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SCALAR AND VECTOR FUNCTIONS, POINT FUNCTIONS, SCALAR POINT FUNCTIONS, VECTOR POINT FUNCTIONS, SCALAR AND VECTOR FIELDS



In vector analysis we deal with scalar and vector functions.


Def. Scalar function. A scalar function is a function that assigns a real number (i.e. a scalar) to a set of real variables. Its general form is


                                    u = f(x1, x2, ... , xn)


where x1, x2, ... , xn are real numbers.



Def. Vector function. A vector function is a function that assigns a vector to a set of real variables. Its general form is  


                        U = f1(x1, x2, ... , xn) i + f2(x1, x2, ... , xn) j + f3(x1, x2, ... , xn) k


or equivalently, in parametric form,


            u1 = f1(x1, x2, ... , xn)

            u2 = f2(x1, x2, ... , xn)

            u3 = f3(x1, x2, ... , xn)


where U = (u1, u2, u3) and x1, x2, ... , xn are real numbers..



Example 1. Function defining a space curve. Let


            R(t) = x(t) i + y(t) j + z(t) k


be a radius vector to a point P(x, y, z) in space which moves as t increases in value. It traces out a curve in space. The parametric representation of space curves is


            x = x(t)

            y = y(t)

            z = z(t) .


Example 2. Function defining a surface in space. The function


            R(u,v) = x(u,v) i + y(u,v) j + z(u,v) k


represents a surface in space. Surfaces are represented by parametric equations of the type


            x = x(u, v)

            y = y(u, v)

            z = z(u, v)


If v is regarded as a parameter, u a variable, then 7) describes a space curve. For each value of v there is another space curve, thus generating a surface.



Def. Point function. A point function u = f(P) is a function that assigns some number or value u to each point P of some region R of space. Examples of point functions are scalar point functions and vector point functions.



Def. Scalar point function. A scalar point function is a function that assigns a real number (i.e. a scalar) to each point of some region of space. If to each point (x, y, z) of a region R in space there is assigned a real number u = Φ(x, y, z), then Φ is called a scalar point function.

Examples. 1. The temperature distribution within some body at a particular point in time. 2. The density distribution within some fluid at a particular point in time.


Syn. scalar function of position



Scalar field. A scalar point function defined over some region is called a scalar field. A scalar field which is independent of time is called a stationary or steady-state scalar field.


A scalar field that varies with time would have the representation


            u = Φ(x, y, z, t) .



Def. Vector point function. A vector point function is a function that assigns a vector to each point of some region of space. If to each point (x, y, z) of a region R in space there is assigned a vector U =U(x, y, z), then U is called a vector point function. Such a function would have a representation


            U = u1(x, y, z) i + u2(x, y, z) j + u3(x, y, z) k


or in parametric form,


            u1 = u1(x, y, z)

            u2 = u2(x, y, z)

            u3 = u3(x, y, z)




Syn. vector function of position



Vector field. A vector point function defined over some region is called a vector field. A vector field which is independent of time is called a stationary or steady-state vector field.


A vector field that varies with time would have the representation


            U = u1(x, y, z, t) i + u2(x, y, z, t) j + u3(x, y, z, t) k


or in parametric form,


            u1 = u1(x, y, z, t)

            u2 = u2(x, y, z, t)

            u3 = u3(x, y, z, t)



Examples. 1. Gravitational field of the earth. 2. Electric field about a current-carrying wire. 3. Magnetic field generated by a magnet. 3. Velocity at different points within a moving fluid. 4. Acceleration at different points within a moving fluid.







References.


  James and James. Mathematics Dictionary.

  Murray R. Spiegel. Vector Analysis.

  Angus E. Tayor. Advanced Calculus.





Examples of vector point functions.


Force fields.


1] gravitational field


2] magnetic field near a magnet or current-carrying wire


3] electric field generated by a charge or current-carrying wire



Velocity field


1] Velocity at different points in space within a moving fluid (e.g. wind velocities in the atmosphere; particle velocities in a stream)



Acceleration field.


1] Acceleration at different points in space within a moving fluid




I Functional representation of a force field (static case).     All of the following are equivalent ways of expressing the functional representation of a static force field:



            ux = f1(x, y, z)

1]        uy = f2(x, y, z)

            uz = f3(x, y, z)


where ux, uy, and uz are the x, y and z components of the force U at point (x, y, z).



            u1 = f1(x, y, z)

2]        u2 = f2(x, y, z)

            u3 = f3(x, y, z)


            u1 = u1(x, y, z)

3]        u2 = u2(x, y, z)

            u3 = u3(x, y, z)


            u1 = u1(x1, x2, x3)

4]        u2 = u2(x1, x2, x3)

            u3 = u3(x1, x2, x3)


ole.gif  


ole1.gif  

 

7]        U = u1(x, y, z) i + u2(x, y, z) j + u3(x, y, z) k


where i, j and k are unit vectors along the coordinate axes.




● A vector field which is independent of time is called a stationary or steady-state vector field.

 




II Functional representation of a force field (dynamic case).        All of the following are equivalent ways of expressing the functional representation of a dynamic force field:



            ux = f1(x, y, z, t)

1]        uy = f2(x, y, z, t)

            uz = f3(x, y, z, t)


where ux, uy, and uz are the x, y and z components of the force U at point (x, y, z) at time t.



            u1 = f1(x, y, z, t)

2]        u2 = f2(x, y, z, t)

            u3 = f3(x, y, z, t)


            u1 = u1(x, y, z, t)

3]        u2 = u2(x, y, z, t)

            u3 = u3(x, y, z, t)


            u1 = u1(x1, x2, x3, t)

4]        u2 = u2(x1, x2, x3, t)

            u3 = u3(x1, x2, x3, t)


ole2.gif  


ole3.gif  

 

7]        U = u1(x, y, z, t) i + u2(x, y, z, t) j + u3(x, y, z, t) k


where i, j and k are unit vectors along the coordinate axes.



III Functional representation of a velocity field in a moving, turbulent fluid. The functional representation of the velocities at various points within a moving, turbulent fluid can be expressed in the following equivalent ways:


            vx = f1(x, y, z, t)

1]        vy = f2(x, y, z, t)

            vz = f3(x, y, z, t)


where vx, vy, and vz are the x, y and z components of the velocity V at point (x, y, z) at time t.



            v1 = f1(x, y, z, t)

2]        v2 = f2(x, y, z, t)

            v3 = f3(x, y, z, t)


            v1 = v1(x, y, z, t)

3]        v2 = v2(x, y, z, t)

            v3 = v3(x, y, z, t)


            v1 = v1(x1, x2, x3, t)

4]        v2 = v2(x1, x2, x3, t)

            v3 = v3(x1, x2, x3, t)


ole4.gif  


ole5.gif  

 

7]        V = v1(x, y, z, t) i + v2(x, y, z, t) j + v3(x, y, z, t) k


where i, j and k are unit vectors along the coordinate axes.




IV Functional representation of an acceleration field in a moving, turbulent fluid. The functional representation of the accelerations at various points within a moving, turbulent fluid can be expressed in the following equivalent ways:


            ax = f1(x, y, z, t)

1]        ay = f2(x, y, z, t)

            az = f3(x, y, z, t)


where ax, ay, and az are the x, y and z components of the acceleration A at point (x, y, z) at time t.



            a1 = f1(x, y, z, t)

2]        a2 = f2(x, y, z, t)

            a3 = f3(x, y, z, t)


            a1 = a1(x, y, z, t)

3]        a2 = a2(x, y, z, t)

            a3 = a3(x, y, z, t)


            a1 = a1(x1, x2, x3, t)

4]        a2 = a2(x1, x2, x3, t)

            a3 = a3(x1, x2, x3, t)


ole6.gif  


ole7.gif  

 

7]        A = a1(x, y, z, t) i + a2(x, y, z, t) j + a3(x, y, z, t) k


where i, j and k are unit vectors along the coordinate axes.


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