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CLIOwin 6.5 PCI User's Manual - Audiomatica Srl

CLIOwin 6.5 PCI User's Manual - Audiomatica Srl

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evaluation; in this case only the data between the start and stop time is analyzed; each<br />

successive slice considers time data from its relative start time (the rearmost, at time<br />

zero, has start time equal to the start window of MLS) to the fixed stop time, the data<br />

being windowed by a particular time window with a smoothed rising edge (see literature<br />

for a discussion about this). Normal values for the Window Rise Time lie within 0.1 and<br />

0.6ms. In CSD mode, should the Time Shift value be left at zero, the routine will<br />

automatically calculate it, spacing the selected Number of Spectra in the interval defined<br />

by start and stop times; if Time Shift is forced by the user be sure to set it small enough<br />

to permit the last spectra to be calculated; if the fixed stop time is passed, then the<br />

calculation defaults as in case of zero Time Shift.<br />

When representing a CSD the program automatically hides the low frequency<br />

part of the spectra that has become unreliable due to the time-frequency<br />

uncertainty principle.<br />

ETF (Energy Time Frequency) is intended for room acoustic evaluation; in this case<br />

all MLS data starting from the start time are computed; then, successive slices are<br />

calculated moving their initial point of the Time Shift value.<br />

12.3.2 FILE DISPLAY MODE SETTINGS AND OPERATION<br />

Root File Name and browse button<br />

Name of one file within the set to be displayed. Pressing the associated button it is<br />

possible to browse the disk and choose the file.<br />

Z-Start<br />

Value associated to the first (rearmost) file.<br />

Z-Stop<br />

Value associated to the first (foremost) file.<br />

Z-Ref<br />

Value associated to the file to be taken as reference.<br />

Start Frequency<br />

Start frequency of the waterfall.<br />

Stop Frequency<br />

Stop frequency of the waterfall.<br />

File display mode is a powerful way for synthesizing a large number of measurements<br />

in a single 3-D graph. This mode allow the representation of the polar response of a<br />

loudspeaker taken as successive frequency responses saved in files.<br />

In order to identify the set of files it is important that all of their names follow a particular<br />

syntax, that give certain information to the processing routines.<br />

The syntax follows: .MLS.<br />

NAME is a common file name, UNITS are the common measurement units (to be<br />

displayed in the graph as Z axis label) and VALUE is a unique value identifying the single<br />

file; these quantities needs to be separated by spaces, it is possible to give negative<br />

numbers to VALUE. For example 'mydriver deg -250.mls' is a valid file name: as the<br />

name tells it is a measurement named mydriver with units deg taken at -2.5 (250<br />

divided by 100) units value.<br />

It is possible to identify one file within the set as reference with the Z-ref value; all<br />

calculations will then be made referenced to it.<br />

Please refer to 12.5 for an example.<br />

Chapter 12 - Waterfall 119

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