Before calculating
Polarization describes the direction and time evolution of the electric field transverse to light propagation. A linearly polarized field oscillates along a fixed axis. A ray sketch alone does not show that axis. A polarizer selects one field component; using it to investigate an existing polarization makes it an analyzer.[1][2]
For the ideal basic calculation the analyzer’s input is already linearly polarized, and I0 refers to that particular stage. Unpolarized light before the first ideal filter is first halved on average. You need cosine and the distinction between field amplitude and its square. Assume unchanged beam collection and no additional losses.[1]
I0 belongs to the analyzer’s input stage
θ is the angle between the existing linear polarization direction and the analyzer transmission axis.[1]
I0 is intensity immediately before the chosen analyzer, not automatically before the entire filter chain. Ideal parallel axes transmit I0, crossed axes transmit zero. Axis orientation is defined modulo 180°:0° and 180° describe the same transmission direction. The intensity curve therefore repeats every 180°.[1]
Intensity is power per cross-sectional area in W/m2. The same relation holds for total power if the unchanged beam cross-section is fully captured. If aperture or beam shape changes between stages, detector power ratios cannot be interpreted as without checking geometry.[1]
Intensity repeats every 180°
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From field projection to intensity
Let the analyzer axis be unit vector a. For a linearly polarized field with fixed direction, projection gives transmitted amplitude . The ideal analyzer removes the perpendicular component. The outgoing field is linear along a, so a subsequent filter must compare its axis with a, not with the original direction before the chain.[2]
C is the same intensity factor before and after the ideal filter in the same medium. Squaring distinguishes intensity from amplitude.[2]
A negative projection represents field sign or phase, not negative intensity. Squaring makes intensity nonnegative. At 90° the projection vanishes, so a later ideal filter cannot restore energy already removed. An absorptive polarizer transfers rejected energy to its surroundings; other designs send it into a different output channel.[1]
The Brewster angle for polarization describes the incidence angle at which light reflected from a suitable interface is completely linearly polarized. Apply the analyzer intensity projection only once the linear input has been properly specified.[1]
Analyze a linearly polarized input
Analyzer at 37°
- Given
- I0=72.0 W/m2; linear input; axis difference 37.0°.
- Find
- Find output intensity and rejected fraction.
Approach: An ideal analyser projects the electric-field amplitude onto its axis; intensity follows the square of that projection.
Calculate and square the amplitude projection.
Apply the intensity factor.
Result: I≈45.92 W/m2; 36.22% is removed from the transmitted channel.
Check: I lies between 0 and 72 W/m2. Using cos 37° instead of its square would give 57.50 W/m2, confusing amplitude and intensity.
A first ideal filter halves unpolarized light
Statistically unpolarized light has no preferred transverse field direction. An ideal linear filter transmits half of mean intensity. This is an average over polarization directions, not Malus with one fixed angle describing the complete input. The output then has the filter’s linear direction and subsequent stages follow Malus.[1]
Averaging gives the ideal half transmission. Partially polarized or elliptical input needs additional information.[1]
Circularly polarized light also gives half intensity through an ideal linear analyzer, but is not unpolarized: its components have a definite phase relation. One intensity value after a linear filter cannot distinguish these states. Complete polarization analysis needs additional optical settings, such as a retardation plate.[2]
Insert a third filter between crossed axes
Three ideal filters at 0°,30° and 90°
- Given
- Unpolarized Iin=120 W/m2; order 0°→30°→90°; no additional losses.
- Find
- Find intensity after each stage.
Approach: The first ideal filter halves unpolarized input intensity. Subsequent stages use Malus with each adjacent axis difference.
The first stage halves intensity and gives 0° linear polarization.
Between 0° and 30°, the axis difference is 30°.
The third stage receives 30° polarization; its relative angle is 60°.
Result: After the stages: 60, 45 and 11.25 W/m2. Without the middle filter, the outer ideal filters are crossed and output is zero.
Check: Output energy is below every preceding stage. The added filter creates no energy; it changes the surviving field’s direction before the final projection. Applying 120 cos290° directly would misdescribe this chain.
Infer angles and uncertainty from intensity ratios
Angle inference requires a chosen interval; other equivalent or mirrored axis orientations produce the same intensity. Differentiate with θ in radians.[1]
For , choosing 0° to 90° gives 53.1301°. Intensity alone does not identify clockwise versus counterclockwise rotation. With I0=60 W/m2 and 45°, I=30 W/m2. A±1° angle shift gives 31.047 or 28.953 W/m2, approximately±3.49% around this operating point.[1]
Near crossed axes, ideal absolute output is small but relative error becomes sensitive. Scattering or finite extinction can dominate the dark signal. Measure background and normalize against parallel transmission before inferring a precise angle from a near-zero detector reading.[1]
With , the ideal model also gives ; no angle can be inferred. Likewise, a measurement at exactly crossed axes does not determine input intensity: every nonnegative input is fully blocked.[1]
Explore further: real polarizers
A simple real model for linear input; principal-axis transmissions refer to the specified spectrum and geometry.[1]
For Tparallel=0.90 and , crossed output is 0.002 I0 rather than zero and parallel output 0.90 I0 rather than I0. Their ratio 450 is the extinction ratio as defined here. Product specifications may use reciprocal conventions or different measurement conditions, so read the numerical definition explicitly.[1]
The ideal relation assumes fixed linear input polarization, stable intensity, an appropriate linear analyzer and unchanged collection. Depolarization, elliptical states, angle-sensitive coatings or a saturated detector require more than a cosine-squared factor. Malus describes directional analysis, not every loss in a complete optical system.[2]
Leakage through a nonideal filter
- Given
- Linear input I0=80.0 W/m2; ; ; unchanged collection.
- Find
- Find intensity at 0°, 45° and 90° and the extinction ratio defined here.
Approach: weight both orthogonal input components by their own power transmissions.
Substitute the three angles separately. At 45° both squared projections are equal.
Result: Crossed orientation transmits 0.160 W/m2 here. Parallel-to-crossed transmission ratio is 450; the filter is not a perfectly blocking polarizer.
Check: All outputs are below 80 W/m2; the 45° value is exactly halfway between parallel and crossed output. Setting and recovers Malus’s law.
The wave relation for propagation speed, wavelength and frequency connects . That relation alone does not determine filter transmission: the polarization state and field-amplitude projection are still needed.[3][1]
Five calculations keeping filter stages distinct
Calculate · Foundation
Linear I0=90 W/m2; analyzer 32°. Calculate I.
Show hint
Intensity contains the squared field factor.
Learning goal: Calculate transmitted intensity for specified linear polarization.
Show solution and calculation
Approach: the input is already linearly polarized.
Apply Malus directly and square the field projection factor.
This gives I≈64.7267 W/m2.
Check: intensity ratio is about 0.719186, between zero and one. A passive ideal filter yields neither negative intensity nor more than 90 W/m2.
Transfer · Application
Unpolarized 80 W/m2 reaches two ideal filters 60° apart. Find output.
Show hint
The first stage halves; the second uses Malus.
Learning goal: Halve unpolarized input first, then use relative axis orientation.
Show solution and calculation
Approach: the first stage halves unpolarized intensity on average.
The second then receives the linear polarization selected by the first.
Intensities are 40 W/m2 and then 10 W/m2.
Check: directly using would omit the first halving. Each correctly treated stage reduces transmitted intensity here.
Calculate · Application
Reduce linear input to 36%. Which ideal analyzer angle between 0° and 90° is required?
Show hint
Take the square root of the intensity ratio first.
Learning goal: Find an analyser angle from a target intensity fraction.
Show solution and calculation
Approach: the chosen interval 0° to 90° fixes the nonnegative cosine branch.
Take the square root of the intensity ratio before inverse cosine.
This gives θ≈53.1301°.
Check: . The negative angle would give the same intensity but is outside the chosen interval.
Interpret · Application
Light is already linearly polarized at 0° with intensity 64 W/m2. An ideal analyser at 90° transmits nothing. An ideal polarizer at 45° is now inserted before it. Calculate intensity after both elements and explain why an extra element permits more output light here. Absorption beyond ideal polarization selection is excluded.
Show hint
Apply Malus’s law sequentially. After the first element polarization is at 45°, so the second relative angle is also 45°.
Learning goal: Explain the effect of inserting another polarizer between crossed axes.
Show solution and calculation
Approach: treat each polarizer relative to the polarization of its own input.
After 45°, intensity is 32 W/m2; after the 90° analyser it is 16 W/m2.
The intermediate polarizer changes the transmitted light’s polarization, so the analyser no longer receives a perpendicular input.
Check: output remains below input intensity. Increased transmission does not create energy.
Error analysis · Foundation
Unpolarized light of intensity 50 W/m2 reaches a single ideal linear polarizer. Someone chooses a laboratory axis and uses Malus’s law to predict zero transmission at rotation angle 90°. Find actual average output intensity and explain which premise of that single-angle calculation is missing.
Show hint
Unpolarized light has no fixed input polarization axis. Averaging cos2 over uniformly distributed directions gives one half.
Learning goal: Avoid assigning unpolarized light an arbitrary direction when applying Malus’s law.
Show solution and calculation
Approach: average the unpolarized input over polarization directions.
A single ideal polarizer transmits 25 W/m2, independently of absolute laboratory orientation.
An angle to a laboratory axis is not an angle to an existing input polarization axis.
Check: only a second polarizer could use its angle relative to the first to modify the now linearly polarized output through Malus’s law.
What to take away
Before calculating, identify the intensity immediately before this filter and its polarization. Linear input uses the squared field projection. An ideal first filter halves unpolarized intensity on average; later stages use adjacent axis differences. An extra filter can change direction but cannot create energy. Real residual light needs a leakage or background model.[1][2]
Sources for this explanation
Quanta · Updated October 2, 2026
- OpenStax University Physics3 §1.7: Malus law and unpolarized input
- MIT6.007 Lecture24: polarized light, linear and circular states, analyzers
- OpenStax University Physics Volume1 §16.1 Traveling Waves
Editorial responsibility: Quanta Study editorial team
Review scope
This explanation, 3 worked examples and 5 exercises are available in German and English. Structure, source references and mathematical notation undergo automated checks. Calculations, model assumptions and both language versions receive a separate AI review.
An internal human subject review is documented for an earlier release of this page. That confirmation does not apply automatically to the revised explanation and new exercises.
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Editorial responsibility, sources and methodsChange history
- Linked polarization and wave context, added inverse zero cases and placed one decimal value wholly inside its math delimiters; preserved examples and intensity curve.
- Explained input stage and field projection; added a periodicity plot and real-transmission example; clarified filter chains and exercise checks.
- Added prerequisites and model assumptions; clarified derivation steps and arithmetic checks; included an additional original example, diagram and summary.
Cite this reference page
Quanta. Malus’s law. Updated October 2, 2026. https://quanta-study.de/en/formula-sheet/malus-gesetz-polarisation
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