Coronagraph Created 2026-10-06 Updated 2026-10-13
A coronagraph is an optical instrument that suppresses a bright source's light before detection while transmitting some light from nearby directions. Its purpose is to reveal faint structure buried in the bright source's point spread function, as in exoplanet direct imaging. A Lyot coronagraph combines a coronagraphic focal plane mask with a Lyot stop in a reimaged optical pupil; blocking the central image alone does not remove its diffraction rings. [ref].
Figure 1.
The four principal planes of a Lyot coronagraph: a focal plane mask and a reimaged optical pupil stop select different parts of the wave amplitude distribution. Qualitative schematic, with illustrative sizes and brightness.
Details.
The original motivation was the solar corona: hiding the bright photosphere would allow longer, repeated observations of faint surrounding light. In his 1930 paper, Lyot explained that short total eclipses restricted observing time and prevented some long exposures for spectral lines. The attraction is an instrument that makes the faint neighborhood accessible on demand. [ref]. The Sun is an extended source; the point-source calculation below illustrates imaging of an unresolved star and is not a quantitative model of the solar corona.
Lyot coronagraph 2026-10-14
A classical Lyot coronagraph first forms an image of a bright source on the optical axis. A coronagraphic focal plane mask hides its core. Relay optics then form an image of the entrance pupil, where a Lyot stop blocks the outer rim and, when needed, borders around internal obstructions. Finally an optical camera forms the science image. The focal plane sorts incoming directions into image positions; the optical pupil sorts contributions across the aperture. This change of plane makes it possible to reject additional stellar light that survives the first mask. [ref].
Lyot stop 2026-10-14
A Lyot stop is a mask in the reimaged optical pupil after a coronagraphic focal plane mask. For an unobstructed circular entrance pupil, it usually transmits a smaller concentric disk. In a classical Lyot coronagraph, much of the residual stellar field lies near the optical pupil boundary; the Lyot stop rejects that field before the final image is formed. It also rejects useful off-axis light, so choosing its opening involves a coronagraph throughput tradeoff. [ref].