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		<summary type="html">&lt;p&gt;117.211.27.60: /* Regression analysis */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;{{about|the Airy special function|the Airy stress function employed in solid mechanics|Stress functions}}&lt;br /&gt;
&lt;br /&gt;
In the physical sciences, the &#039;&#039;&#039;Airy function&#039;&#039;&#039; &#039;&#039;&#039;Ai(&#039;&#039;x&#039;&#039;)&#039;&#039;&#039; is a [[special function]] named after the British astronomer [[George Biddell Airy]] (1801–92). The function Ai(&#039;&#039;x&#039;&#039;) and the related function &#039;&#039;&#039;Bi(&#039;&#039;x&#039;&#039;)&#039;&#039;&#039;, which is also called the &#039;&#039;&#039;Airy function&#039;&#039;&#039;, but sometimes referred to as the Bairy function, are solutions to the [[differential equation]] &lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\frac{d^2y}{dx^2} - xy = 0 , \,\!&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
known as the &#039;&#039;&#039;Airy equation&#039;&#039;&#039; or the &#039;&#039;&#039;Stokes equation&#039;&#039;&#039;. This is the simplest second-order [[linear differential equation]] with a turning point (a point where the character of the solutions changes from oscillatory to exponential).&lt;br /&gt;
&lt;br /&gt;
The Airy function is the solution to [[Schrödinger&#039;s equation]] for a particle confined within a triangular [[potential well]] and for a particle in a one-dimensional constant force field. For the same reason, it also serves to provide uniform semiclassical approximations near a turning point in the [[WKB method]], when the potential may be locally approximated by a linear function of position. The triangular potential well solution is directly relevant for the understanding of many semiconductor devices.  &lt;br /&gt;
&lt;br /&gt;
The Airy function also underlies the form of the intensity near an optical directional [[caustic (optics)|caustic]], such as that of the [[rainbow]]. Historically, this was the mathematical problem that led Airy to develop this special function. The Airy function is also important in [[microscopy]] and [[astronomy]]; it describes the pattern, due to [[diffraction]] and [[interference]], produced by a [[point source]] of light (one which is smaller than the resolution limit of a [[microscope]] or [[telescope]]).&lt;br /&gt;
&lt;br /&gt;
==Definitions==&lt;br /&gt;
[[Image:Airy Functions.svg|right|thumb|400px|Plot of Ai(&#039;&#039;x&#039;&#039;) in red and Bi(&#039;&#039;x&#039;&#039;) in blue]]&lt;br /&gt;
For real values of &#039;&#039;x&#039;&#039;, the Airy function of the first kind can be defined by the [[improper Riemann integral]]:&lt;br /&gt;
:&amp;lt;math&amp;gt;\mathrm{Ai}(x) = \frac{1}{\pi}\int_0^\infty\cos\left(\tfrac{t^3}{3} + xt\right)\, dt\equiv \frac{1}{\pi}\lim_{b\to\infty} \int_0^b \cos\left(\tfrac{t^3}{3} + xt\right)\, dt,&amp;lt;/math&amp;gt;&lt;br /&gt;
which converges because the positive and negative parts of the [[Riemann-Lebesgue lemma|rapid oscillations tend to cancel one another out]] (as can be checked by [[integration by parts]]). &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;y&#039;&#039; = Ai(&#039;&#039;x&#039;&#039;) satisfies the Airy equation &lt;br /&gt;
:&amp;lt;math&amp;gt;y&#039;&#039; - xy = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
This equation has two [[linear independence|linearly independent]] solutions. &lt;br /&gt;
Up to scalar multiplication, Ai(&#039;&#039;x&#039;&#039;) is the solution subject to the condition &#039;&#039;y&#039;&#039; → 0 as &#039;&#039;x&#039;&#039; → ∞. &lt;br /&gt;
The standard choice for the other solution is the Airy function of the second kind, denoted Bi(&#039;&#039;x&#039;&#039;). It is defined as the solution with the same amplitude of oscillation as Ai(&#039;&#039;x&#039;&#039;) as &#039;&#039;x&#039;&#039; → −∞ which differs in phase by π/2:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\mathrm{Bi}(x) = \frac{1}{\pi} \int_0^\infty \left[\exp\left(-\tfrac{t^3}{3} + xt\right) + \sin\left(\tfrac{t^3}{3} + xt\right)\,\right]dt.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==Properties==&lt;br /&gt;
The values of Ai(&#039;&#039;x&#039;&#039;) and Bi(&#039;&#039;x&#039;&#039;) and their derivatives at &#039;&#039;x&#039;&#039; = 0 are given by&lt;br /&gt;
:&amp;lt;math&amp;gt;\begin{align}&lt;br /&gt;
 \mathrm{Ai}(0) &amp;amp;{}= \frac{1}{3^{\frac{2}{3}}\Gamma(\tfrac23)}, &amp;amp; \quad \mathrm{Ai}&#039;(0) &amp;amp;{}= -\frac{1}{3^{\frac{1}{3}}\Gamma(\tfrac13)}, \\&lt;br /&gt;
 \mathrm{Bi}(0) &amp;amp;{}= \frac{1}{3^{\frac{1}{6}}\Gamma(\tfrac23)}, &amp;amp; \quad \mathrm{Bi}&#039;(0) &amp;amp;{}= \frac{3^{\frac{1}{6}}}{\Gamma(\tfrac13)}.&lt;br /&gt;
\end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
Here, Γ denotes the [[Gamma function]]. It follows that the [[Wronskian]] of Ai(&#039;&#039;x&#039;&#039;) and Bi(&#039;&#039;x&#039;&#039;) is 1/π.&lt;br /&gt;
&lt;br /&gt;
When &#039;&#039;x&#039;&#039; is positive, Ai(&#039;&#039;x&#039;&#039;) is positive, [[convex function|convex]], and decreasing exponentially to zero, while Bi(&#039;&#039;x&#039;&#039;) is positive, convex, and increasing exponentially. When &#039;&#039;x&#039;&#039; is negative, Ai(&#039;&#039;x&#039;&#039;) and Bi(&#039;&#039;x&#039;&#039;) oscillate around zero with ever-increasing frequency and ever-decreasing amplitude. This is supported by the asymptotic formulae below for the Airy functions.&lt;br /&gt;
&lt;br /&gt;
The Airy functions are orthogonal&amp;lt;ref&amp;gt;David E. Aspnes, Physical Review, &#039;&#039;&#039;147&#039;&#039;&#039;, 554 (1966)&amp;lt;/ref&amp;gt; in the sense that&lt;br /&gt;
:&amp;lt;math&amp;gt; \int_{-\infty}^\infty \mathrm{Ai}(t+x) \mathrm{Ai}(t+y) dt = \delta(x-y)&amp;lt;/math&amp;gt;&lt;br /&gt;
again using an improper Riemann integral.&lt;br /&gt;
&lt;br /&gt;
==Asymptotic formulae==&lt;br /&gt;
As explained below, the Airy functions can be extended to the complex plane, giving [[entire function]]s. The asymptotic behaviour of the Airy functions as &#039;&#039;|z|&#039;&#039; goes to infinity at a constant value of arg(&#039;&#039;z&#039;&#039;) depends on arg(&#039;&#039;z&#039;&#039;). For |arg(&#039;&#039;z&#039;&#039;)| &amp;lt; π we have the following [[asymptotic formula]] for Ai(&#039;&#039;z&#039;&#039;):&amp;lt;ref&amp;gt;{{harvtxt|Abramowitz|Stegun|1970|p=[http://people.math.sfu.ca/~cbm/aands/page_448.htm 448]}}, Eqns 10.4.59 and 10.4.63&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\mathrm{Ai}(z)\sim \frac{e^{-\frac{2}{3}z^{\frac{3}{2}}}}{2\sqrt\pi\,z^{\frac{1}{4}}}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
and a similar one for Bi(&#039;&#039;z&#039;&#039;), but only applicable when |arg(&#039;&#039;z&#039;&#039;)| &amp;lt; π/3:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\mathrm{Bi}(z)\sim \frac{e^{\frac{2}{3}z^{\frac{3}{2}}}}{\sqrt\pi\,z^{\frac{1}{4}}}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
A more accurate formula for Ai(&#039;&#039;z&#039;&#039;) and a formula for Bi(&#039;&#039;z&#039;&#039;) when π/3 &amp;lt; |arg(&#039;&#039;z&#039;&#039;)| &amp;lt; π or, equivalently, for Ai(−&#039;&#039;z&#039;&#039;) and Bi(−&#039;&#039;z&#039;&#039;) when |arg(&#039;&#039;z&#039;&#039;)| &amp;lt; 2π/3 but not zero, are:&amp;lt;ref&amp;gt;{{harvtxt|Abramowitz|Stegun|1970|p=[http://people.math.sfu.ca/~cbm/aands/page_448.htm 448]}}, Eqns 10.4.60 and 10.4.64&amp;lt;/ref&amp;gt;&lt;br /&gt;
:&amp;lt;math&amp;gt;\begin{align}&lt;br /&gt;
 \mathrm{Ai}(-z) &amp;amp;{}\sim \frac{\sin \left(\frac23z^{\frac{3}{2}}+\frac{\pi}{4} \right)}{\sqrt\pi\,z^{\frac{1}{4}}} \\[6pt]&lt;br /&gt;
 \mathrm{Bi}(-z) &amp;amp;{}\sim \frac{\cos \left(\frac23z^{\frac{3}{2}}+\frac{\pi}{4} \right)}{\sqrt\pi\,z^{\frac{1}{4}}}. &lt;br /&gt;
\end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
When |arg(&#039;&#039;z&#039;&#039;)| = 0 these are good approximations but are not asymptotic because the ratio between Ai(−&#039;&#039;z&#039;&#039;) or Bi(−&#039;&#039;z&#039;&#039;) and the above approximation goes to infinity whenever the sine or cosine goes to zero.&lt;br /&gt;
[[Asymptotic analysis|Asymptotic expansions]] for these limits are also available. These are listed in (Abramowitz and Stegun, 1954) and (Olver, 1974).&lt;br /&gt;
&lt;br /&gt;
==Complex arguments==&lt;br /&gt;
We can extend the definition of the Airy function to the complex plane by&lt;br /&gt;
:&amp;lt;math&amp;gt;\mathrm{Ai}(z) = \frac{1}{2\pi i} \int_{C} \exp\left(\tfrac{t^3}{3} - zt\right)\, dt,&amp;lt;/math&amp;gt;&lt;br /&gt;
where the integral is over a path &#039;&#039;C&#039;&#039; starting at the point at infinity with argument −π/2 and ending at the point at infinity with argument π/2. Alternatively, we can use the differential equation &#039;&#039;y&#039;&#039;′′ − &#039;&#039;xy&#039;&#039; = 0 to extend Ai(&#039;&#039;x&#039;&#039;) and Bi(&#039;&#039;x&#039;&#039;) to [[entire function]]s on the complex plane.&lt;br /&gt;
&lt;br /&gt;
The asymptotic formula for Ai(&#039;&#039;x&#039;&#039;) is still valid in the complex plane if the principal value of &#039;&#039;x&#039;&#039;&amp;lt;sup&amp;gt;2/3&amp;lt;/sup&amp;gt; is taken and &#039;&#039;x&#039;&#039; is bounded away from the negative real axis. The formula for Bi(&#039;&#039;x&#039;&#039;) is valid provided &#039;&#039;x&#039;&#039; is in the sector {&#039;&#039;x&#039;&#039; ∈ &#039;&#039;&#039;C&#039;&#039;&#039; : |arg(&#039;&#039;x&#039;&#039;)| &amp;lt; (π/3)−δ} for some positive δ. Finally, the formulae for Ai(−&#039;&#039;x&#039;&#039;) and Bi(−&#039;&#039;x&#039;&#039;) are valid if &#039;&#039;x&#039;&#039; is in the sector {&#039;&#039;x&#039;&#039; ∈ &#039;&#039;&#039;C&#039;&#039;&#039; : |arg(&#039;&#039;x&#039;&#039;)| &amp;lt; (2π/3)−δ}.&lt;br /&gt;
&lt;br /&gt;
It follows from the asymptotic behaviour of the Airy functions that both Ai(&#039;&#039;x&#039;&#039;) and Bi(&#039;&#039;x&#039;&#039;) have an infinity of zeros on the negative real axis. The function Ai(&#039;&#039;x&#039;&#039;) has no other zeros in the complex plane, while the function Bi(&#039;&#039;x&#039;&#039;) also has infinitely many zeros in the sector {&#039;&#039;z&#039;&#039; ∈ &#039;&#039;&#039;C&#039;&#039;&#039; : π/3 &amp;lt; |arg(&#039;&#039;z&#039;&#039;)| &amp;lt; π/2}.&lt;br /&gt;
&lt;br /&gt;
===Plots===&lt;br /&gt;
&lt;br /&gt;
{| style=&amp;quot;text-align:center&amp;quot; align=center&lt;br /&gt;
! &amp;lt;math&amp;gt;\Re \left[ \mathrm{Ai} ( x + iy) \right] &amp;lt;/math&amp;gt;&lt;br /&gt;
! &amp;lt;math&amp;gt;\Im \left[ \mathrm{Ai} ( x + iy) \right] &amp;lt;/math&amp;gt;&lt;br /&gt;
! &amp;lt;math&amp;gt;| \mathrm{Ai} ( x + iy) | \, &amp;lt;/math&amp;gt;&lt;br /&gt;
! &amp;lt;math&amp;gt;\mathrm{arg} \left[ \mathrm{Ai} ( x + iy) \right] \, &amp;lt;/math&amp;gt;&lt;br /&gt;
|-&lt;br /&gt;
|[[Image:AiryAi Real Surface.png|200px]]&lt;br /&gt;
|[[Image:AiryAi Imag Surface.png|200px]]&lt;br /&gt;
|[[Image:AiryAi Abs Surface.png|200px]]&lt;br /&gt;
|[[Image:AiryAi Arg Surface.png|200px]]&lt;br /&gt;
|-&lt;br /&gt;
|[[Image:AiryAi Real Contour.svg|200px]]&lt;br /&gt;
|[[Image:AiryAi Imag Contour.svg|200px]]&lt;br /&gt;
|[[Image:AiryAi Abs Contour.svg|200px]]&lt;br /&gt;
|[[Image:AiryAi Arg Contour.svg|200px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{| style=&amp;quot;text-align:center&amp;quot; align=center&lt;br /&gt;
! &amp;lt;math&amp;gt;\Re \left[ \mathrm{Bi} ( x + iy) \right] &amp;lt;/math&amp;gt;&lt;br /&gt;
! &amp;lt;math&amp;gt;\Im \left[ \mathrm{Bi} ( x + iy) \right] &amp;lt;/math&amp;gt;&lt;br /&gt;
! &amp;lt;math&amp;gt;| \mathrm{Bi} ( x + iy) | \, &amp;lt;/math&amp;gt;&lt;br /&gt;
! &amp;lt;math&amp;gt;\mathrm{arg} \left[ \mathrm{Bi} ( x + iy) \right] \, &amp;lt;/math&amp;gt;&lt;br /&gt;
|-&lt;br /&gt;
|[[Image:AiryBi Real Surface.png|200px]]&lt;br /&gt;
|[[Image:AiryBi Imag Surface.png|200px]]&lt;br /&gt;
|[[Image:AiryBi Abs Surface.png|200px]]&lt;br /&gt;
|[[Image:AiryBi Arg Surface.png|200px]]&lt;br /&gt;
|-&lt;br /&gt;
|[[Image:AiryBi Real Contour.svg|200px]]&lt;br /&gt;
|[[Image:AiryBi Imag Contour.svg|200px]]&lt;br /&gt;
|[[Image:AiryBi Abs Contour.svg|200px]]&lt;br /&gt;
|[[Image:AiryBi Arg Contour.svg|200px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==Relation to other special functions==&lt;br /&gt;
For positive arguments, the Airy functions are related to the [[Bessel function#Modified Bessel functions|modified Bessel functions]]:&lt;br /&gt;
:&amp;lt;math&amp;gt;\begin{align}&lt;br /&gt;
 \mathrm{Ai}(x) &amp;amp;{}= \frac1\pi \sqrt{\frac{x}{3}} \, K_{\frac{1}{3}}\left(\tfrac23 x^{\frac{3}{2}}\right), \\&lt;br /&gt;
 \mathrm{Bi}(x) &amp;amp;{}= \sqrt{\frac{x}{3}} \left(I_{\frac{1}{3}}\left(\tfrac23 x^{\frac{3}{2}}\right) + I_{-\frac{1}{3}}\left(\tfrac23 x^{\frac{3}{2}}\right)\right).&lt;br /&gt;
\end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
Here, &#039;&#039;I&#039;&#039;&amp;lt;sub&amp;gt;±1/3&amp;lt;/sub&amp;gt; and &#039;&#039;K&#039;&#039;&amp;lt;sub&amp;gt;1/3&amp;lt;/sub&amp;gt; are solutions of &lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;x^2y&#039;&#039; + xy&#039; - \left (x^2 + \tfrac{1}{9} \right )y = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The first derivative of Airy function is&lt;br /&gt;
:&amp;lt;math&amp;gt;  \mathrm{Ai&#039;}(x) = - \frac{x} {\pi \sqrt{3}} \, K_{\frac{2}{3}}\left(\tfrac23 x^{\frac{3}{2}}\right) .&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Functions &#039;&#039;K&#039;&#039;&amp;lt;sub&amp;gt;1/3&amp;lt;/sub&amp;gt; and &#039;&#039;K&#039;&#039;&amp;lt;sub&amp;gt;2/3&amp;lt;/sub&amp;gt; can  be represented in terms of rapidly converged integrals&amp;lt;ref&amp;gt;M.Kh.Khokonov. Cascade Processes of Energy Loss by Emission of Hard Photons //  JETP, V.99, No.4, pp. 690-707 \ (2004).&amp;lt;/ref&amp;gt; (see also [[Bessel function#Modified Bessel functions|modified Bessel functions]] )&lt;br /&gt;
&lt;br /&gt;
For negative arguments, the Airy function are related to the [[Bessel function]]s:&lt;br /&gt;
:&amp;lt;math&amp;gt;\begin{align}&lt;br /&gt;
 \mathrm{Ai}(-x) &amp;amp;{}= \sqrt{\frac{x}{9}} \left(J_{\frac{1}{3}}\left(\tfrac23 x^{\frac{3}{2}}\right) + J_{-\frac{1}{3}}\left(\tfrac23 x^{\frac{3}{2}}\right)\right), \\&lt;br /&gt;
 \mathrm{Bi}(-x) &amp;amp;{}= \sqrt{\frac{x}{3}} \left(J_{-\frac{1}{3}}\left(\tfrac23 x^{\frac{3}{2}}\right) - J_{\frac{1}{3}}\left(\tfrac23 x^{\frac{3}{2}}\right)\right). &lt;br /&gt;
\end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
Here, &#039;&#039;J&#039;&#039;&amp;lt;sub&amp;gt;±1/3&amp;lt;/sub&amp;gt; are solutions of &lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;x^2y&#039;&#039; + xy&#039; + \left (x^2 - \tfrac{1}{9} \right )y = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The [[Scorer&#039;s function]]s solve the equation &#039;&#039;y&#039;&#039;′′ − &#039;&#039;xy&#039;&#039; = 1/π. They can also be expressed in terms of the Airy functions:&lt;br /&gt;
:&amp;lt;math&amp;gt;\begin{align}&lt;br /&gt;
 \mathrm{Gi}(x) &amp;amp;{}= \mathrm{Bi}(x) \int_x^\infty \mathrm{Ai}(t) \, dt + \mathrm{Ai}(x) \int_0^x \mathrm{Bi}(t) \, dt, \\&lt;br /&gt;
 \mathrm{Hi}(x) &amp;amp;{}= \mathrm{Bi}(x) \int_{-\infty}^x \mathrm{Ai}(t) \, dt - \mathrm{Ai}(x) \int_{-\infty}^x \mathrm{Bi}(t) \, dt. &lt;br /&gt;
\end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==Fourier transform==&lt;br /&gt;
Using the definition of the Airy function Ai(&#039;&#039;x&#039;&#039;), it is straightforward to show its [[Fourier transform]] is given by&lt;br /&gt;
:&amp;lt;math&amp;gt;\mathcal{F}(\mathrm{Ai})(k) := \int_{-\infty}^{\infty} \mathrm{Ai}(x)\ e^{- 2\pi i k x}\,dx = e^{\frac{i}{3}(2\pi k)^3}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==Fabry–Pérot interferometer Airy Function==&lt;br /&gt;
The transmittance function of a [[Fabry–Pérot interferometer]] is also referred to as the &#039;&#039;Airy Function&#039;&#039;:&amp;lt;ref&amp;gt;{{cite book | first=Eugene|last=Hecht|year=1987|title=Optics|edition=2nd ed.|publisher=Addison Wesley|isbn=0-201-11609-X}} Sect. 9.6&amp;lt;/ref&amp;gt;&lt;br /&gt;
:&amp;lt;math&amp;gt;T_e = \frac{1}{1+F\sin^2(\frac{\delta}{2})},&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where both surfaces have reflectance &#039;&#039;R&#039;&#039; and&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; F = \frac{4R}{{(1-R)^2}}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
is the &#039;&#039;coefficient of finesse&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
==History==&lt;br /&gt;
The Airy function is named after the [[British (people)|British]] [[astronomer]] and [[physicist]] [[George Biddell Airy]] (1801–1892), who encountered it in his early study of [[optics]] in physics (Airy 1838). The notation Ai(&#039;&#039;x&#039;&#039;) was introduced by [[Harold Jeffreys]]. Airy had become the British [[Astronomer Royal]] in 1835, and he held that post until his retirement in 1881.&lt;br /&gt;
&lt;br /&gt;
==See also==&lt;br /&gt;
&lt;br /&gt;
*The proof of [[Witten&#039;s conjecture]] used a matrix-valued generalization of the Airy function.&lt;br /&gt;
*[[Airy zeta function]]&lt;br /&gt;
&lt;br /&gt;
==Notes==&lt;br /&gt;
&amp;lt;references /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==References==&lt;br /&gt;
*{{AS ref|10|446}}&lt;br /&gt;
* {{citation|last=Airy |year=1838|title= On the intensity of light in the neighbourhood of a caustic|journal=Transactions of the Cambridge Philosophical Society|volume=6|pages= 379–402|url=http://books.google.com/?id=-yI8AAAAMAAJ&amp;amp;dq=Transactions+of+the+Cambridge+Philosophical+Society+1838|publisher=University Press}}&lt;br /&gt;
* Olver (1974). &#039;&#039;Asymptotics and Special Functions,&#039;&#039; Chapter&amp;amp;nbsp;11. Academic Press, New York.&lt;br /&gt;
* {{Citation | last1=Press | first1=WH | last2=Teukolsky | first2=SA | last3=Vetterling | first3=WT | last4=Flannery | first4=BP | year=2007 | title=Numerical Recipes: The Art of Scientific Computing | edition=3rd | publisher=Cambridge University Press |  publication-place=New York | isbn=978-0-521-88068-8 | chapter=Section 6.6.3. Airy Functions | chapter-url=http://apps.nrbook.com/empanel/index.html#pg=289}}&lt;br /&gt;
* {{Citation | last1=Vallée | first1=Olivier | last2=Soares | first2=Manuel | title=Airy functions and applications to physics | url=http://www.worldscibooks.com/physics/p345.html | publisher=Imperial College Press | location=London | isbn=978-1-86094-478-9 | mr=2114198 | year=2004}}&lt;br /&gt;
&lt;br /&gt;
==External links==&lt;br /&gt;
* {{springer|title=Airy functions|id=p/a011210}}&lt;br /&gt;
* {{MathWorld | urlname=AiryFunctions | title=Airy Functions}}&lt;br /&gt;
* Wolfram function pages for [http://functions.wolfram.com/Bessel-TypeFunctions/AiryAi/ Ai] and [http://functions.wolfram.com/Bessel-TypeFunctions/AiryBi/ Bi] functions. Includes formulas, function evaluator, and plotting calculator.&lt;br /&gt;
* {{dlmf|title= Airy and related functions |id=9|first=F. W. J.|last= Olver}}&lt;br /&gt;
&lt;br /&gt;
[[Category:Special functions]]&lt;br /&gt;
[[Category:Special hypergeometric functions]]&lt;br /&gt;
[[Category:Ordinary differential equations]]&lt;/div&gt;</summary>
		<author><name>117.211.27.60</name></author>
	</entry>
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