Phys Met Short Answer Flashcards
Charles’ Law
V1/T1 = V2/T2
Concept: Describes how gas expands when heated at constant pressure.
Boyle’s Law
P1V2 = P2V2
Concept: Explains how increasing the pressure on a gas decreases its volume if the temperature remains constant
Universal Gas Constant (R) vs. Specific Gas Constant (R)*
Universal Gas Constant: R* = 8.314J/molK
Specific Gas Constant: R = R/ Molar Mass of Gas
Gas Constant for Dry Air (Rd): 287 J/kgK
Gas Constant for Dry Air (R_v): 461 J/kgK
Similarities: All derived from R. R is being divided by the mass of the gas
Differences: Each R is used for specific things (Rd for dry air for example) ; values lol ; R* provides a general reference for gases
Ideal Gas Law (Moist & Dry Air)
Dry Air: P = pRdT
Moist Air: P = pRTv
p = density ; Rd = dry gas constant ; T = Temperature ; Tv = Virtual Temp
Dry Ideal Gas Law: The Ideal Gas Law for dry air tells us that pressure is directly proportional to the density and temperature of dry air. This equation helps determine the air’s density at different pressures and temperatures.
Moist Ideal Gas Law: The Ideal Gas Law for moist air describes how the total pressure of moist air depends on its density and virtual temperature. By using the virtual temperature, we can apply the Ideal Gas Law to situations involving varying moisture levels, which affects air buoyancy, stability, and density.
Avogadro’s Law
V1/n1 = V2/n2
V = Volume ; n = amount of moles (if k is provided, it is a constant)
Concept: Equal volumes of different gases contain equal numbers of molecules under the same temperature and pressure.
Dalton’s Law
∑ P (P1+P2+P3…)
P = Partial pressures of the individual gases.
Concept: The total pressure of a gas mixture equals the sum of each gas’s partial pressure.
Virtual Temperature
Tv = T(1+0.608w)
T = Actual temp (typically in K) ; w = Mixing ratio (g/kg kg/kg)
Concept: Temperature that dry air would need to match the density of moist air.
Hydrostatic Equation
dP/dz = -pg
p = liquid density ; q = 9.81 m/s^2
Concept: Describes the balance between the upward force of air pressure and the downward force of gravity. Explains why atmospheric pressure decreases with height and helps estimate pressure changes vertically.
Geopotential vs. Geometric Height
Geopotential Height: Adjusted for variations in gravity with altitude.
Geometric Height: Direct measurement above sea level.
What It Tells Us: Geopotential height is more practical in meteorology for comparing energy changes with altitude.
Hypsometric Equation
Z2-Z1 = (RT)/g ln(P1/P2)
R = Gas constant ; T = Mean temperature (in K) ; g = 9.81 m/s^2 ; P1/ P2 = pressure values
Concept: Relates pressure difference to temperature and height in the atmosphere.
Equivalent Barotropic Structures
Concept: Barotropic structures mean temperature is uniform horizontally at any given level. In baroclinic structures, temperature varies horizontally. Helps distinguish between stable systems and those with vertical temperature gradients, affecting atmospheric circulation.
Examples: Barotropic—tropical storms; Baroclinic—mid-latitude cyclones.
Reduction to Sea Level Pressure
Standardizes pressure readings to sea level to allow for consistent comparisons across locations at different altitudes.
First Law of Thermodynamics
ΔU = Q + W
ΔU = change in internal energy, U ; Q = the sum of all heat transfer into and out of the system ; W = the net work done on the system
Concept: Energy conservation principle for systems. Describes how adding heat affects internal energy and work done on/by the atmosphere.
Enthalpy
H = U + pV
U = internal energy ; p = pressure ; V = volume
Concept: The total heat content in a system at constant pressure. Reflects the energy stored and exchanged in atmospheric processes.
Potential Temperature (θ)
θ = T(p0/p)^R/Cp
T = Actual temp ; p0 = reference pressure (typically 1000 hPa) ; p = pressure ; R/Cp = 0.286
Concept: The temperature an air parcel would have if brought adiabatically to p0.