Vector fields in polar coordinates A vector field in polar coordinates has the form F ( r , θ ) = F ( r , θ ) u r + g ( r , θ ) u θ , where the unit vectors are defined in Exercise 62 . Sketch the following vector fields and express them in Cartesian coordinates. 62. Vectors in ℝ 2 may also be expressed in terms of polar coordinates. The standard coordinate unit vectors in polar coordinates are denoted u r and u θ (see figure). Unlike the coordinate unite vectors in Cartesian coordinates, u r and u θ change their direction depending on the point ( r , θ ). Use the figure to show that for r > 0, the following relationships among the unit vectors in Cartesian and polar coordinates hold: u r = cos θ i + sin θ j i = u r cos θ − u θ sin θ u θ = sin θ i + cos θ j j = u r sin θ + u θ cos θ 66. F = r u θ
Vector fields in polar coordinates A vector field in polar coordinates has the form F ( r , θ ) = F ( r , θ ) u r + g ( r , θ ) u θ , where the unit vectors are defined in Exercise 62 . Sketch the following vector fields and express them in Cartesian coordinates. 62. Vectors in ℝ 2 may also be expressed in terms of polar coordinates. The standard coordinate unit vectors in polar coordinates are denoted u r and u θ (see figure). Unlike the coordinate unite vectors in Cartesian coordinates, u r and u θ change their direction depending on the point ( r , θ ). Use the figure to show that for r > 0, the following relationships among the unit vectors in Cartesian and polar coordinates hold: u r = cos θ i + sin θ j i = u r cos θ − u θ sin θ u θ = sin θ i + cos θ j j = u r sin θ + u θ cos θ 66. F = r u θ
Solution Summary: The author explains how to sketch the vector field and express it in Cartesian coordinates.
Vector fields in polar coordinates A vector field in polar coordinates has the form F(r, θ) = F(r, θ) ur + g(r, θ) uθ, where the unit vectors are defined in Exercise 62. Sketch the following vector fields and express them in Cartesian coordinates.
62. Vectors in ℝ2 may also be expressed in terms of polar coordinates. The standard coordinate unit vectors in polar coordinates are denoted ur and uθ (see figure). Unlike the coordinate unite vectors in Cartesian coordinates, ur and uθ change their direction depending on the point (r, θ). Use the figure to show that for r > 0, the following relationships among the unit vectors in Cartesian and polar coordinates hold:
ur = cos θi + sin θj i = ur cos θ − uθ sin θ
uθ = sin θi + cos θj j = ur sin θ + uθ cos θ
66. F = ruθ
Quantities that have magnitude and direction but not position. Some examples of vectors are velocity, displacement, acceleration, and force. They are sometimes called Euclidean or spatial vectors.
Given that the outward flux of a vector field through the sphere of radius r centered at the origin is
5(1 cos(2r)) sin(r), and D is the value of the divergence of the vector field at the origin, the value of sin (2D) is
-0.998
0.616
0.963
0.486
0.835
-0.070
-0.668
-0.129
10
The hypotenuse of a right triangle has one end at the origin and one end on the curve y =
Express the area of the triangle as a function of x.
A(x) =
In Problems 17-26, solve the initial value problem.
17. dy = (1+ y²) tan x, y(0) = √√3
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