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		<title>Dupin cyclide</title>
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		<updated>2014-02-02T01:46:24Z</updated>

		<summary type="html">&lt;p&gt;151.40.126.195: Corrected the definition&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;{{For|the song &amp;quot;Cesaro Summability&amp;quot; by the band Tool|Ænima}}&lt;br /&gt;
&lt;br /&gt;
In [[mathematical analysis]], &#039;&#039;&#039;Cesàro summation&#039;&#039;&#039; is an alternative means of assigning a sum to an [[Series (mathematics)|infinite series]].  If the series [[Convergent series|converges]] in the usual sense to a sum &#039;&#039;A&#039;&#039;, then the series is also Cesàro summable and has Cesàro sum &#039;&#039;A&#039;&#039;.  The significance of Cesàro summation is that a series which does not converge may still have a well-defined Cesàro sum.&lt;br /&gt;
&lt;br /&gt;
Cesàro summation is named for the Italian analyst [[Ernesto Cesàro]] (1859–1906).&lt;br /&gt;
&lt;br /&gt;
== Definition ==&lt;br /&gt;
Let {&#039;&#039;a&#039;&#039;&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;} be a [[sequence]], and let&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;s_k = a_1 + \cdots + a_k&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
be the &#039;&#039;k&#039;&#039;th [[partial sum]] of the [[Series (mathematics)|series]]&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\sum_{n=1}^\infty a_n.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The series &amp;lt;math&amp;gt;\sum_{n=1}^\infty a_n&amp;lt;/math&amp;gt; is called &#039;&#039;&#039;Cesàro summable&#039;&#039;&#039;, with Cesàro sum &amp;lt;math&amp;gt;A \in \R&amp;lt;/math&amp;gt;, if the average value of its partial sums &amp;lt;math&amp;gt;s_k&amp;lt;/math&amp;gt; tends to &amp;lt;math&amp;gt;A&amp;lt;/math&amp;gt;:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\lim_{n\to\infty} \frac{1}{n}\sum_{k=1}^n s_k = A.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
In other words, the Cesàro sum of an infinite series is the limit of the [[arithmetic mean]] ([[average]]) of the first &#039;&#039;n&#039;&#039; partial sums of the series, as &#039;&#039;n&#039;&#039; goes to infinity. It is easy to show that any [[Convergent Series|convergent series]] is Cesaro summable, and the sum of the series agrees with its Cesaro sum. However, as the first example below demonstrates, there are series that diverge but are nonetheless Cesaro summable.&lt;br /&gt;
&lt;br /&gt;
== Examples ==&lt;br /&gt;
&lt;br /&gt;
Let &#039;&#039;a&#039;&#039;&amp;lt;sub&amp;gt;&#039;&#039;n&#039;&#039;&amp;lt;/sub&amp;gt; = (&amp;amp;minus;1)&amp;lt;sup&amp;gt;&#039;&#039;n&#039;&#039;+1&amp;lt;/sup&amp;gt; for &#039;&#039;n&#039;&#039; ≥ 1.  That is, {&#039;&#039;a&#039;&#039;&amp;lt;sub&amp;gt;&#039;&#039;n&#039;&#039;&amp;lt;/sub&amp;gt;} is the sequence&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;1, -1, 1, -1, \ldots.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
and let &#039;&#039;G&#039;&#039; denote the series &amp;lt;math&amp;gt; \sum_{n=1}^\infty a_n =1-1+1-1+1-\cdots &amp;lt;/math&amp;gt;    &lt;br /&gt;
&lt;br /&gt;
Then the sequence of partial sums {&#039;&#039;s&#039;&#039;&amp;lt;sub&amp;gt;&#039;&#039;n&#039;&#039;&amp;lt;/sub&amp;gt;} &amp;lt;math&amp;gt;  = \sum_{k=1}^n a_k  &amp;lt;/math&amp;gt; is&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;1, 0, 1, 0, \ldots,\,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
so that the series &#039;&#039;G&#039;&#039;, known as [[Grandi&#039;s series]], clearly does not converge.  On the other hand, the terms of the sequence {&#039;&#039;t&#039;&#039;&amp;lt;sub&amp;gt;&#039;&#039;n&#039;&#039;&amp;lt;/sub&amp;gt;} of the (partial) means of the {&#039;&#039;s&#039;&#039;&amp;lt;sub&amp;gt;&#039;&#039;n&#039;&#039;&amp;lt;/sub&amp;gt;} where &lt;br /&gt;
:&amp;lt;math&amp;gt; t_n = \frac{1}{n}\sum_{k=1}^n s_k &amp;lt;/math&amp;gt; &lt;br /&gt;
are&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\frac{1}{1}, \,\frac{1}{2}, \,\frac{2}{3}, \,\frac{2}{4}, \,\frac{3}{5}, \,\frac{3}{6}, \,\frac{4}{7}, \,\frac{4}{8}, \,\ldots,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
so that &lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\lim_{n\to\infty} t_n = 1/2.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Therefore the Cesàro sum of the series &#039;&#039;G&#039;&#039; is 1/2.&lt;br /&gt;
&lt;br /&gt;
On the other hand, now let &#039;&#039;a&#039;&#039;&amp;lt;sub&amp;gt;&#039;&#039;n&#039;&#039;&amp;lt;/sub&amp;gt; = &#039;&#039;n&#039;&#039; for &#039;&#039;n&#039;&#039; ≥ 1.  That is, {&#039;&#039;a&#039;&#039;&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;} is the sequence&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;1, 2, 3, 4, \ldots.\,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
and let &#039;&#039;G&#039;&#039; now denote the series &amp;lt;math&amp;gt; \sum_{n=1}^\infty a_n =1+2+3+4+5+\cdots &amp;lt;/math&amp;gt;      &lt;br /&gt;
&lt;br /&gt;
Then the sequence of partial sums {&#039;&#039;s&#039;&#039;&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt;} is&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;1, 3, 6, 10, \ldots,\,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
and the evaluation of &#039;&#039;G&#039;&#039; diverges to infinity.     &lt;br /&gt;
The terms of the sequence of means of partial sums {&#039;&#039;t&#039;&#039;&amp;lt;sub&amp;gt;n&amp;lt;/sub&amp;gt; } are here&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\frac{1}{1}, \,\frac{4}{2}, \,\frac{10}{3}, \,\frac{20}{4}, \,\ldots.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Thus, this sequence diverges to infinity as well as &#039;&#039;G&#039;&#039;, and &#039;&#039;G&#039;&#039; is now &#039;&#039;&#039;not&#039;&#039;&#039; Cesàro summable. In fact, any series which diverges to (positive or negative) infinity the Cesàro method also leads to a sequence that diverges likewise, and hence such a series is not Cesàro summable.&lt;br /&gt;
&lt;br /&gt;
==(C, α) summation==&lt;br /&gt;
&lt;br /&gt;
In 1890, Ernesto Cesàro stated a broader family of summation methods which have since been called (C, &#039;&#039;n&#039;&#039;) for non-negative integers &#039;&#039;n&#039;&#039;. The (C, 0) method is just ordinary summation, and (C, 1) is Cesàro summation as described above.&lt;br /&gt;
&lt;br /&gt;
The higher-order methods can be described as follows: given a series Σ&#039;&#039;a&#039;&#039;&amp;lt;sub&amp;gt;&#039;&#039;n&#039;&#039;&amp;lt;/sub&amp;gt;, define the quantities&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;A_n^{-1}=a_n;\quad A_n^\alpha=\sum_{k=0}^n A_k^{\alpha-1}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
and define &#039;&#039;E&#039;&#039;&amp;lt;sub&amp;gt;&#039;&#039;n&#039;&#039;&amp;lt;/sub&amp;gt;&amp;lt;sup&amp;gt;α&amp;lt;/sup&amp;gt; to be &#039;&#039;A&#039;&#039;&amp;lt;sub&amp;gt;&#039;&#039;n&#039;&#039;&amp;lt;/sub&amp;gt;&amp;lt;sup&amp;gt;α&amp;lt;/sup&amp;gt; for the series 1 + 0 + 0 + 0 + · · ·. Then the (C, α) sum of Σ&#039;&#039;a&#039;&#039;&amp;lt;sub&amp;gt;&#039;&#039;n&#039;&#039;&amp;lt;/sub&amp;gt; is denoted by (C, α)-Σ&#039;&#039;a&#039;&#039;&amp;lt;sub&amp;gt;&#039;&#039;n&#039;&#039;&amp;lt;/sub&amp;gt; and has the value&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;(C,\alpha)-\sum_{j=0}^\infty a_j=\lim_{n\to\infty}\frac{A_n^\alpha}{E_n^\alpha}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
if it exists {{harv|Shawyer|Watson|1994|loc=pp.16-17}}. This description represents an &amp;lt;math&amp;gt;\alpha&amp;lt;/math&amp;gt;-times iterated application of the initial summation method and can be restated as &lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;(C,\alpha)-\sum_{j=0}^\infty a_j = \lim_{n\to\infty} \sum_{j=0}^n \frac{{n \choose j}}{{n+\alpha \choose j}} a_j.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Even more generally, for &amp;lt;math&amp;gt;\alpha\in\mathbb{R}\setminus(-\mathbb{N})&amp;lt;/math&amp;gt;, let &#039;&#039;A&#039;&#039;&amp;lt;sub&amp;gt;&#039;&#039;n&#039;&#039;&amp;lt;/sub&amp;gt;&amp;lt;sup&amp;gt;α&amp;lt;/sup&amp;gt; be implicitly given by the coefficients of the series&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\sum_{n=0}^\infty A_n^\alpha x^n=\frac{\displaystyle{\sum_{n=0}^\infty a_nx^n}}{(1-x)^{1+\alpha}},&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
and &#039;&#039;E&#039;&#039;&amp;lt;sub&amp;gt;&#039;&#039;n&#039;&#039;&amp;lt;/sub&amp;gt;&amp;lt;sup&amp;gt;α&amp;lt;/sup&amp;gt; as above.  In particular, &#039;&#039;E&#039;&#039;&amp;lt;sub&amp;gt;&#039;&#039;n&#039;&#039;&amp;lt;/sub&amp;gt;&amp;lt;sup&amp;gt;α&amp;lt;/sup&amp;gt; are the [[binomial coefficient#Newton&#039;s binomial series|binomial coefficients]] of power &amp;amp;minus;1&amp;amp;nbsp;&amp;amp;minus;&amp;amp;nbsp;α.  Then the (C, α) sum of Σ&amp;amp;nbsp;&#039;&#039;a&#039;&#039;&amp;lt;sub&amp;gt;&#039;&#039;n&#039;&#039;&amp;lt;/sub&amp;gt; is defined as above.&lt;br /&gt;
&lt;br /&gt;
The existence of a (C, α) summation implies every higher order summation, and also that &#039;&#039;a&#039;&#039;&amp;lt;sub&amp;gt;&#039;&#039;n&#039;&#039;&amp;lt;/sub&amp;gt;&amp;amp;nbsp;=&amp;amp;nbsp;&#039;&#039;o&#039;&#039;(&#039;&#039;n&#039;&#039;&amp;lt;sup&amp;gt;α&amp;lt;/sup&amp;gt;) if α&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;&amp;amp;minus;1.&lt;br /&gt;
&lt;br /&gt;
== Cesàro summability of an integral ==&lt;br /&gt;
Let α ≥ 0.  The [[integral]] &amp;lt;math&amp;gt;\scriptstyle{\int_0^\infty f(x)\,dx}&amp;lt;/math&amp;gt; is Cesàro summable (C, α) if&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\lim_{\lambda\to\infty}\int_0^\lambda\left(1-\frac{x}{\lambda}\right)^\alpha f(x)\, dx &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
exists and is finite {{harv|Titchmarsh|1948|loc=§1.15}}.  The value of this limit, should it exist, is the (C, α) sum of the integral.  Analogously to the case of the sum of a series, if α=0, the result is convergence of the [[improper integral]].  In the case α=1, (C, 1) convergence is equivalent to the existence of the limit&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\lim_{\lambda\to \infty}\frac{1}{\lambda}\int_0^\lambda\left\{\int_0^xf(y)\, dy\right\}\,dx&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
which is the limit of means of the partial integrals.&lt;br /&gt;
&lt;br /&gt;
As is the case with series, if an integral is (C,α) summable for some value of α&amp;amp;nbsp;≥&amp;amp;nbsp;0, then it is also (C,β) summable for all β&amp;amp;nbsp;&amp;gt;&amp;amp;nbsp;α, and the value of the resulting limit is the same.&lt;br /&gt;
&lt;br /&gt;
== See also ==&lt;br /&gt;
* [[Abel summation]]&lt;br /&gt;
* [[Abel&#039;s summation formula]]&lt;br /&gt;
* [[Abel–Plana formula]]&lt;br /&gt;
* [[Borel summation]]&lt;br /&gt;
* [[Euler summation]]&lt;br /&gt;
* [[Lambert summation]]&lt;br /&gt;
* [[Cesàro mean]]&lt;br /&gt;
* [[Divergent series]]&lt;br /&gt;
* [[Fejér&#039;s theorem]]&lt;br /&gt;
* [[Riesz mean]]&lt;br /&gt;
* [[Perron&#039;s formula]]&lt;br /&gt;
* [[Abelian and tauberian theorems]]&lt;br /&gt;
* [[Silverman–Toeplitz theorem]]&lt;br /&gt;
* [[Summation by parts]]&lt;br /&gt;
&lt;br /&gt;
==References==&lt;br /&gt;
*{{citation |last1=Shawyer|first1=Bruce|first2=Bruce|last2=Watson |title=Borel&#039;s Methods of Summability: Theory and Applications |publisher=Oxford UP |year=1994 |id=ISBN 0-19-853585-6}}.&lt;br /&gt;
* {{citation|last=Titchmarsh|first=E|authorlink=Edward Charles Titchmarsh|title=Introduction to the theory of Fourier integrals|isbn=978-0-8284-0324-5|year=1948|edition=2nd|publication-date=1986|publisher=Chelsea Pub. Co.|location=New York, N.Y.}}.&lt;br /&gt;
* {{springer|title=Cesàro summation methods|first=I.I.|last=Volkov|year=2001|id=c/c021360}}&lt;br /&gt;
* {{citation|title=Trigonometric series|first=Antoni|last=Zygmund|authorlink=Antoni Zygmund|publisher=Cambridge University Press|year=1968|publication-date=1988|isbn=978-0-521-35885-9|edition=2nd}}.&lt;br /&gt;
&lt;br /&gt;
{{DEFAULTSORT:Cesaro summation}}&lt;br /&gt;
&lt;br /&gt;
[[Category:Summability methods]]&lt;/div&gt;</summary>
		<author><name>151.40.126.195</name></author>
	</entry>
	<entry>
		<id>https://en.formulasearchengine.com/w/index.php?title=Gabriel_Lam%C3%A9&amp;diff=1647</id>
		<title>Gabriel Lamé</title>
		<link rel="alternate" type="text/html" href="https://en.formulasearchengine.com/w/index.php?title=Gabriel_Lam%C3%A9&amp;diff=1647"/>
		<updated>2013-12-26T10:34:58Z</updated>

		<summary type="html">&lt;p&gt;151.40.54.238: removed redundancy&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[Image:triangle-td and fd.png|thumb|400px|A bandlimited triangle wave pictured in the time domain (top) and frequency domain (bottom). The fundamental is at 220 Hz (A3).]]&lt;br /&gt;
{{Listen|filename=220 Hz anti-aliased triangle wave.ogg|title=Triangle wave sound sample|description=5 seconds of triangle wave at 220 Hz|format=[[Ogg]]}}&lt;br /&gt;
&lt;br /&gt;
A &#039;&#039;&#039;triangle wave&#039;&#039;&#039; is a [[non-sinusoidal waveform]] named for its [[Triangle|triangular]] shape.  It is a [[periodic function|periodic]], [[piecewise linear function|piecewise linear]], [[continuous function|continuous]] [[function of a real variable|real function]].&lt;br /&gt;
&lt;br /&gt;
Like a [[square wave]], the triangle wave contains only odd [[harmonic]]s, due to its [[Even and odd functions|odd symmetry]]. However, the higher harmonics [[roll-off|roll off]] much faster than in a square wave (proportional to the inverse square of the harmonic number as opposed to just the inverse).&lt;br /&gt;
&lt;br /&gt;
==Harmonics==&lt;br /&gt;
[[Image:Synthesis triangle.gif|thumb|350px|right|Animation of the additive synthesis of a triangle wave with an increasing number of harmonics. See [[Fourier_Transform | Fourier Analysis]] for a mathematical description. ]]&lt;br /&gt;
&lt;br /&gt;
It is possible to approximate a triangle wave with [[additive synthesis]] by adding odd harmonics of the fundamental, multiplying every (4n−1)th harmonic by −1 (or changing its phase by π), and rolling off the harmonics by the inverse square of their relative frequency to the [[Fundamental frequency|fundamental]]. &lt;br /&gt;
&lt;br /&gt;
This infinite [[Fourier series]] converges to the triangle wave:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;&lt;br /&gt;
\begin{align}&lt;br /&gt;
x_\mathrm{triangle}(t) &amp;amp; {} = \frac {8}{\pi^2} \sum_{k=0}^\infty (-1)^k \, \frac{ \sin \left( (2k+1) t \right)}{(2k+1)^2} \\&lt;br /&gt;
&amp;amp; {} = \frac{8}{\pi^2} \left( \sin ( t)-{1 \over 9} \sin (3 t)+{1 \over 25} \sin (5 t) - \cdots \right)&lt;br /&gt;
\end{align}&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==Definitions==&lt;br /&gt;
[[Image:Waveforms.svg|thumb|400px|[[sine wave|Sine]], [[square wave|square]], triangle, and [[sawtooth wave|sawtooth]] waveforms]]&lt;br /&gt;
&lt;br /&gt;
Another definition of the triangle wave, with range from -1 to 1 and period 2&#039;&#039;a&#039;&#039; is:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; x(t)=\frac{2}{a} \left (t-a \left \lfloor\frac{t}{a}+\frac{1}{2} \right \rfloor \right )(-1)^\left \lfloor\frac{t}{a}+\frac{1}{2} \right \rfloor&amp;lt;/math&amp;gt;&lt;br /&gt;
:where the symbol &amp;lt;math&amp;gt;\scriptstyle \lfloor n \rfloor&amp;lt;/math&amp;gt; represent the [[Floor and ceiling functions|floor function]] of &#039;&#039;n&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
Also, the triangle wave can be the absolute value of the [[sawtooth wave]]:&amp;lt;br&amp;gt;&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; x(t)= \left | 2 \left ( {t \over a} - \left \lfloor {t \over a} + {1 \over 2} \right \rfloor \right) \right | &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
or, for a range from -1 to +1: &lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; x(t)= 2 \left | 2 \left ( {t \over a} - \left \lfloor {t \over a} + {1 \over 2} \right \rfloor \right) \right | - 1 &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The triangle wave can also be expressed as the integral of the square wave:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\int\sgn(\sin(x))\,dx\,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
A simple equation with a period of 4, with &amp;lt;math&amp;gt;y(0) = 1&amp;lt;/math&amp;gt;. &lt;br /&gt;
As this only uses the [[modulo operation]] and [[absolute value]], this can be used to simply implement a triangle wave on hardware electronics with less CPU power:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;y(x) = |x\,\bmod\,4 - 2|-1&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
or, a more complex and complete version of the above equation with a period of 2π and starting with &amp;lt;math&amp;gt;y(0) = 0&amp;lt;/math&amp;gt;:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;y(x) = \left|4\left(\left(\frac{x}{2\pi} - 0.25\right)\,\bmod\,1\right) - 2\right|-1&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
In terms of sine and arcsine with period &#039;&#039;p&#039;&#039; and amplitude &#039;&#039;a&#039;&#039;:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;y(x) = \frac{2a}{\pi}\arcsin\left(\sin\left(\frac{2\pi}{p}x\right)\right)&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==See also==&lt;br /&gt;
* [[List of periodic functions]]&lt;br /&gt;
* [[Triangle function]]&lt;br /&gt;
* [[Wave]]s&lt;br /&gt;
* [[Sound]]&lt;br /&gt;
* [[Zigzag]]&lt;br /&gt;
&lt;br /&gt;
==References==&lt;br /&gt;
*{{MathWorld|urlname=FourierSeriesTriangleWave|title=Fourier Series - Triangle Wave}}&lt;br /&gt;
&lt;br /&gt;
{{DEFAULTSORT:Triangle Wave}}&lt;br /&gt;
[[Category:Fourier series]]&lt;br /&gt;
[[Category:Waveforms]]&lt;/div&gt;</summary>
		<author><name>151.40.54.238</name></author>
	</entry>
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