Carpinteria High School Football,
Valerie Robinson Obituary,
Articles A
15.6 Cylindrical and Spherical Coordinates - Whitman College \[\int\limits_{0}^{2\pi}\int\limits_{0}^{\pi}\int\limits_{0}^{\infty}\psi^*(r,\theta,\phi)\psi(r,\theta,\phi) \, r^2 \sin\theta \, dr d\theta d\phi=\int\limits_{0}^{2\pi}\int\limits_{0}^{\pi}\int\limits_{0}^{\infty}A^2e^{-2r/a_0}\,r^2\sin\theta\,dr d\theta d\phi=1 \nonumber\], \[\int\limits_{0}^{2\pi}\int\limits_{0}^{\pi}\int\limits_{0}^{\infty}A^2e^{-2r/a_0}\,r^2\sin\theta\,dr d\theta d\phi=A^2\int\limits_{0}^{2\pi}d\phi\int\limits_{0}^{\pi}\sin\theta \;d\theta\int\limits_{0}^{\infty}e^{-2r/a_0}\,r^2\;dr \nonumber\]. If the inclination is zero or 180 degrees ( radians), the azimuth is arbitrary. Two important partial differential equations that arise in many physical problems, Laplace's equation and the Helmholtz equation, allow a separation of variables in spherical coordinates. A series of astronomical coordinate systems are used to measure the elevation angle from different fundamental planes.
Spherical Coordinates -- from Wolfram MathWorld \underbrace {r \, d\theta}_{\text{longitude component}} *\underbrace {r \, \color{blue}{\sin{\theta}} \,d \phi}_{\text{latitude component}}}^{\text{area of an infinitesimal rectangle}} The Cartesian unit vectors are thus related to the spherical unit vectors by: The general form of the formula to prove the differential line element, is[5]. , Coming back to coordinates in two dimensions, it is intuitive to understand why the area element in cartesian coordinates is \(dA=dx\;dy\) independently of the values of \(x\) and \(y\). The answer is no, because the volume element in spherical coordinates depends also on the actual position of the point. Spherical coordinates are somewhat more difficult to understand. Conversely, the Cartesian coordinates may be retrieved from the spherical coordinates (radius r, inclination , azimuth ), where r [0, ), [0, ], [0, 2), by, Cylindrical coordinates (axial radius , azimuth , elevation z) may be converted into spherical coordinates (central radius r, inclination , azimuth ), by the formulas, Conversely, the spherical coordinates may be converted into cylindrical coordinates by the formulae. Find \(A\). @R.C. This is shown in the left side of Figure \(\PageIndex{2}\). $$dA=r^2d\Omega$$. These relationships are not hard to derive if one considers the triangles shown in Figure \(\PageIndex{4}\): In any coordinate system it is useful to define a differential area and a differential volume element. ( The spherical-polar basis vectors are ( e r, e , e ) which is related to the cartesian basis vectors as follows: The lowest energy state, which in chemistry we call the 1s orbital, turns out to be: This particular orbital depends on \(r\) only, which should not surprise a chemist given that the electron density in all \(s\)-orbitals is spherically symmetric. I know you can supposedly visualize a change of area on the surface of the sphere, but I'm not particularly good at doing that sadly. In three dimensions, the spherical coordinate system defines a point in space by three numbers: the distance \(r\) to the origin, a polar angle \(\phi\) that measures the angle between the positive \(x\)-axis and the line from the origin to the point \(P\) projected onto the \(xy\)-plane, and the angle \(\theta\) defined as the is the angle between the \(z\)-axis and the line from the origin to the point \(P\): Before we move on, it is important to mention that depending on the field, you may see the Greek letter \(\theta\) (instead of \(\phi\)) used for the angle between the positive \(x\)-axis and the line from the origin to the point \(P\) projected onto the \(xy\)-plane.
PDF Geometry Coordinate Geometry Spherical Coordinates A bit of googling and I found this one for you! You then just take the determinant of this 3-by-3 matrix, which can be done by cofactor expansion for instance. r These choices determine a reference plane that contains the origin and is perpendicular to the zenith. the orbitals of the atom). Notice that the area highlighted in gray increases as we move away from the origin. Why is this sentence from The Great Gatsby grammatical? The difference between the phonemes /p/ and /b/ in Japanese. Because of the probabilistic interpretation of wave functions, we determine this constant by normalization. The answer is no, because the volume element in spherical coordinates depends also on the actual position of the point. )
Phys. Rev. Phys. Educ. Res. 15, 010112 (2019) - Physics students This will make more sense in a minute.
differential geometry - Surface Element in Spherical Coordinates Be able to integrate functions expressed in polar or spherical coordinates. We also knew that all space meant \(-\infty\leq x\leq \infty\), \(-\infty\leq y\leq \infty\) and \(-\infty\leq z\leq \infty\), and therefore we wrote: \[\int_{-\infty }^{\infty }\int_{-\infty }^{\infty }\int_{-\infty }^{\infty }{\left | \psi (x,y,z) \right |}^2\; dx \;dy \;dz=1 \nonumber\]. There is an intuitive explanation for that. $$. ( vegan) just to try it, does this inconvenience the caterers and staff? - the incident has nothing to do with me; can I use this this way? Figure 6.7 Area element for a cylinder: normal vector r Example 6.1 Area Element of Disk Consider an infinitesimal area element on the surface of a disc (Figure 6.8) in the xy-plane. It is also convenient, in many contexts, to allow negative radial distances, with the convention that I want to work out an integral over the surface of a sphere - ie $r$ constant. ) (25.4.7) z = r cos . In spherical polar coordinates, the element of volume for a body that is symmetrical about the polar axis is, Whilst its element of surface area is, Although the homework statement continues, my question is actually about how the expression for dS given in the problem statement was arrived at in the first place.
The latitude component is its horizontal side. In this case, \(n=2\) and \(a=2/a_0\), so: \[\int\limits_{0}^{\infty}e^{-2r/a_0}\,r^2\;dr=\dfrac{2! ( I'm just wondering is there an "easier" way to do this (eg. The volume element spanning from r to r + dr, to + d, and to + d is specified by the determinant of the Jacobian matrix of partial derivatives, Thus, for example, a function f(r, , ) can be integrated over every point in R3 by the triple integral. The differential of area is \(dA=r\;drd\theta\). r where $B$ is the parameter domain corresponding to the exact piece $S$ of surface. This will make more sense in a minute. For example a sphere that has the cartesian equation \(x^2+y^2+z^2=R^2\) has the very simple equation \(r = R\) in spherical coordinates. Integrating over all possible orientations in 3D, Calculate the integral of $\phi(x,y,z)$ over the surface of the area of the unit sphere, Curl of a vector in spherical coordinates, Analytically derive n-spherical coordinates conversions from cartesian coordinates, Integral over a sphere in spherical coordinates, Surface integral of a vector function. Such a volume element is sometimes called an area element. where we used the fact that \(|\psi|^2=\psi^* \psi\). 180 , , $$h_1=r\sin(\theta),h_2=r$$ 4. However, the limits of integration, and the expression used for \(dA\), will depend on the coordinate system used in the integration. It is now time to turn our attention to triple integrals in spherical coordinates. 6. I am trying to find out the area element of a sphere given by the equation: r 2 = x 2 + y 2 + z 2 The sphere is centered around the origin of the Cartesian basis vectors ( e x, e y, e z). ) {\displaystyle (r,\theta ,\varphi )} Connect and share knowledge within a single location that is structured and easy to search. However, the azimuth is often restricted to the interval (180, +180], or (, +] in radians, instead of [0, 360). Intuitively, because its value goes from zero to 1, and then back to zero. ) can be written as[6]. $$x=r\cos(\phi)\sin(\theta)$$ Their total length along a longitude will be $r \, \pi$ and total length along the equator latitude will be $r \, 2\pi$. By clicking Accept all cookies, you agree Stack Exchange can store cookies on your device and disclose information in accordance with our Cookie Policy. The spherical coordinate systems used in mathematics normally use radians rather than degrees and measure the azimuthal angle counterclockwise from the x-axis to the y-axis rather than clockwise from north (0) to east (+90) like the horizontal coordinate system. Is it possible to rotate a window 90 degrees if it has the same length and width?
12.7: Cylindrical and Spherical Coordinates - Mathematics LibreTexts , \[\int\limits_{all\; space} |\psi|^2\;dV=\int\limits_{0}^{2\pi}\int\limits_{0}^{\pi}\int\limits_{0}^{\infty}\psi^*(r,\theta,\phi)\psi(r,\theta,\phi)\,r^2\sin\theta\,dr d\theta d\phi=1 \nonumber\]. These coordinates are known as cartesian coordinates or rectangular coordinates, and you are already familiar with their two-dimensional and three-dimensional representation.
Spherical charge distribution 2013 - Purdue University PDF Sp Geometry > Coordinate Geometry > Interactive Entries > Interactive . When the system is used for physical three-space, it is customary to use positive sign for azimuth angles that are measured in the counter-clockwise sense from the reference direction on the reference plane, as seen from the zenith side of the plane. But what if we had to integrate a function that is expressed in spherical coordinates? In the plane, any point \(P\) can be represented by two signed numbers, usually written as \((x,y)\), where the coordinate \(x\) is the distance perpendicular to the \(x\) axis, and the coordinate \(y\) is the distance perpendicular to the \(y\) axis (Figure \(\PageIndex{1}\), left). $$y=r\sin(\phi)\sin(\theta)$$ From (a) and (b) it follows that an element of area on the unit sphere centered at the origin in 3-space is just dphi dz. In any coordinate system it is useful to define a differential area and a differential volume element. This will make more sense in a minute. 1. (
32.4: Spherical Coordinates - Chemistry LibreTexts PDF Today in Physics 217: more vector calculus - University of Rochester }{(2/a_0)^3}=\dfrac{2}{8/a_0^3}=\dfrac{a_0^3}{4} \nonumber\], \[A^2\int\limits_{0}^{2\pi}d\phi\int\limits_{0}^{\pi}\sin\theta \;d\theta\int\limits_{0}^{\infty}e^{-2r/a_0}\,r^2\;dr=A^2\times2\pi\times2\times \dfrac{a_0^3}{4}=1 \nonumber\], \[A^2\times \pi \times a_0^3=1\rightarrow A=\dfrac{1}{\sqrt{\pi a_0^3}} \nonumber\], \[\displaystyle{\color{Maroon}\dfrac{1}{\sqrt{\pi a_0^3}}e^{-r/a_0}} \nonumber\]. This page titled 10.2: Area and Volume Elements is shared under a CC BY-NC-SA 4.0 license and was authored, remixed, and/or curated by Marcia Levitus via source content that was edited to the style and standards of the LibreTexts platform; a detailed edit history is available upon request. We will see that \(p\) and \(d\) orbitals depend on the angles as well. We already know that often the symmetry of a problem makes it natural (and easier!) The del operator in this system leads to the following expressions for the gradient, divergence, curl and (scalar) Laplacian, Further, the inverse Jacobian in Cartesian coordinates is, In spherical coordinates, given two points with being the azimuthal coordinate, The distance between the two points can be expressed as, In spherical coordinates, the position of a point or particle (although better written as a triple 1. atoms). Write the g ij matrix. (a) The area of [a slice of the spherical surface between two parallel planes (within the poles)] is proportional to its width. Computing the elements of the first fundamental form, we find that The straightforward way to do this is just the Jacobian. r For positions on the Earth or other solid celestial body, the reference plane is usually taken to be the plane perpendicular to the axis of rotation. The geometrical derivation of the volume is a little bit more complicated, but from Figure \(\PageIndex{4}\) you should be able to see that \(dV\) depends on \(r\) and \(\theta\), but not on \(\phi\). Lets see how this affects a double integral with an example from quantum mechanics. Some combinations of these choices result in a left-handed coordinate system. We also acknowledge previous National Science Foundation support under grant numbers 1246120, 1525057, and 1413739. In the conventions used, The desired coefficients are the magnitudes of these vectors:[5], The surface element spanning from to + d and to + d on a spherical surface at (constant) radius r is then, The surface element in a surface of polar angle constant (a cone with vertex the origin) is, The surface element in a surface of azimuth constant (a vertical half-plane) is. Converting integration dV in spherical coordinates for volume but not for surface? }{a^{n+1}}, \nonumber\]. This can be very confusing, so you will have to be careful. There is yet another way to look at it using the notion of the solid angle. However, modern geographical coordinate systems are quite complex, and the positions implied by these simple formulae may be wrong by several kilometers. ) Just as the two-dimensional Cartesian coordinate system is useful on the plane, a two-dimensional spherical coordinate system is useful on the surface of a sphere. \nonumber\], \[\int_{0}^{\infty}x^ne^{-ax}dx=\dfrac{n! In cartesian coordinates the differential area element is simply \(dA=dx\;dy\) (Figure \(\PageIndex{1}\)), and the volume element is simply \(dV=dx\;dy\;dz\). [2] The polar angle is often replaced by the elevation angle measured from the reference plane towards the positive Z axis, so that the elevation angle of zero is at the horizon; the depression angle is the negative of the elevation angle. Notice the difference between \(\vec{r}\), a vector, and \(r\), the distance to the origin (and therefore the modulus of the vector). Here is the picture. What happens when we drop this sine adjustment for the latitude? +
PDF Week 7: Integration: Special Coordinates - Warwick The lowest energy state, which in chemistry we call the 1s orbital, turns out to be: This particular orbital depends on \(r\) only, which should not surprise a chemist given that the electron density in all \(s\)-orbitals is spherically symmetric. A number of polar plots are required, taken at a wide selection of frequencies, as the pattern changes greatly with frequency. When using spherical coordinates, it is important that you see how these two angles are defined so you can identify which is which. We are trying to integrate the area of a sphere with radius r in spherical coordinates. The differential of area is \(dA=dxdy\): \[\int\limits_{all\;space} |\psi|^2\;dA=\int\limits_{-\infty}^{\infty}\int\limits_{-\infty}^{\infty} A^2e^{-2a(x^2+y^2)}\;dxdy=1 \nonumber\], In polar coordinates, all space means \(0
14.5: Spherical Coordinates - Chemistry LibreTexts where we used the fact that \(|\psi|^2=\psi^* \psi\). rev2023.3.3.43278. Accessibility StatementFor more information contact us atinfo@libretexts.orgor check out our status page at https://status.libretexts.org. \overbrace{ to denote radial distance, inclination (or elevation), and azimuth, respectively, is common practice in physics, and is specified by ISO standard 80000-2:2019, and earlier in ISO 31-11 (1992). Then the area element has a particularly simple form: The function \(\psi(x,y)=A e^{-a(x^2+y^2)}\) can be expressed in polar coordinates as: \(\psi(r,\theta)=A e^{-ar^2}\), \[\int\limits_{all\;space} |\psi|^2\;dA=\int\limits_{0}^{\infty}\int\limits_{0}^{2\pi} A^2 e^{-2ar^2}r\;d\theta dr=1 \nonumber\]. In cartesian coordinates the differential area element is simply \(dA=dx\;dy\) (Figure \(\PageIndex{1}\)), and the volume element is simply \(dV=dx\;dy\;dz\). $$ 6. Find \( d s^{2} \) in spherical coordinates by the | Chegg.com This will make more sense in a minute. These formulae assume that the two systems have the same origin and same reference plane, measure the azimuth angle in the same senses from the same axis, and that the spherical angle is inclination from the cylindrical z axis. The value of should be greater than or equal to 0, i.e., 0. is used to describe the location of P. Let Q be the projection of point P on the xy plane. These formulae assume that the two systems have the same origin, that the spherical reference plane is the Cartesian xy plane, that is inclination from the z direction, and that the azimuth angles are measured from the Cartesian x axis (so that the y axis has = +90). I've edited my response for you. Degrees are most common in geography, astronomy, and engineering, whereas radians are commonly used in mathematics and theoretical physics. In cartesian coordinates, the differential volume element is simply \(dV= dx\,dy\,dz\), regardless of the values of \(x, y\) and \(z\). The spherical coordinates of the origin, O, are (0, 0, 0). The same value is of course obtained by integrating in cartesian coordinates. ( Element of surface area in spherical coordinates - Physics Forums To subscribe to this RSS feed, copy and paste this URL into your RSS reader. That is, where $\theta$ and radius $r$ map out the zero longitude (part of a circle of a plane). ( Spherical coordinates are useful in analyzing systems that are symmetrical about a point. The angles are typically measured in degrees () or radians (rad), where 360=2 rad. Geometry Coordinate Geometry Spherical Coordinates Download Wolfram Notebook Spherical coordinates, also called spherical polar coordinates (Walton 1967, Arfken 1985), are a system of curvilinear coordinates that are natural for describing positions on a sphere or spheroid. Surface integrals of scalar fields. The angle $\theta$ runs from the North pole to South pole in radians. The correct quadrants for and are implied by the correctness of the planar rectangular to polar conversions. PDF Concepts of primary interest: The line element Coordinate directions Often, positions are represented by a vector, \(\vec{r}\), shown in red in Figure \(\PageIndex{1}\). The differential \(dV\) is \(dV=r^2\sin\theta\,d\theta\,d\phi\,dr\), so, \[\int\limits_{all\;space} |\psi|^2\;dV=\int\limits_{0}^{2\pi}\int\limits_{0}^{\pi}\int\limits_{0}^{\infty}\psi^*(r,\theta,\phi)\psi(r,\theta,\phi)\,r^2\sin\theta\,dr d\theta d\phi=1 \nonumber\]. When radius is fixed, the two angular coordinates make a coordinate system on the sphere sometimes called spherical polar coordinates. Other conventions are also used, such as r for radius from the z-axis, so great care needs to be taken to check the meaning of the symbols. thickness so that dividing by the thickness d and setting = a, we get Tool for making coordinates changes system in 3d-space (Cartesian, spherical, cylindrical, etc. This gives the transformation from the spherical to the cartesian, the other way around is given by its inverse. , It is also possible to deal with ellipsoids in Cartesian coordinates by using a modified version of the spherical coordinates. $$S:\quad (u,v)\ \mapsto\ {\bf x}(u,v)$$ $$\int_{-1 \leq z \leq 1, 0 \leq \phi \leq 2\pi} f(\phi,z) d\phi dz$$. In linear algebra, the vector from the origin O to the point P is often called the position vector of P. Several different conventions exist for representing the three coordinates, and for the order in which they should be written. The relationship between the cartesian coordinates and the spherical coordinates can be summarized as: \[\label{eq:coordinates_5} x=r\sin\theta\cos\phi\], \[\label{eq:coordinates_6} y=r\sin\theta\sin\phi\], \[\label{eq:coordinates_7} z=r\cos\theta\]. We'll find our tangent vectors via the usual parametrization which you gave, namely, This statement is true regardless of whether the function is expressed in polar or cartesian coordinates. One can add or subtract any number of full turns to either angular measure without changing the angles themselves, and therefore without changing the point. { "32.01:_Complex_Numbers" : "property get [Map MindTouch.Deki.Logic.ExtensionProcessorQueryProvider+<>c__DisplayClass228_0.b__1]()", "32.02:_Probability_and_Statistics" : "property get [Map MindTouch.Deki.Logic.ExtensionProcessorQueryProvider+<>c__DisplayClass228_0.b__1]()", "32.03:_Vectors" : "property get [Map MindTouch.Deki.Logic.ExtensionProcessorQueryProvider+<>c__DisplayClass228_0.b__1]()", "32.04:_Spherical_Coordinates" : "property get [Map MindTouch.Deki.Logic.ExtensionProcessorQueryProvider+<>c__DisplayClass228_0.b__1]()", "32.05:_Determinants" : "property get [Map MindTouch.Deki.Logic.ExtensionProcessorQueryProvider+<>c__DisplayClass228_0.b__1]()", "32.06:_Matrices" : "property get [Map MindTouch.Deki.Logic.ExtensionProcessorQueryProvider+<>c__DisplayClass228_0.b__1]()", "32.07:_Numerical_Methods" : "property get [Map MindTouch.Deki.Logic.ExtensionProcessorQueryProvider+<>c__DisplayClass228_0.b__1]()", "32.08:_Partial_Differentiation" : "property get [Map MindTouch.Deki.Logic.ExtensionProcessorQueryProvider+<>c__DisplayClass228_0.b__1]()", "32.09:_Series_and_Limits" : "property get [Map MindTouch.Deki.Logic.ExtensionProcessorQueryProvider+<>c__DisplayClass228_0.b__1]()", "32.10:_Fourier_Analysis" : "property get [Map MindTouch.Deki.Logic.ExtensionProcessorQueryProvider+<>c__DisplayClass228_0.b__1]()", "32.11:_The_Binomial_Distribution_and_Stirling\'s_Appromixation" : "property get [Map MindTouch.Deki.Logic.ExtensionProcessorQueryProvider+<>c__DisplayClass228_0.b__1]()" }, { "00:_Front_Matter" : "property get [Map MindTouch.Deki.Logic.ExtensionProcessorQueryProvider+<>c__DisplayClass228_0.b__1]()", "01:_The_Dawn_of_the_Quantum_Theory" : "property get [Map MindTouch.Deki.Logic.ExtensionProcessorQueryProvider+<>c__DisplayClass228_0.b__1]()", "02:_The_Classical_Wave_Equation" : "property get [Map MindTouch.Deki.Logic.ExtensionProcessorQueryProvider+<>c__DisplayClass228_0.b__1]()", "03:_The_Schrodinger_Equation_and_a_Particle_in_a_Box" : "property get [Map MindTouch.Deki.Logic.ExtensionProcessorQueryProvider+<>c__DisplayClass228_0.b__1]()", "04:_Postulates_and_Principles_of_Quantum_Mechanics" : "property get [Map MindTouch.Deki.Logic.ExtensionProcessorQueryProvider+<>c__DisplayClass228_0.b__1]()", "05:_The_Harmonic_Oscillator_and_the_Rigid_Rotor" : "property get [Map MindTouch.Deki.Logic.ExtensionProcessorQueryProvider+<>c__DisplayClass228_0.b__1]()", "06:_The_Hydrogen_Atom" : "property get [Map MindTouch.Deki.Logic.ExtensionProcessorQueryProvider+<>c__DisplayClass228_0.b__1]()", "07:_Approximation_Methods" : "property get [Map MindTouch.Deki.Logic.ExtensionProcessorQueryProvider+<>c__DisplayClass228_0.b__1]()", "08:_Multielectron_Atoms" : "property get [Map MindTouch.Deki.Logic.ExtensionProcessorQueryProvider+<>c__DisplayClass228_0.b__1]()", "09:_Chemical_Bonding_in_Diatomic_Molecules" : "property get [Map MindTouch.Deki.Logic.ExtensionProcessorQueryProvider+<>c__DisplayClass228_0.b__1]()", "10:_Bonding_in_Polyatomic_Molecules" : "property get [Map MindTouch.Deki.Logic.ExtensionProcessorQueryProvider+<>c__DisplayClass228_0.b__1]()", "11:_Computational_Quantum_Chemistry" : "property get [Map MindTouch.Deki.Logic.ExtensionProcessorQueryProvider+<>c__DisplayClass228_0.b__1]()", "12:_Group_Theory_-_The_Exploitation_of_Symmetry" : "property get [Map MindTouch.Deki.Logic.ExtensionProcessorQueryProvider+<>c__DisplayClass228_0.b__1]()", "13:_Molecular_Spectroscopy" : "property get [Map MindTouch.Deki.Logic.ExtensionProcessorQueryProvider+<>c__DisplayClass228_0.b__1]()", "14:_Nuclear_Magnetic_Resonance_Spectroscopy" : "property get [Map MindTouch.Deki.Logic.ExtensionProcessorQueryProvider+<>c__DisplayClass228_0.b__1]()", "15:_Lasers_Laser_Spectroscopy_and_Photochemistry" : "property get [Map MindTouch.Deki.Logic.ExtensionProcessorQueryProvider+<>c__DisplayClass228_0.b__1]()", "16:_The_Properties_of_Gases" : "property get [Map MindTouch.Deki.Logic.ExtensionProcessorQueryProvider+<>c__DisplayClass228_0.b__1]()", "17:_Boltzmann_Factor_and_Partition_Functions" : "property get [Map MindTouch.Deki.Logic.ExtensionProcessorQueryProvider+<>c__DisplayClass228_0.b__1]()", "18:_Partition_Functions_and_Ideal_Gases" : "property get [Map MindTouch.Deki.Logic.ExtensionProcessorQueryProvider+<>c__DisplayClass228_0.b__1]()", "19:_The_First_Law_of_Thermodynamics" : "property get [Map MindTouch.Deki.Logic.ExtensionProcessorQueryProvider+<>c__DisplayClass228_0.b__1]()", "20:_Entropy_and_The_Second_Law_of_Thermodynamics" : "property get [Map MindTouch.Deki.Logic.ExtensionProcessorQueryProvider+<>c__DisplayClass228_0.b__1]()", "21:_Entropy_and_the_Third_Law_of_Thermodynamics" : "property get [Map MindTouch.Deki.Logic.ExtensionProcessorQueryProvider+<>c__DisplayClass228_0.b__1]()", "22:_Helmholtz_and_Gibbs_Energies" : "property get [Map MindTouch.Deki.Logic.ExtensionProcessorQueryProvider+<>c__DisplayClass228_0.b__1]()", "23:_Phase_Equilibria" : "property get [Map MindTouch.Deki.Logic.ExtensionProcessorQueryProvider+<>c__DisplayClass228_0.b__1]()", "24:_Solutions_I_-_Volatile_Solutes" : "property get [Map MindTouch.Deki.Logic.ExtensionProcessorQueryProvider+<>c__DisplayClass228_0.b__1]()", "25:_Solutions_II_-_Nonvolatile_Solutes" : "property get [Map MindTouch.Deki.Logic.ExtensionProcessorQueryProvider+<>c__DisplayClass228_0.b__1]()", "26:_Chemical_Equilibrium" : "property get [Map MindTouch.Deki.Logic.ExtensionProcessorQueryProvider+<>c__DisplayClass228_0.b__1]()", "27:_The_Kinetic_Theory_of_Gases" : "property get [Map MindTouch.Deki.Logic.ExtensionProcessorQueryProvider+<>c__DisplayClass228_0.b__1]()", "28:_Chemical_Kinetics_I_-_Rate_Laws" : "property get [Map MindTouch.Deki.Logic.ExtensionProcessorQueryProvider+<>c__DisplayClass228_0.b__1]()", "29:_Chemical_Kinetics_II-_Reaction_Mechanisms" : "property get [Map MindTouch.Deki.Logic.ExtensionProcessorQueryProvider+<>c__DisplayClass228_0.b__1]()", "30:_Gas-Phase_Reaction_Dynamics" : "property get [Map MindTouch.Deki.Logic.ExtensionProcessorQueryProvider+<>c__DisplayClass228_0.b__1]()", "31:_Solids_and_Surface_Chemistry" : "property get [Map MindTouch.Deki.Logic.ExtensionProcessorQueryProvider+<>c__DisplayClass228_0.b__1]()", "32:_Math_Chapters" : "property get [Map MindTouch.Deki.Logic.ExtensionProcessorQueryProvider+<>c__DisplayClass228_0.b__1]()", Appendices : "property get [Map MindTouch.Deki.Logic.ExtensionProcessorQueryProvider+<>c__DisplayClass228_0.b__1]()", "zz:_Back_Matter" : "property get [Map MindTouch.Deki.Logic.ExtensionProcessorQueryProvider+<>c__DisplayClass228_0.b__1]()" }, [ "article:topic", "showtoc:no", "license:ccbyncsa", "Spherical Coordinates", "autonumheader:yes2", "licenseversion:40" ], https://chem.libretexts.org/@app/auth/3/login?returnto=https%3A%2F%2Fchem.libretexts.org%2FBookshelves%2FPhysical_and_Theoretical_Chemistry_Textbook_Maps%2FPhysical_Chemistry_(LibreTexts)%2F32%253A_Math_Chapters%2F32.04%253A_Spherical_Coordinates, \( \newcommand{\vecs}[1]{\overset { \scriptstyle \rightharpoonup} {\mathbf{#1}}}\) \( \newcommand{\vecd}[1]{\overset{-\!-\!\rightharpoonup}{\vphantom{a}\smash{#1}}} \)\(\newcommand{\id}{\mathrm{id}}\) \( \newcommand{\Span}{\mathrm{span}}\) \( \newcommand{\kernel}{\mathrm{null}\,}\) \( \newcommand{\range}{\mathrm{range}\,}\) \( \newcommand{\RealPart}{\mathrm{Re}}\) \( \newcommand{\ImaginaryPart}{\mathrm{Im}}\) \( \newcommand{\Argument}{\mathrm{Arg}}\) \( \newcommand{\norm}[1]{\| #1 \|}\) \( \newcommand{\inner}[2]{\langle #1, #2 \rangle}\) \( \newcommand{\Span}{\mathrm{span}}\) \(\newcommand{\id}{\mathrm{id}}\) \( \newcommand{\Span}{\mathrm{span}}\) \( \newcommand{\kernel}{\mathrm{null}\,}\) \( \newcommand{\range}{\mathrm{range}\,}\) \( \newcommand{\RealPart}{\mathrm{Re}}\) \( \newcommand{\ImaginaryPart}{\mathrm{Im}}\) \( \newcommand{\Argument}{\mathrm{Arg}}\) \( \newcommand{\norm}[1]{\| #1 \|}\) \( \newcommand{\inner}[2]{\langle #1, #2 \rangle}\) \( \newcommand{\Span}{\mathrm{span}}\)\(\newcommand{\AA}{\unicode[.8,0]{x212B}}\), status page at https://status.libretexts.org.