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shconfidence.html
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shconfidence.html
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<h1 id="shconfidence">SHConfidence</h1>
<p>Compute the probability that two functions are correlated at a given spherical harmonic degree for a given correlation coefficient.</p>
<h1 id="usage">Usage</h1>
<p><code>prob</code> = SHConfidence (<code>l</code>, <code>corr</code>)</p>
<h1 id="parameters">Parameters</h1>
<dl>
<dt><code>prob</code> : output, real*8</dt>
<dd>Probability that two functions expressed in spherical coefficients with spectral correlation <code>corr</code> are correlated at degree <code>l</code>.
</dd>
<dt><code>l</code> : input, integer</dt>
<dd>The spherical harmonic degree.
</dd>
<dt><code>corr</code> : input, real*8</dt>
<dd>The correlation coefficient of the two data sets at degree <code>l</code>.
</dd>
</dl>
<h1 id="description">Description</h1>
<p><code>SHConfidence</code> will calculate the probability (between 0 and 1) that two sets of spherical harmonic coefficients with spectral correlation <code>corr</code> are linearly correlated at a given degree. This is calculated using equation A7 from Pauer et al. (2006).</p>
<h1 id="references">References</h1>
<p>Pauer, M, K. Fleming, and O. Cadek, Modeling the dynamic component of the geoid and topography of Venus, J. Geophys. Res., 111, E11012, doi:10.1029/2005JE002511, 2006.</p>
<h1 id="see-also">See also</h1>
<p><a href="shadmitcorr.html">shadmitcorr</a>, <a href="shpowerspectrum.html">shpowerspectrum</a>, <a href="shcrosspowerspectrum.html">shcrosspowerspectrum</a></p>
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> <a href="../../../index.html" class="dir">Home</a> > <a href="../../documentation.html" class="dir">Documentation</a> > <a href="../../f95-routines.html" class="dir">Fortran 95</a> > <a href="../../gspectra.html" class="dir">Global Spectral Analysis</a></p>
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<td class="c1"><a href="http://www.ipgp.fr/">Institut de Physique du Globe de Paris</a></td>
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<td class="c3">© 2015 <a href="http://www.ipgp.fr/~wieczor">Mark Wieczorek</a></td>
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