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Practice Midterm 1 Solution Material Type: Notes; Professor: Auroux; Class: Multivariable Calculus; Subject: Mathematics; University: University of California - Berkeley; Term: Fall 2010;
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1
0
2 − 2 y
2 y− 2
y dxdy.
b) By symmetry ¯x = 0.
D
r
2 ρ rdrdθ =
2 π
0
1
0
r
2 |r cos θ|rdrdθ = 4
π/ 2
0
1
0
r
4 cos θdrdθ = 4
π/ 2
0
cos θdθ =
2 , 0 ≤ x ≤ 1: so
C
yx
3 dx + y
2 dy =
1
0
x
2 x
3 dx + (x
2 )
2 (2xdx) =
1
0
3 x
5 dx =
2
2 , Py = ax
2
2
. Qx = Py provided a = 6 and b = 3.
b) fx = 6x
2 y + y
3
3 y + xy
3
3
2
′ (y).
Comparing this with Q, we get 2x
3
2
′ (y) = 2x
3
2
′ (y) = 2 and g = 2y + c. So
f = 2x
3
y + xy
3
c) C starts at (1, 0) and ends at (−e
π , 0), so
C
F · d~r = f (−e
π , 0) − f (1, 0) = −e
−π − 1.
u x
u y
vx vy
2 x/y −x
2 /y
2
y x
= 3x
2
/y. Therefore, dudv = | 3 x
2 /y| dxdy = 3|u| dxdy
and hence dx dy =
3 |u|
du dv.
b)
R
dx dy =
4
2
5
1
3 u
dudv =
4
2
ln 5 dv =
ln 5.
C
M dx =
R
−My dA. (Green’s theorem)
b) We want M such that −M y
= (x + y)
2
. We can use e.g. M = −
(x + y)
3 .
F = 2y, so
C
F · nˆ ds =
R
2 y dA =
1
0
x
3
0
2 y dydx =
1
0
x
6
dx =
b) For the flux through C 1 , ˆn = −ˆ implies
F · nˆ = −(1 + y
2 ) = −1 where y = 0. The length
of C 1
is 1, so the total flux through C 1
is
C 1
(−1) ds = −1. The flux through C 2
is zero because
nˆ = ˆı and
F ⊥ ˆı.
c)
C 3
F · ˆn ds =
C 1 +C 2 +C 3
F · nˆ ds −
C 1
F · nˆ ds −
C 2
F · nˆ ds =
¡
¡ ¡
¡ ¡
1
1
π/ 2
0
1
0
1
0
r
2 r dz dr dθ.
¡
¡
a) sphere: ρ = 2a cos φ. b) plane: ρ = a sec φ.
c)
2 π
0
π/ 4
0
2 a cos φ
a sec φ
ρ
2
sin φ dρ dφ dθ.
∂
∂y
(2xy + z
3 ) = 2x =
∂
∂x
(x
2
∂
∂z
(2xy + z
3 ) = 3z
∂
∂x
(y
2
2 − 1);
∂
∂z
(x
2
∂
∂y
(y
2
2 − 1); so
F is conservative.
b)
∂f
∂x
= 2xy + z
3 , so f (x, y, z) = x
2 y + xz
3
∂f
∂y
= x
2
∂g
∂y
= x
2
∂g
∂y
= 2yz.
Therefore g(y, z) = y
2 z + h(z), and f (x, y, z) = x
2 y + xz
3
2 z + h(z).
∂f
∂z
= 3xz
2
2
′ (z) = y
2
2 − 1, so h
′ (z) = −1.
Therefore h(z) = −z + c, and f (x, y, z) = x
2 y + xz
3
2 z − z + c.
2 − y
2 , so ˆn dS = 〈−f x
, −f y
, 1 〉 dx dy = 〈 2 x, 2 y, 1 〉 dx dy.
Therefore
S
F · nˆ dS =
S
〈x, y, 2(1 − z)〉 · 〈 2 x, 2 y, 1 〉 dx dy =
S
2 x
2
2
S
4 x
2
2 dx dy (since z = 1 − x
2 − y
2 ).
Shadow = unit disc x
2
2 ≤ 1; switching to polar coordinates, we have
S
F · nˆ dS =
2 π
0
1
0
4 r
2 r dr dθ =
2 π
0
r
4
1
0
dθ = 2π.