Spherical aberration in high NA objectives

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SUMMARY

Spherical aberration (SA) is a significant residual aberration in high numerical aperture (NA) microscope objectives, particularly immersion lenses. These lenses are designed to work with a specific coverslip thickness and refractive index, typically 0.17mm and n=1.518, to minimize aberrations. If the coverslip deviates from these specifications, SA can increase dramatically. The phase factor acquired by light as it passes through the coverslip is influenced by its thickness and refractive index, and this relationship can be described using Zernike polynomials.

PREREQUISITES
  • Understanding of spherical aberration in optics
  • Familiarity with numerical aperture (NA) concepts
  • Knowledge of refractive index and its impact on light propagation
  • Basic principles of Zernike polynomials in wavefront analysis
NEXT STEPS
  • Research the design principles of high NA immersion microscope objectives
  • Learn about the effects of coverslip thickness on optical performance
  • Study the application of Zernike polynomials in optical aberration correction
  • Explore the use of different refractive index immersion oils for phase correction
USEFUL FOR

Optical engineers, microscopy specialists, and researchers involved in high-resolution imaging and optical design will benefit from this discussion.

omg!
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hi everybody,

i would appreciate it if someone could clarify the concept of spherical aberrations in the context of high NA objectives in which use lenses are used that are not exclusively of the spherical type.
a common thing that you hear is that some objective is corrected for 0.17mm coverglass of n=1.518, or something like that. i have always interpreted it as in this example:

as the wave front that emerges from a point light source traverses the cover glass and immersion oil towards the objective, the phase relation is changed depending on angle so that the wave front gets deformed. what a "corrected" objective then does is to compensate for this deformed wave front.

is this correct?
thank you very much for your help!
 
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omg! said:
hi everybody,

i would appreciate it if someone could clarify the concept of spherical aberrations in the context of high NA objectives in which use lenses are used that are not exclusively of the spherical type.
a common thing that you hear is that some objective is corrected for 0.17mm coverglass of n=1.518, or something like that. i have always interpreted it as in this example:

as the wave front that emerges from a point light source traverses the cover glass and immersion oil towards the objective, the phase relation is changed depending on angle so that the wave front gets deformed. what a "corrected" objective then does is to compensate for this deformed wave front.

is this correct?
thank you very much for your help!

Spherical aberration (SA) is (usually) the largest residual aberration in a well-corrected lens- *any* well corrected lens. Because SA scales as (IIRC) the square of the numerical aperture, well-corrected high-NA (typically immersion) microscope objectives can easily suffer from the presence of SA.

In a well-corrected immersion lens, the coverslip is actually part of the total optical design- the lens has been carefully designed to work with a very precise thickness of coverslip (some specialized lenses are designed to be adjusted for use with a range of coverslip thickness), and if the coverslip is the incorrect thickness, lens aberrations can get really large really fast- and especially SA. I know one (rather extreme) person who goes so far as to measure each coverslip with a micrometer before use, and discards ones that are outside his specification.

The reason the particular index of refraction is specified is also to minimize aberrations- the immersion oil should have the same refractive index as the coverslip, which is also the same refractive index as the mounting medium and glass slide (so-called 'homogeneous conditions').

http://www.microscopyu.com/articles/formulas/formulascoverslipcorrection.html

To be sure, there are lenses designed to be used with no coverslip- generally, reflected light objectives and dipping objectives.

Careful tweaking of the optics can fractionally improve performance: for example, because my laser tweezers use 1064nm light, there is significant (IIRC) positive SA which I can correct by using a higher-than-normal refractive index immersion oil, which introduces a compensating negative SA.
 
thank you very much for your clarification!

what I'm still asking myself is whether or not the cover glass correction corrects a phase factor of the electromagnetic field that it acquires by traveling through the cover glass. in other words, if the cover glass is thicker or thinner than it is supposed to be, do the waves that propagate towards the objective get an additional phase factor \exp ( i f(\theta)), where \theta is the angle between the k-vector and the optical axis, that leads to spherical aberration? if so, what exactly is the function f ?

thanks again!
 
omg! said:
thank you very much for your clarification!

what I'm still asking myself is whether or not the cover glass correction corrects a phase factor of the electromagnetic field that it acquires by traveling through the cover glass. in other words, if the cover glass is thicker or thinner than it is supposed to be, do the waves that propagate towards the objective get an additional phase factor \exp ( i f(\theta)), where \theta is the angle between the k-vector and the optical axis, that leads to spherical aberration? if so, what exactly is the function f ?

thanks again!

Sort of- as light passes through the coverslip, the wavefront picks up a phase factor given by what you wrote. The function f is given by the 'reduced thickness' of the glass (d/n, where d is the actual thickness and n the index of refraction), which will vary with both direction(as d varies) and color (as n varies).

If the phase factor is off-nominal (either d is out of tolerance, or n is out of tolerance), there will be a residual error in the phase that is not corrected by the imaging system. The specific phase function can be complicated, and is usually expanded in Zernike polynomials- orthogonal functions defined on the unit circle.

http://www.telescope-optics.net/zernike_coefficients.htm
 

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