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A lab report detailing the concept of polarized light, its components, and various types such as plane, elliptical, and circular polarization. It includes the definition of the cross product, the relationship between electric and magnetic fields, and the difference between polarization and polarizability. The document also discusses the use of polarizers, a radiometer, and other equipment for investigating polarized light.
Typology: Lab Reports
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1051-455-20073, Physical Optics
This lab introduces the concept of polarization of light. As we have said in class (and as is obvious from the name), electromagnetic radiation requires two traveling-wave vector components to prop- agate: the electric field, often specified by E, and the magnetic field B. The two components are orthogonal (perpendicular) to each other, and mutually orthogonal to the direction of travel, which is often specifed by the vector quantity s (the Poynting vector):
s ≡ E × B
where “×” specifies the mathematical “cross product”.
1.1.1 Cross Product
Just to review, the cross product of two arbitrary three-dimensional vectors a = [ax, ay, az ] and b = [bx, by, bz ] is defined:
a×b ≡ det
ˆx yˆ ˆz ax ay az bx by bz
≡ ˆx (ay bz − by az ) + ˆy (az bx − bz ax) + ˆz (axby − ay bx)
where ˆx, ˆy, and ˆz are the unit vectors directed along the respective Cartesian axes and det [ ] represents the evaluation of the determinant of the 3 × 3 matrix. You may recall that the “cross product” is defined ONLY for 3-D spatial vectors. For example, if the electric field E is oriented along in the x -direction with amplitude Ex (so that E||xˆ, where || indicates “is parallel to”). The electric field is E = ˆx · Ex + ˆy · 0 + ˆz · 0. Consider also that the magnetic field B ⊥ E is oriented along the y-direction (B||ˆy, B = ˆx · 0 + ˆy · By + ˆz · 0 ), then the electromagnetic field travels in the direction specified by:
E^ ˆ × Bˆ ≡ det
ˆx ˆy ˆz Ex 0 0 0 By 0
= ˆx (0 · 0 − By · 0) + ˆy (Ex · 0 − 0 · 0) + ˆz (Ex · By − 0 · 0) = ˆz (Ex · By)
Thus the electromagnetic wave propagates in the direction of the positive z axis.
1.1.2 Polarization
In vacuum (sometimes called free space), the electric and magnetic fields propagate in phase, which means that both have extrema or nulls at the same locations in space-time. For example, if the electric field is a traveling wave with phase k 0 z − ω 0 t + φ 0 , then the two component fields are:
E [z, t] = ˆxE 0 cos [k 0 z − ω 0 t + φ 0 ]
B [z, t] = ˆyB 0 cos [k 0 z − ω 0 t + φ 0 ] = yˆ
μ E 0 c
cos [k 0 z − ω 0 t + φ 0 ]
where c is the velocity of light in vacuum. Of course, we know the relationships of the wavenumber k 0 = 2π/λ 0 , the temporal angular frequency ω 0 = 2πν 0 = 2πc/λ 0 , and the veloctiy c = λ 0 ν 0. Because the amplitude of the electric field is larger by a factor of c, the phenomena associated with
the electric field are easier to measure. Most of the force exerted by the electromagnetic field on a charge comes form the electric field E (which may vary with time/position), so it is the direction of E that is called the polarization.
For waves in vacuum, the electric and magnetic fields are “in phase” and the wave travels in the direction specified by ˆs = Eˆ × Bˆ.
As a side comment, note the difference between the polarization of the E-M wave and the polar- izability of a material, which is a measure of the effect of the electric field on the bound charges in the material. Polarized light comes in different flavors: plane (or linear), elliptical, and circular. In the first lab on oscillations, we introduced some of the types of polarized light when we added oscillations in the x- and y-directions (then called the real and imaginary parts) with different amplitudes and initial phases. The most commonly referenced type of light is plane polarized, where the the electric field vector E points in the same direction for different points in the wave. Plane-polarized waves with E oriented along the x- or y-axis are easy to visualize; just construct a traveling wave oriented along that direction. Plane-polarized waves at an arbitrary angle θ may be constructed by adding x- and y-components with the same frequency and phase and different amplitudes, e.g.,
E [z, t] = ˆxEx cos [k 0 z − ω 0 t + φ 0 ] + ˆyEy cos [k 0 z − ω 0 t + φ 0 ] When the two component electric fields are “in phase” (so that the arguments of the two cosines are equal for all [z, t]), then the angle of polarization, specified by θ, is obtained by a formula analogous to that for the phase of a complex number:
θ = tan−^1
Ey cos [k 0 z − ω 0 t + φ 0 ] Ex cos [k 0 z − ω 0 t + φ 0 ]
= tan−^1
Ey Ex
Angle of linear polarization for (Ex)max = 1 and (Ey)max = 0. 5 is tan=
h Ey Ex
i ' 0. 463 radians ' 26. 6 ◦.
Like linearly polarized light, circularly polarized light has two orthogonal states, i.e., clockwise and counterclockwise rotation of the E-vector. These are termed right-handed (RHCP) and left-handed (LHCP). There are two conventions for the nomenclature:
right left
hand in the direction of propagation. If the fingers point in the direction of rotation of the E-vector, then the light is
The conservation of angular momentup ensures that the “handedness” of circularly or elliptically polarized light changes upon reflection, i.e., if the incident wave is RHCP, then the reflected wave is LHCP.
The “handedness” of circularly or elliptically polarized light changes upon reflection due to conservation of angular momentum.
This lab consists of several sections:
Your lab kit includes linear and circular polarizers, and quarter-wave and half-wave plates.
(a) Orient two polarizers in orthogonal directions and look at the transmitted light. (b) Add a third polarizer AFTER the first two so that it is oriented at an angle of approxi- mately π/ 4 radians (45◦) and note the result. (c) Add a third polarizer BETWEEN the first two so that it is oriented at an angle of approximately π/ 4 radians and note the result.
(a) Mount a screen behind polarizer P 1 and test the radiation from the laser to see if it is plane polarized and, if so, at what angle. (b) Measure the “baseline” intensity of the source using the CCD camera (with lens). You may have to attenuate the light source with a piece of paper and/or stop down the aperture of the lens. (c) Insert one polarizer in front of the detector and measure the intensity relative to the original unfiltered light. How much light does one polarizer let through? Next, increase the intensity of the light until you nearly get a saturated image on the CCD. (d) Add a second polarizer to the path and orient it first to maximize and then to minimize the intensity of the transmitted light. Measure both intensities.
(a) Examine scattered light from the blue sky for linear polarization. Look at several angles measured relative to the sun. (b) Determine the direction where the light is most completely polarized. This knowledge is useful to determine the direction of polarization of any linear polarizer. (c) Test skylight for circular polarization.
Polarization of sunlight due to scattering by molecules in the atmosphere.
In your writeups, be sure to include the following items.
√ N σ uncertainty.