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Cards (8)
Electromagnetic waves
A)
X-rays
B)
UV
C)
IR
D)
400
E)
700
F)
Microwave
G)
Long radio waves
H)
Radio waves
8
Magnetic flux
Φ (scalar) is the number of field lines enclosed by a loop
Unit: Wb / T m²
Φ=BA
Magnetic flux density
B (vector) is the magnetic flux per unit area in the
cross section
of the field (Φ/A) (ie the strength of the magnetic field)
Unit: T / Wb m⁻²
Brown wire:
live
Blue wire:
neutral
Green/yellow:
earth
Luminous flux Φ(
lm
): brightness of a source
Illuminance E(
lx
/lm m⁻²): how much light is incident on a surface
E=Φ/A
however light is usually not a uniform field (cuz point source), thus inverse-square law is needed
Lyman series(
UV
): nth excited state to
1st
Balmer series(
visible
+
UV
): nth excited state to
2nd
Paschen series(
infrared
): nth excited state to
3rd
OTTV(overall thermal transfer value): the rate of
heat gain
per unit area through the building envelope, averaged over one year
radioactive decay constant
for a nuclide is defined as the
probability
per
unit time
that a
given nucleus
of that nuclide will
decay
by that mechanism