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11 <title>Cross-spectral density estimates (LTPDA Toolbox)</title>
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14 <meta name="description" content=
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15 "Presents an overview of the features, system requirements, and starting the toolbox.">
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16 </head>
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21 <p style="font-size:1px;"> </p>
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25 <tr>
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26 <td valign="baseline"><b>LTPDA Toolbox</b></td><td><a href="../helptoc.html">contents</a></td>
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27
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28 <td valign="baseline" align="right"><a href=
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29 "sigproc_psd.html"><img src="b_prev.gif" border="0" align=
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30 "bottom" alt="Power spectral density estimates"></a> <a href=
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31 "sigproc_cohere.html"><img src="b_next.gif" border="0" align=
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32 "bottom" alt="Cross coherence estimates"></a></td>
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33 </tr>
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34 </table>
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35
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36 <h1 class="title"><a name="f3-12899" id="f3-12899"></a>Cross-spectral density estimates</h1>
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37 <hr>
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38
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39 <p>
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40 <h2>Description</h2>
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41 <p>
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42 Cross-power spectral density is performed by the Welch's averaged, modified periodogram method.
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43 The LTPDA method <a href="matlab:doc('ao/cpsd')">ao/cpsd</a> estimates the cross-spectral density of time-series
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44 signals, included in the input <tt>ao</tt>s following the Welch's averaged, modified periodogram method <a href="#references">[1]</a>.
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45 Data are windowed prior to the estimation of the spectra, by multiplying
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46 it with a <a href="specwin.html">spectral window object</a>, and can be detrended by polinomial of time in order to reduce the impact
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47 of the border discontinuities. The window length is adjustable to shorter lenghts to reduce the spectral
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48 density uncertainties, and the percentage of subsequent window overlap can be adjusted as well.
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49 <br>
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50 <br>
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51 <h2>Syntax</h2>
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52 </p>
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53 <div class="fragment"><pre>
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54 <br> b = cpsd(a1,a2,pl)
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55 </pre>
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56 </div>
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57 <p>
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58 <tt>a1</tt> and <tt>a2</tt> are the 2 <tt>ao</tt>s containing the input time series to be evaluated, <tt>b</tt> is the output object,
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59 and <tt>pl</tt> is an optional parameters list.
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60 <h2>Parameters</h2>
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61 The parameter list <tt>pl</tt> includes the following parameters:</p>
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62 <ul>
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63 <li> <tt>'Nfft'</tt> - number of samples in each fft [default: length of input data]
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64 A string value containing the variable 'fs' can
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65 also be used, e.g., plist('Nfft', '2*fs') </li>
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66 <li> <tt>'Win'</tt> - the window to be applied to the data to remove the
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67 discontinuities at edges of segments. [default: taken from user prefs].<br>
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68 The window is described by a string with its name and, only in the case of Kaiser window,
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69 the additional parameter <tt>'psll'</tt>. <br>For instance: plist('Win', 'Kaiser', 'psll', 200). </li>
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70 <li> <tt>'Olap'</tt> - segment percent overlap [default: -1, (taken from window function)] </li>
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71 <li> <tt>'Order'</tt> - order of segment detrending <ul>
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72 <li> -1 - no detrending </li>
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73 <li> 0 - subtract mean [default] </li>
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74 <li> 1 - subtract linear fit </li>
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75 <li> N - subtract fit of polynomial, order N </li> </ul> </li>
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76 <li><tt>'Navs'</tt> - number of averages. If set, and if Nfft was set to 0 or -1, the number of points for each window will be calculated to match the request. [default: -1, not set] </li>
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77 <li><tt>'Times'</tt> - interval of time to evaluate the calculation on. If empty [default], it will take the whole section.</li>
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78 </ul>
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79 <p>
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80 The length of the window is set by the value of the parameter <tt>'Nfft'</tt>, so that the window
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81 is actually rebuilt using only the key features of the window, i.e. the name and, for Kaiser windows, the PSLL.
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82 </p>
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83
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84 <p>As an alternative to setting the number of points <tt>'Nfft'</tt> in each window, it's possible to ask for a given number of CPSD estimates by setting the <tt>'Navs'</tt> parameter, and the algorithm takes care of calculating the correct window length, according to the amount of overlap between subsequent segments.</p>
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85 <p>
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86 <table cellspacing="0" class="note" summary="Note" cellpadding="5" border="1">
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87 <tr width="90%">
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88 <td>
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89 If the user doesn't specify the value of a given parameter, the default value is used.
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90 </td>
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91 </tr>
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92 </table>
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93 </p>
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94
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95 <p>
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96 The function makes CPSD estimates between the 2 input <tt>ao</tt>s. The input argument
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97 list must contain 2 analysis objects, and the output will contain the CPSD estimate.
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98 If passing two identical objects <tt>ai</tt>, the output will be equivalent to the output of <tt>psd(ai)</tt>.
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99 </p>
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100 </pre> </div>
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101 </p>
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102 <p>
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103 <h2>Algorithm</h2>
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104 <p>
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105 The algorithm is based in standard MATLAB's tools, as the ones used by <a href="matlab:doc('pwelch')">pwelch</a>. However, in order to
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106 compute the standard deviation of mean for each frequency bin, the averaging of the different segments is performed using Welford's
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107 algorithm <a href="#references">[2]</a> which allows to compute mean and variance in one loop.
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108 </p>
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109 <h2>Example</h2>
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110 </p>
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111 <p>
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112 Evaluation of the CPSD of two time-series represented by: a low frequency sinewave signal superimposed to
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113 white noise, and a low frequency sinewave signal at the same frequency, phase shifted and with different
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114 amplitude, superimposed to white noise.
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115 </p>
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116 <div class="fragment"><pre>
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117 nsecs = 1000;
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118 x = ao(plist(<span class="string">'waveform'</span>,<span class="string">'sine wave'</span>,<span class="string">'f'</span>,0.1,<span class="string">'A'</span>,1,<span class="string">'nsecs'</span>,nsecs,<span class="string">'fs'</span>,10)) + ...
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119 ao(plist(<span class="string">'waveform'</span>,<span class="string">'noise'</span>,<span class="string">'type'</span>,<span class="string">'normal'</span>,<span class="string">'nsecs'</span>,nsecs,<span class="string">'fs'</span>,10));
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120 x.setYunits(<span class="string">'m'</span>);
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121 y = ao(plist(<span class="string">'waveform'</span>,<span class="string">'sine wave'</span>,<span class="string">'f</span>',0.1,<span class="string">'A'</span>,2,<span class="string">'nsecs'</span>,nsecs,<span class="string">'fs'</span>,10,<span class="string">'phi'</span>,90)) + ...
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122 4*ao(plist(<span class="string">'waveform'</span>,<span class="string">'noise'</span>,<span class="string">'type'</span>,<span class="string">'normal'</span>,<span class="string">'nsecs'</span>,nsecs,<span class="string">'fs'</span>,10));
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123 y.setYunits(<span class="string">'V'</span>);
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124 z = cpsd(x,y,plist(<span class="string">'nfft'</span>,1000));
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125 iplot(z);
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126 </pre>
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127 </div>
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128
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129 <img src="images/cpsd_1.png" alt="" border="3">
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130 <br>
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131
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132 <h2><a name="references">References</a></h2>
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133
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134 <ol>
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135 <li> P.D. Welch, The Use of Fast Fourier Transform for the Estimation of Power Spectra: A Method Based on Time Averaging Over Short,
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136 Modified Periodograms, <i>IEEE Trans. on Audio and Electroacoustics</i>, Vol. 15, No. 2 (1967), pp. 70 - 73</a></li>
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137 <li> B. P. Weldford, Note on a Method for Calculating Corrected Sums of Squares and Products,
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138 <i>Technometrics<i>, Vol. 4, No. 3 (1962), pp 419 - 420.</li>
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139 </ol>
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140
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141
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142
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143
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144
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145 </p>
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146
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147 <br>
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148 <br>
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149 <table class="nav" summary="Navigation aid" border="0" width=
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150 "100%" cellpadding="0" cellspacing="0">
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151 <tr valign="top">
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152 <td align="left" width="20"><a href="sigproc_psd.html"><img src=
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153 "b_prev.gif" border="0" align="bottom" alt=
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154 "Power spectral density estimates"></a> </td>
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155
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156 <td align="left">Power spectral density estimates</td>
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157
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158 <td> </td>
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159
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160 <td align="right">Cross coherence estimates</td>
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161
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162 <td align="right" width="20"><a href=
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163 "sigproc_cohere.html"><img src="b_next.gif" border="0" align=
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164 "bottom" alt="Cross coherence estimates"></a></td>
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165 </tr>
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166 </table><br>
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167
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168 <p class="copy">©LTP Team</p>
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169 </body>
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170 </html>
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