upgrade
upgrade

☁️Atmospheric Physics

Key Atmospheric Optical Phenomena

Study smarter with Fiveable

Get study guides, practice questions, and cheatsheets for all your subjects. Join 500,000+ students with a 96% pass rate.

Get Started

Why This Matters

Atmospheric optical phenomena aren't just beautiful—they're your window into understanding how light behaves when it encounters different media. Every rainbow, halo, and mirage demonstrates core physics principles you'll be tested on: refraction, reflection, diffraction, scattering, and dispersion. These phenomena connect directly to concepts like Snell's law, the wavelength dependence of refractive index, and particle-light interactions that appear throughout atmospheric physics.

When you see these phenomena on an exam, you're being tested on your ability to identify the underlying mechanism. Can you distinguish between refraction through ice crystals versus water droplets? Do you know why some effects require the sun at specific angles? Don't just memorize which phenomenon looks like what—know why each one forms and what physical principle it demonstrates. That's what separates a 5 from a 3.


Refraction Through Ice Crystals

When light passes through hexagonal ice crystals suspended in cirrus clouds or cold air, it bends at specific angles determined by the crystal geometry and the refractive index of ice (approximately 1.31). The 22° and 46° deviation angles produce the most common ice crystal phenomena.

Halos

  • 22° halos form when light refracts through randomly oriented hexagonal ice crystals—the minimum deviation angle creates the characteristic bright ring
  • Cirrus clouds at high altitudes (above 6 km) provide the ice crystals, making halos useful weather indicators for approaching fronts
  • Both sun and moon can produce halos, though lunar halos appear less colorful due to lower light intensity affecting color perception

Sun Dogs (Parhelia)

  • Horizontal crystal orientation is key—plate-shaped ice crystals floating flat produce bright spots at exactly 22° on either side of the sun
  • Low sun angles (below 45°) are required because horizontally oriented crystals only intercept light effectively when the sun is near the horizon
  • Color separation occurs with red closest to the sun and blue farther out, demonstrating dispersion through the ice prism

Circumhorizontal Arcs

  • High sun angle required (above 58°)—light enters through the vertical side faces of horizontally oriented ice crystals and exits through the bottom
  • Plate crystals must be large and well-aligned, which is why these "fire rainbows" are relatively rare
  • Parallel to horizon appearance distinguishes them from rainbows, which are always centered on the antisolar point

Light Pillars

  • Reflection, not refraction—flat ice crystals act as tiny mirrors, reflecting light sources vertically
  • Column-shaped crystals falling with their long axes horizontal create pillars extending above and below the light source
  • Artificial lights often produce more dramatic pillars than the sun because multiple point sources create overlapping columns

Compare: Sun dogs vs. 22° halos—both involve 22° refraction through ice, but sun dogs require horizontally oriented plate crystals while halos form from randomly oriented crystals. If an FRQ asks about crystal orientation effects, this is your go-to contrast.


Refraction Through Water Droplets

Liquid water droplets act as tiny spherical lenses with a refractive index of about 1.33. Light entering a droplet undergoes refraction at entry, internal reflection off the back surface, and refraction again at exit—with each color bending at slightly different angles due to dispersion.

Rainbows

  • Primary rainbow forms at 42° from the antisolar point via one internal reflection—red on the outside (42°42°) and violet inside (40°40°) due to wavelength-dependent refraction
  • Secondary rainbow appears at 51° with reversed colors from two internal reflections, always fainter due to additional light loss
  • Alexander's dark band between primary and secondary rainbows is darker because no light rays emerge at those angles—a key exam detail

Green Flash

  • Atmospheric refraction bends sunlight like a weak prism, with blue/green light refracted more than red
  • Differential extinction removes blue light through Rayleigh scattering, leaving green as the last visible color at sunset
  • Clear horizon and stable atmospheric layers are essential—any turbulence or haze destroys the effect

Compare: Rainbows vs. green flash—both involve refraction separating colors, but rainbows use discrete water droplets as prisms while the green flash uses the entire atmosphere as a gradient-index lens. This illustrates how the same principle operates at vastly different scales.


Diffraction Effects

When light waves encounter obstacles or apertures comparable to their wavelength, they bend around edges and interfere with each other. Water droplets in the 10-50 μm range produce the most vivid diffraction phenomena, with angular size inversely proportional to droplet size.

Coronas

  • Small, uniform droplets are essential—the colored rings form from interference of light diffracted around droplet edges
  • Angular radius inversely proportional to droplet size: θλ/d\theta \propto \lambda/d, so smaller droplets produce larger coronas
  • Thin clouds work best; thick clouds produce overlapping patterns that wash out the colors

Glories

  • Backscattering mechanism involves light entering droplets, reflecting internally, and diffracting as it exits back toward the light source
  • Observer's shadow marks the center (antisolar point), with concentric colored rings surrounding it
  • Aircraft observations are ideal because you need uniform cloud droplets below you and sun behind you

Brocken Spectre

  • Shadow projection onto fog or cloud creates the dark silhouette; the glory around it is the optical phenomenon
  • Magnification illusion occurs because the shadow falls on droplets at varying distances, making it appear enormous
  • Antisolar point geometry means the observer must have sun directly behind them and mist/cloud in front

Compare: Coronas vs. glories—both are diffraction phenomena involving similar-sized water droplets, but coronas appear around the light source (forward scattering) while glories appear around your shadow (backscattering). The geometry is exactly opposite.


Temperature-Gradient Refraction

When air layers have different temperatures, they have different densities and therefore different refractive indices. Light rays curve toward denser (cooler) air, bending continuously rather than at discrete interfaces. This produces mirages and other distortion effects.

Mirages (Inferior)

  • Hot surface creates low-density air below cooler air—light curves upward, making the sky appear reflected on the ground
  • Total internal reflection isn't actually occurring; it's continuous refraction through the gradient that bends rays back up
  • "Water on road" effect is sky light reaching your eyes from below, interpreted by your brain as a reflective surface

Fata Morgana

  • Temperature inversion (warm air over cold) creates a superior mirage where objects appear elevated and distorted
  • Multiple alternating layers produce the complex stacking and stretching effects—objects can appear as towers, cliffs, or floating islands
  • Polar and coastal regions are prime locations due to cold water/ice creating strong inversions

Compare: Inferior mirage vs. Fata Morgana—both result from refractive index gradients, but inferior mirages need hot surfaces (light curves up) while Fata Morgana needs temperature inversions (light curves down). The thermal structure determines whether images appear below or above the actual object.


Scattering Phenomena

Particles in the atmosphere scatter light differently depending on their size relative to the wavelength. Rayleigh scattering (particles << wavelength) affects short wavelengths most, while Mie scattering (particles ~ wavelength) is less wavelength-dependent.

Crepuscular Rays

  • Shadow casting by clouds creates alternating bright and dark bands—the rays are actually parallel but appear to converge due to perspective
  • Aerosols and dust make the rays visible by scattering sunlight into your eyes; clean air produces no visible beams
  • Anticrepuscular rays converge at the antisolar point opposite the sun, proving the rays are geometrically parallel

Heiligenschein

  • Retroreflection from dew droplets—each spherical drop focuses light onto the leaf surface behind it, which reflects back through the drop
  • Opposition effect means the bright halo appears around your own shadow because you're looking directly back along the incident light path
  • Cat's eye retroreflectors on roads use the same principle artificially—this is the natural version

Compare: Crepuscular rays vs. Heiligenschein—both involve scattering/reflection making light visible, but crepuscular rays show light's path through the atmosphere while Heiligenschein shows retroreflection back toward the source. One reveals the medium; the other reveals the geometry.


Non-Optical Atmospheric Phenomena

Some spectacular atmospheric light displays don't involve the optical properties of air, water, or ice at all—they result from entirely different physical mechanisms operating in the upper atmosphere.

Auroras

  • Solar wind particles (electrons and protons) are channeled by Earth's magnetic field toward the poles, where they collide with atmospheric gases
  • Emission spectra determine colors: oxygen produces green (558 nm) and red (630 nm), nitrogen produces blue and purple
  • Altitude affects color—green dominates at 100-300 km, red appears above 300 km where oxygen atoms are less frequently de-excited by collisions

Noctilucent Clouds

  • Mesospheric ice crystals form at ~80 km altitude—the highest clouds in Earth's atmosphere
  • Twilight illumination makes them visible when the lower atmosphere is in shadow but sunlight still reaches the mesosphere
  • Climate change indicator—increasing methane oxidizes to water vapor in the upper atmosphere, potentially making these clouds more frequent

Compare: Auroras vs. noctilucent clouds—both are upper-atmosphere phenomena visible at night, but auroras involve particle excitation and emission while noctilucent clouds involve scattering from ice crystals. One is plasma physics; the other is classical optics at extreme altitude.


Quick Reference Table

ConceptBest Examples
Refraction through ice crystalsHalos, sun dogs, circumhorizontal arcs, light pillars
Refraction through water dropletsRainbows, green flash
Diffraction around small dropletsCoronas, glories, Brocken spectre
Temperature gradient refractionInferior mirages, Fata Morgana
Atmospheric scatteringCrepuscular rays, Heiligenschein
Crystal orientation dependenceSun dogs (horizontal), halos (random), light pillars (reflection)
Antisolar point phenomenaRainbows, glories, Brocken spectre, anticrepuscular rays
Upper atmosphere effectsAuroras (emission), noctilucent clouds (scattering)

Self-Check Questions

  1. Both sun dogs and 22° halos involve light passing through ice crystals at the same angle. What physical difference in crystal orientation explains why sun dogs appear as discrete spots while halos form complete rings?

  2. You observe a corona around the moon that appears unusually large. Based on the relationship θλ/d\theta \propto \lambda/d, what can you infer about the water droplets producing it compared to a typical corona?

  3. Compare and contrast the formation mechanisms of rainbows and circumhorizontal arcs. Both display spectral colors, but why does one appear as an arc centered on the antisolar point while the other appears parallel to the horizon?

  4. An FRQ describes a desert scene where distant mountains appear to float above the horizon. Identify the phenomenon, explain the temperature structure required, and contrast it with the "water on the road" effect seen on hot pavement.

  5. Which two phenomena from this guide require you to be positioned at the antisolar point (sun directly behind you) to observe them? What role does this geometry play in their formation?