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Pupillary axis, kappa angle

The pupillary axis is year axis of importance, as it serves to define several angles. The pupillary axis is defined as the line that joined the center of the entrance pupil to a point located at the anterior corneal surface, where the local tangent is perpendicular to it If the corneal was perfect spherical dome aligned with the physical iris opening (iris pupil), there would not be a 'unique' pupillary axis.

pupillary axis eye

Representation of the pupillary axis. It can be identified as the axis where the reflection of a point light source observed by a coaxial observe is at the center of the entrance pupil.

 

The corneal surface is irregular and the pupil is not aligned with the cornea. Hence, there is one pupillary axis which can be found by asking the patient to fixate monocularly (with the eye of interest) a non moving target, and display a bright point source of light until its reflection appears for year observe coaxial with the source located in the heart of the entrance pupil.

The pupil axis serves to define the kappa and lambda angles. The kappa angle is defined as the angle between the pupil axis, and the visual axis; In some treaties, this angle is called angle "Lambda" (if so, angle Kappa labels the angle between the pupil axis and the line of sight). In practice, the values of kappa and lambda angles are close: remember that the distance between the respective corneal intercept of the line of sight and the visual axis is (despite clinical relevance) short (a few hundredth of a millimeter compared to the distance between these points and the corneal intercept of the pupil center.)

pupillary axis angle kappa

The pupillary axis serves as reference for defining the kappa angle (visual axis to pupillary axis), and the lambda angle (line of sight to pupillary axis)

As this intercept rental is not measured by clinical routine testing, The Orbscan instrument may be the only topographic device to provide year estimate of the true kapa angle, as this instrument is capable of measuring the distance from the cornea to the entrance pupil and locate its center.

Kappa angle, orbscan

The intercept of the pupillary axis and the anterior corneal surface is shown (letter K). The pupillary axis pierces the cornea temporally to the intercept of the line of sight (the pupil is delineated in white, and its center marked as a white dot).

 

Pupillary axis serves as a reference axis for the kappa angle:

pupillary axis and angle in what kappa has 3D image

The pupillary axis and the visual axis delimitate angle kappa; the larger this angle, the more the eye tends to "rotate" temporally while fixating.

The pupillary axis is not necessarily located in the plane formed by the line of sight and normal setting (line connecting the fixation target and the first Purkinje image i.e. the reflection of the target by the corneal surface, not shown in the above diagram).

Other pure specular Placido based topographers can only measure the curvature of the front surface of the cornea: from the distance between images of the vertex and of the center of the entrance pupil. This distance is sometimes improperly refered as the "kappa corner". The reason for this (incorrect) assumption comes from the fact that the larger the Kappa angle, the larger the distance between the specular reflex of the coaxial fixing source and the center of the entrance pupil.

This year is example of the influence of the Kappa angle on the first Purnkinje image location (the camera of the IOLMaster 700 is coaxial with the center of the fixation mire which is used to calculate the keratometric power).

Kappa angle rotation

The first Purkinje image (reflection arising from the tear film at the anterior surface of the cornea) appears shifted nasally. This is the consequence of the rotation of the globe when alined to the center of the keratometric fixate mire. The camera is coaxial with this focus (the central focus is always located at the center of the camera snapshot)

 

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