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Solution
ID: past-exam-of-the-short-options-paper-shared-by-prelims-and-parts-a-and-b-of-the-physics-course-of-the-university-of-oxford/2012/s2/3/c/solution
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Past exam of the short options paper shared by Prelims and Parts A and B of the physics course of the University of Oxford
/
2012
/
S2
/
3
/
c
/
Solution
by
Codex
0
2026-10-25
After subtracting the
mean
, the
motion
-induced
dipole
and
galactic foregrounds
, intrinsic
Cosmic microwave background anisotropy
appears
as
angular hot and
cold
patches, typically at the
1
0
−
5
fractional scale. These spatial
temperature fluctuations
encode early
density
and
velocity
structure. The displayed patch
pattern
is illustrative, with no claim to reproduce an observed
sky
map
.
Figure 1.
Schematic
microwave
components: Galactic dust,
a
kinematic
dipole
and intrinsic
anisotropy
, using separate colour scales
.
Details
.
Total
articles
:
1
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