Fanno and Rayleigh Flow, calculating exit conditions

Click For Summary
The discussion centers on the application of Fanno flow and Rayleigh flow equations, specifically how to derive exit conditions from known inlet conditions. Users express confusion regarding the significance of star parameters, which represent conditions at sonic flow (Mach number 1) and serve as reference values. To calculate exit conditions, one can use the provided equations along with inlet parameters, applying the relationship between pressures and densities. The Mach number in the equations refers to the initial Mach number, which is 0.1 in this case. Understanding these concepts allows for accurate calculations of flow parameters in duct systems.
roldy
Messages
206
Reaction score
2
I've seen equations for Fanno flow and Rayleigh flow but I am confused on how to use them properly.

Fanno Flow

<br /> \frac{P}{P^{*}}=\frac{1}{M}\frac{1}{\sqrt{\left(\frac{2}{\gamma+1}}\right)\left(1+\frac{\gamma-1}{2}M^2\right)}<br />

<br /> \frac{\rho}{\rho^{*}}=\frac{1}{M}{\sqrt{\left(\frac{2}{\gamma+1}}\right)\left(1+\frac{\gamma-1}{2}M^2\right)}<br />

<br /> \frac{T}{T^{*}}=\frac{1}{\left(\frac{2}{\gamma+1}\right)\left(1+\frac{\gamma-1}{2}M^2\right)}<br />

<br /> \frac{U}{U^{*}}=M\frac{1}{\sqrt{\left(\frac{2}{\gamma+1}}\right)\left(1+\frac{\gamma-1}{2}M^2\right)}<br />

<br /> \frac{P_0}{P_0^{*}}=\frac{1}{M}\left[\left(\frac{2}{\gamma+1}}\right)\left(1+\frac{\gamma-1}{2}M^2\right)\right]^{\frac{\gamma+1}{2(\gamma-1)}}<br />

<br /> T_0=T_0^{*}<br />

Inlet conditions:

P_0=101325 Pa

T_0=288 K

M_0=0.1

Area=0.1 m^2

T_{wall}=3000K

Friction Coefficient(C_f)=0.2

Duct Length=10 m

Adiabatic, no work interaction, constant area

I guess my confusion comes from the * parameters. If I know my inlet conditions only, how can I calculate the exit conditions from these equations? What do the numerator parameters represent? Are they the values at the exit? The Mach number in these equations, are they any the given Mach number (in this case 0.1)?
 
Physics news on Phys.org
The star quantities just represent the pressure at sonic condition (M = 1). It is just a reference condition. If you had, for example, p_{1} and wanted p_{2}, you would simply do:
p_{2} = \frac{p_2}{p^*}\frac{p^*}{p_1}p_1

You can generally find those values in tables or just calculate them directly if you wish.
 
Due to the constant never ending supply of "cool stuff" happening in Aerospace these days I'm creating this thread to consolidate posts every time something new comes along. Please feel free to add random information if its relevant. So to start things off here is the SpaceX Dragon launch coming up shortly, I'll be following up afterwards to see how it all goes. :smile: https://blogs.nasa.gov/spacex/

Similar threads

  • · Replies 1 ·
Replies
1
Views
2K
  • · Replies 3 ·
Replies
3
Views
1K
  • · Replies 2 ·
Replies
2
Views
858
Replies
6
Views
2K
Replies
5
Views
4K
  • · Replies 4 ·
Replies
4
Views
4K
  • · Replies 1 ·
Replies
1
Views
2K
Replies
9
Views
2K
  • · Replies 21 ·
Replies
21
Views
2K
Replies
7
Views
1K