $T_e = T + \frac{L_v}{C_p} \cdot W$ is referred to as the equivalent temperature of the parcel.
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Lapse Rates (video)
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environmental : $\Gamma_e$ = 6.5 degrees C per 1000 m
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dry adiabatic : $\Gamma_d$ = 10 degrees C per 1000 m
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moist adiabatic : $\Gamma_m$ = 6 degrees C per 1000 m
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Atmospheric Stability (video)
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Stabilizing Events
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upper levels of the atmosphere warm
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warm advection
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lower levels of the atmosphere cool
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radiational cooling
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cold advection
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air moving over a cold surface
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subsidence inversions
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top of the subsiding layer sinks more than the bottom of the layer
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Destabilizing Events (video)
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cooling aloft
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cold advection
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short wave
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radiational cooling (cloud tops or air)
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warming at the surface
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solar radiational heating
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warm advection
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air moving over a warm surface
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mixing
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lifting of an entire layer
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convective instability
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Cloud Development (video)
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Thermodynamic Chart : Skew T - Log P (video)
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Example Exercises