Find the centroid (centre of mass when the surface density is
constant) of the frustum of the circular cone
Surface density r
= constant |
|
Taking moments about the x-y plane:
DMz =
z Dm
Therefore the centroid of the frustum of the cone is at
Find the total flux that passes through the hemisphere
using:
the surface projection method and
S:
x 2 + y 2
+ z 2
= a 2, z > 0
(by symmetry)
But everywhere on the hemisphere r = a
Switch to plane polar coordinates, in which
dA = r dr
df.
x = r cos f,
y = r
sin f,
Þ
x 2 + y 2 =
r 2
everywhere on the hemisphere
Use the parameters
(q, f)
(0 £ q £ p/2,
0 £ f <
2p).
[Note: this vector N
has a different magnitude from the vector N
in part (a) of this question.]
But everywhere on the hemisphere r = a
What can you say about the relative orientation of the vector field D and the normal N to the hemisphere?
From part (b) above, vectors D and N are both multiples of the displacement vector r. D and N are therefore parallel to each other everywhere on the hemisphere.
Find the total flux of the vector field
through that part of the
circular paraboloid
Projection method:
z = 4 - x 2
- y 2
(first octant only)
Use plane polar coordinates
x =
r cos f,
y = r sin f,
Þ
x 2 + y 2 =
r 2
Þ
z = 4 - r 2
and
Therefore
Net flux through S = p. |
or
Surface parametric net method:
Use parameters r and
f:
x =
r cos f,
y = r sin f,
z =
4 - r 2
A thin sheet, in the shape of the paraboloid
It lies within the coaxial region between the circular cylinders
and
In order to obtain a better visualization of the surface S, examine its projection onto any vertical plane containing the z-axis and its projection onto the x-y plane:
Let r 2 = x 2
+ y 2, then the paraboloid is
z =
16 - r 2
Cylinder C1 is
r 2 = 1
Cylinder C2 is
r 2 = 9
The sheet is therefore defined by
z = 16 - r 2,
7 £ z
£ 15,
x ³ 0 ,
y ³ 0.
Surface parametric net method:
Use parameters (r, f):
1 £ r
£ 3 ,
0 £ f £ p/2
The surface density then becomes
Total mass:
Therefore (assuming S.I. units)
Total mass = 10 kg |
Projection Method:
z = 16 -
(x 2 + y 2)
Convert to plane polar coordinates:
Therefore (assuming S.I. units)
Total mass = 10 kg |
Elements of first moments:
DMx =
x . Dm =
x r DS
= x r N
Dr Df
By symmetry,
DMz =
z . Dm =
z r DS
= z r N
Dr
Df
Therefore the centre of mass is at
Or, to 3 d.p.,
(1.613, 1.613, 9.933) |
Fluid is flowing along a cylindrical pipe. The circular
cross section inside the pipe has a constant radius of
a (m).
The Cartesian coordinate system is aligned with the x axis
along the line of symmetry (centre line) of the pipe. The other
two axes are in the plane of one of the circular cross sections.
The velocity of fluid at any point
Find the flux Q (in m3/s) (the
rate at which fluid is flowing through the pipe).
The x-z and y-z planes are illustrated here,
together with the velocity profile in the former case:
The speed increases from zero on the wall of the pipe to a maximum
of v 0 along the centre line.
The flux Q is the flux of the velocity vector
v of the fluid across a circular cross
section in the direction of a unit normal to that cross section.
The unit normal is
Transform to plane polar coordinates:
[We can also verify that this answer is dimensionally
consistent:
the units on the right side are [m s–1] ×
[m]2 = [m3 s–1]
which are the units for volume per unit time.]
Complete the evaluation (in Example 2.6.3 of the lecture notes)
of the line integral
around the unit square in the x-z plane for
,
(without using Stokes’ theorem).
From example 2.6.3, the positive orientation
around the square is OGHJ (the y axis is
directed into the page).
In the x-z plane y = 0
Compute the line integral around the four sides of the
square, starting with OG:
The above was presented in a lecture.
Below are the calculations for the other three sides of the
square:
Therefore
Use a parametric net (q, f)
that is a close relative of the spherical polar coordinate
system:
x = 2 sin q cos f ,
y = 2 sin q sin f ,
z = cos q
Þ
x2 + y2 =
4 sin2q
and
x2 + y2
+ 4z2 =
4 sin2q +
4 cos2q = 4
The parameter ranges are 0 <
q < p/2 ,
0 < f < 2p
Employ the abbreviations
cq =
cos q ,
sq =
sin q ,
cf =
cos f ,
sf =
sin f
Therefore
By symmetry,
Taking moments about the xy-plane:
Therefore the centre of mass is at the point
The shadow of the ellipsoid on the xy-plane is
the area bounded by the circle
Everywhere on the ellipsoid,
Switch to plane polar coordinates (r, q):
Therefore
By symmetry,
Taking moments about the xy-plane:
But the projection is the region bounded by a circle of
radius 2.
Þ
A = p (2)2
Therefore the centre of mass is at the point