Aero formulas: Difference between revisions

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(more entropy and variables)
(more thermodynamics)
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|style="background:white"| {{SERVER}}/images/formulas_mirror/dUeqdQmindW.png
|style="background:white"| {{SERVER}}/images/formulas_mirror/dUeqdQmindW.png
|[https://en.wikipedia.org/wiki/First_law_of_thermodynamics First law of Thermodynamics]
|[https://en.wikipedia.org/wiki/First_law_of_thermodynamics First law of thermodynamics]
|Variations of internal energy of a system between two states is the sum of the received heat and work (minus the ''given'' work).
|Variations of internal energy of a system between two states is the sum of the received heat and work (minus the ''given'' work).
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|style="background:white"| {{SERVER}}/images/formulas_mirror/enthalpy.png
|style="background:white"| {{SERVER}}/images/formulas_mirror/enthalpy.png
|[https://en.wikipedia.org/wiki/Enthalpy Enthalpy]
|[https://en.wikipedia.org/wiki/Enthalpy Enthalpy]
|Total amount of energy of a system, defined as the sum of the internal energy U and pressure * volume.
|Total amount of energy of a system, defined as the sum of the internal energy U of the system and pressure * volume at the boundary of the system and its environment.
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|style="background:white"| {{SERVER}}/images/formulas_mirror/workExpand.png
|style="background:white"| {{SERVER}}/images/formulas_mirror/workExpand.png
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|Entropy variation as a whole.
|Entropy variation as a whole.
|Entropy variation of a system is generally compensated by the inverse variation of the surroundings, not including losses.
|Entropy variation of a system is generally compensated by the inverse variation of the surroundings, not including losses.
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|style="background:white"| {{SERVER}}/images/formulas_mirror/dS.png
|[https://en.wikipedia.org/wiki/Second_law_of_thermodynamics Second law of thermodynamics]
|A change in the entropy of a system is the infinitesimal transfer of heat to a closed system driving a reversible process, divided by the equilibrium temperature of the system.
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|style="background:white"| {{SERVER}}/images/formulas_mirror/gibbs.png
|style="background:white"| {{SERVER}}/images/formulas_mirror/gibbs.png
|[https://en.wikipedia.org/wiki/Gibbs_free_energy Gibbs free energy] / Free enthalpy
|[https://en.wikipedia.org/wiki/Gibbs_free_energy Gibbs free energy] / Free enthalpy
|Useful work obtainable from a system at isobaric and isothermal conditions. Since H is U + pV, it can be replaced in the equation, making G = H - TS.
|Useful work obtainable from a system at '''isobaric''' and '''isothermal''' conditions. Since H is U + pV, it can be replaced in the equation, making G = H - TS.
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|style="background:white"| {{SERVER}}/images/formulas_mirror/deltaG.png
|style="background:white"| {{SERVER}}/images/formulas_mirror/deltaG.png
|[https://en.wikipedia.org/wiki/Gibbs_free_energy Gibbs free energy] variation.
|[https://en.wikipedia.org/wiki/Gibbs_free_energy Gibbs free energy] variation.
|This derivation is only valid at constant temperature.
|If ΔG < 0, the system's transformation can be spontaneous, if ΔG = 0 the transformation is inversible and the system is in an equilibrium state, if ΔG > 0 it can't be spontaneous.
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Revision as of 00:25, 11 April 2012

Resources on physics related to aerodynamics

The List of elementary physics formulae on wikipedia is useful.

List of variables

Variable Meaning Unit (SI)
γ (gamma) Surface tension N.m-1 (Newton per meter)
μ (mu) or η (eta) Viscosity Pa·s (Pascal second) or P (Poise, 1 Poise is 0.1 Pa.s)
C, Cp, CV Heat capacity, general, at constant pressure, at constant volume. J.K-1 (Joule per Kelvin)
G Gibbs free energy J (Joule)
H Enthalpy: total energy of a thermodynamic system. J (Joule)
ΔHvap or L Vaporization heat or Latent heat of vaporization: energy required to vaporize a mole of liquid at a given temperature. J.mol-1 (Joule per mole)
Q Amount of Heat J (Joule)
T Temperature K (Kelvin)
S Entropy J.K-1 (Joule per Kelvin)
U Internal energy of a system (see first law of Thermodynamics below) J (Joule)
V Volume m3 (cubic meter)
W Work: mechanical constraints on the system. J (Joule)
n Quantity of matter mol (mole)
p Pressure Pa (Pascal)

List of constants

Constant Meaning Value Unit (SI)
NA or N Avogadro constant, number of atoms or molecules in a mole. 6.02214129.1023 mol-1
R ideal gas constant 8.3144621 J.K−1.mol−1
kB or k Boltzmann constant, gas constant R divided by Avogadro number. 1.3806488.10-23 J.K-1

List of equations

Equation Name Meaning
pvnrtk.png Ideal gas equation Relation between properties of an ideal gas (state equation). k is kB.
clausius-clapeyron.png Clausius-Clapeyron relation Relation between the pressure, latent heat of vaporization and temperature of a vapour at two temperatures (approximation, at low temperatures).
QeqmL.png Heat at state change for an ideal gas. The heat required to change the state of a some matter, L being the latent heat. Delta H equals Q only when pressure is constant (isobaric).
dUeqdQmindW.png First law of thermodynamics Variations of internal energy of a system between two states is the sum of the received heat and work (minus the given work).
enthalpy.png Enthalpy Total amount of energy of a system, defined as the sum of the internal energy U of the system and pressure * volume at the boundary of the system and its environment.
workExpand.png Work of gas expansion. Work done by expanding an ideal gas.
entropy_dueqtdsmpdv.png Entropy Internal energy related to entropy variation for a closed system in thermal equilibrium (fundamental thermodynamic relation).
ΔSuniverse = ΔSsurroundings + ΔSsystem Entropy variation as a whole. Entropy variation of a system is generally compensated by the inverse variation of the surroundings, not including losses.
dS.png Second law of thermodynamics A change in the entropy of a system is the infinitesimal transfer of heat to a closed system driving a reversible process, divided by the equilibrium temperature of the system.
gibbs.png Gibbs free energy / Free enthalpy Useful work obtainable from a system at isobaric and isothermal conditions. Since H is U + pV, it can be replaced in the equation, making G = H - TS.
deltaG.png Gibbs free energy variation. If ΔG < 0, the system's transformation can be spontaneous, if ΔG = 0 the transformation is inversible and the system is in an equilibrium state, if ΔG > 0 it can't be spontaneous.