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Horn Research Update

Fall 2013

MSc Work

Since I have followed the Integrated PhD programme at NTNU, I did not finish my MSc until this summer (2013), even though I started om my PhD in the summer of 2011. Anyway, my MSc is now completed, and I'm working full time on my PhD.

My MSc thesis was of course also on horns, where I extended the Modal Propagation Method to rectangular horns with asymmetries. I also did an attempt on curved horns, but that was a very complex subject, as it turned out. The modes in the bend is described by Bessel functions of non-integer and imaginary order, and I also needed to find the zeros of such functions. Not that easy... You can see the result of my work here: MSc Thesis.

PhD Work

This fall I started working on the modal radiation impedance of rectangular ducts. I implemented some of this in my MSc thesis, so the basic functions for computing the radiation impedance for a horn mounted in an infinite baffle are available. However, most horns are not mounted in infinite baffles. They are mounted in finite baffles, unbaffled, or placed on the floor, near walls, in real rooms. Therefore I started looking into the influence of mutual impedance.

If a surface vibrates with a certain velocity, there will be a force pressing back on this surface due to the reaction of the air the surface moves. The force will be frequency dependent, and it will be more or less out of phase with the velocity. At low frequencies, there is nearly a 90 degree phase difference between the two, and little power is radiated. At higher frequencies they fall into phase, and the source radiates with maximum efficiency. The ratio of this force to the velocity is called the radiation impedance. 

If two or more surfaces are vibrating, or if a source vibrates near a hard wall, so that an image source is formed due to the "mirroring effect" of the wall, each source will generate a pressure on the other. The ratio of the pressure of one source to the velocity of the other is called the mutual radiation impedance. It has to be taken into account whenever sources are near walls, or when there are multiple sources.

In addition to mutual impedance, diffraction from the baffle edges for horns in finite baffles also creates pressure on the radiating surface. To quantify this effect is what I'm currently working on.

Experimental Work

All these simulation models do of course have to be checked against reality. The workshop at the university has therefore built me some pretty horns to measure. They have an aluminium inner skin, and 4 layers of 3mm MDF laminated on top of that, finished with some bracing, as shown on the picture below:

Testhorn2

Having this horn ready, I mounted it in a fairly large baffle, and measured in the anechoic chamber at the University. The test setup is shown below:

MeasureHorn2

I measured both the throat impedance using the two-microphone method, and the pressure at various points. 

Below is a graph of the measured throat impedance, compared to the impedance simulated with the Modal Propagation Method, using 16 modes in each direction. Seems like I'm on the right track with this method....

The deviations from the simulated impedance above 2.5kHz is first the cross-modes in the measurement tube, and then, above 4kHz, we can see the effect of the microphone spacing becoming less than half a wavelength. 

Measured vs Sim

This horn is intended as a 1:4 scale model of a 50Hz midbass horn. An even shorter version of it, designed to be mounted near a floor/wall intersection, is also under way. This is quite common for midbass horns, and the idea is to try out this horn at various positions in a scale model of a room. 

The general rule of thumb has been that by placing a horn near a wall, one can get away with a smaller mouth. This is not necessarily the case. Below is an example. The pale (overlay) lines are the throat impedance for the horn mounted in an infinite baffle, the same as above. The darker lines shows what happens when a wall is placed near the horn (30cm from the center of the mouth, which is 35x35cm). It is actually worse than the horn in the baffle alone.

Measured Wall30

Placing the horn nearer the wall (20cm from the center of the mouth) improves the situation. And the nearer it gets, the better. Conversely, at 40cm the impedance is much more peaky than at 30cm.

But note also that the higher frequency ripple increases. 

Measured Wall20.jpg

More data will be published on this later. But for the time being, it is worth keeping in mind that things are not as simple as rules of thumb may lead us to believe. Especially with horns.

Modes in horns

Not only plane or spherical waves propagate in horns. Above a certain frequency, the wave front becomes much more complex, and this complex wave front can be described as a weighted sum of mode functions.

You may be familiar with standing waves in rooms. These standing waves can only exist at certain frequencies, and their shape is given by the so-called boundary conditions. For a room with hard walls, the boundary condition is that the velocity perpendicular to the wall should be zero. That means that the pressure has its maximum values at the walls. A room will have modes in all three directions, and the pressure at any point will be a sum of the contributions from all excited modes.

Another example of modes is the vibration of a string. A string is fixed at the ends, so the boundary condition is that the displacement should be zero at the ends. The mode functions for displacement are sine functions. Then the string can vibrate with shapes that are sums of sine functions that can fulfil the condition of zero displacement at the ends.

In horns, the pressure distribution across a cross-section can also be viewed as a sum of mode functions that meet the boundary conditions. For an axisymmetric horn, using a plane cross section, these functions can be cylindrical Bessel functions. These are the mode functions for a cylindrical tube of constant cross section. A horn can be approximated by a series of short, cylindrical tubes. At each change of cross section, the mode functions in the two tubes must be matched. The mode functions will not be the same in the two tubes. This means that a single mode coming to a change in cross section will generate a series of other modes in the following duct. This is known as mode coupling.

This fact can be used to simulate horns, by letting the wave at the throat propagate through the horn, generating new modes at each change in cross section, and letting them propagate or decay through the next part of the horn, and so on. A method to do this is described by Kemp in his thesis. During my project in Numerical Acoustics this fall (2011), I implemented this method and compared it to BEM. The report can be found here. The end result was in very good agreement with BERIM (a boundary element method for horns in infinite baffles), and much faster. I plan to make the method available, hopefully both as a little Windows executable, and as a Matlab toolbox. Update: The Matlab toolbox is available here.

Update: Spring 2012 I undertook a more detailed evaluation of the modal propagation method, to check the accuracy and computation times etc. The report can be downloaded here.

 

This is my first blog post here. I'm not sure how much time I will devote to writing blog posts, but I hope to put up something here every now and then. Anyway, this is my 

Horn Research Blog.

This summer (2011) I was accepted for the integrated PhD programme at NTNU, the Norwegian University of Science and Technology. My thesis will be on horns for domestic use. All this means that I'm officially a horn researcher! 

The integrated PhD means that I will be doing my Masters in parallel with the first year of the PhD. So far I have not had much time to do proper horn research. But I have been working on an article on finite horns, and a simulation method for horns that includes higher order modes. 

That concludes my first posting.