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Modelling a short squarewave pulse with Telegrapher's Equation 
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#1
Dec1410, 02:59 AM

P: 1

I am interested in looking at the voltage component of a short (possibly nanosecond width) pulse in a coaxial cable along the cable at a given distance, Z, along the line. I am "cheating" by using the steady state Telegrapher's equation [Eq. 1] and formulating a periodic pulse approximation. It may not be desirable to use this steady state equation, but some form of the Telegrapher's Eq. is advised (suggestions for alternatives are appreciated). This is unlike my "physical" setup in which I will send a single pulse of information (microwave signal). I have determined Fourier approximation [Eq. 2] of my input pulse and the Fourier Coefficient [A]. My understanding is that the infinite series of circuits, as described by the Telegrapher's Equation, is dependent on frequency. I also recognize that I am going to use he Coefficent [A] as my "weighted" distribution of frequencies to calculate my inherent, frequency dependent components.
Eq. 1 [tex]\frac{\partial}{\partial x} V(x,t) =L \frac{\partial}{\partial t} I(x,t)  R I(x,t)[/tex] [tex]\frac{\partial}{\partial x} I(x,t) = C \frac{\partial}{\partial t} V(x,t)  G V(x,t)[/tex] Eq. 2 [tex]\frac{1}{2T} + \sum_{n=1}^{200} a_n \cos(\frac{2\pi n t}{T}) + b_n \sin(\frac{2\pi n t}{T})[/tex] In my summation, 200 is the current limit as to not consume too much time approximating in Mathematica. where a_{n} is [tex]\frac{2}{T}\int^{\frac{T}{2}}_{0}{\cos(\frac{2 \pi n t}{T})[/tex] and b_{n} is [tex]\frac{2}{T}\int^{\frac{T}{2}}_{0}{\sin(\frac{2 \pi n t}{T})[/tex] NB: I am only using an integration for half of my period because the squarewave is 1 from 0 to [tex]\frac{T}{2}[/tex] and 0 from [tex]\frac{T}{2}[/tex] to [tex]T[/tex]; Therefore, the second half of the period has an integration of zero. My Fourier Coefficient is represented by [tex]b_n[/tex], since [tex]a_n[/tex] is effectively zero. Therefore, my "weighted" frequency formula, that determines the frequency dependent terms of the Telegrapher's Equation is [tex]b_n[/tex]. Now, I have to admit, I know I should solve [Eq.1] with Dirichlet approach, due to the boundary conditions, but that is the limit of my knowledge on the matter. I want to know what my pulse looks like at some t, or z. Can anyone offer some insight into solving this initial equation and determining the dispersed signal's wave equation? NB2: As I am using Mathematica, I can attach the existing notebook if desired. 


#2
Dec1410, 07:24 AM

P: 1,235

bearphys,
As you have included resistive terms, this equation has (now) some dispersive properties. All modes wil not be travelling at the same speed and the shape of a multimodal pulse will be modified during propagation. Without the resistive terms, the propagation speed is v= w/k = eps 1/sqrt(LC) , where w is the angular frequency, k is the wavevector and v the wave velocity, and eps means +1 or 1 . It could be interresting to start by the analysis of weak damping. When r and G are small enough, the wave will simply show an additional damping given by: w/k = eps 1/sqrt(LC)  i (R/L+G/C)/(2k) (this is a dispersion relation, approximated first order for small R and G) (i is the imaginary constant = sqrt(1)) (calculation to be checked) This indicates that short wavelengths (large k) will be less attenuated than long wavelengths. Indeed, in complex notation, the wave will be represented by this kind of spacetime dependance: exp(i(k z  w t)) where w and k are related by the dispersion relation. The time dependence can always be represented by a fourier series, of course. However, what you are looking for the decay of the signal along the transmission line. Therefore, you need now to concentrate on representing the spatial dependance. In your representation, you might assume that the an and bn are functions of z. You need then to develop the differential equations for these functions. 


#3
Dec1410, 07:55 AM

P: 1,235

I just realised there is a good wiki on transmission lines .
This wiki does even provide a compact approximate solution valid when the resistive terms are small enough: In that case you can see that the dispersion is simply due to the decay of the wave. Because of the decay along the line, the pulse is deformed. Note how obvious this solution is again, except for the precise expression of the decay index. You could use this approximation to get some insight on your method. Indeed, by expanding this approximate solution in Fourier series, would could have a taste of what you are looking for. Later on, you could try to get a general method valid even for large resistive terms, or for other sources of dispersion. 


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