Wavelength and precision of observation

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SUMMARY

The discussion centers on the relationship between wavelength and observation precision, emphasizing the diffraction limit as formulated by Abbe. It establishes that shorter wavelengths yield higher resolution due to a larger wave-vector magnitude, enabling the transmission of a broader range of spatial frequencies. The conversation highlights that systems with higher numerical apertures can achieve better resolution, and introduces the concept of evanescent waves, which can be utilized in near-field and super-resolution imaging techniques. The diffraction limit is quantified as approximately half the wavelength, indicating that for a wavelength of 590 nm, the smallest observable detail is around 295 nm.

PREREQUISITES
  • Understanding of diffraction limit principles
  • Familiarity with spatial frequencies and wave-vectors
  • Knowledge of numerical aperture in optical systems
  • Basic concepts of evanescent waves and their applications
NEXT STEPS
  • Research the principles of near-field imaging techniques
  • Explore super-resolution microscopy methods
  • Study the mathematical foundations of Fourier transforms in optics
  • Investigate the role of numerical aperture in optical resolution
USEFUL FOR

Optical engineers, physicists, and researchers in microscopy and imaging technologies will benefit from this discussion, particularly those focused on enhancing resolution in optical systems.

annie122
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I don't understand why when you make an observation, you need a wavelength shorter than the wanted precision.
i.e. you can't make clear pictures of golf balls with radio waves, you can't observe things smaller than a photon with an optical microscope.
 
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It is due to the diffraction limit, first formulated by Abbe. The essence of the diffraction limit is as follows;

- The resolution of an optical field is given by the range of spatial frequencies (or wave-vectors) present. Sharper details require more spatial frequencies to be present, i.e. typical Fourier transform principles apply.

- A focusing system can only transmit a limited range of spatial frequencies. For a monochromatic wave (fixed wave-vector magnitude), the size of the transverse wave-vector components depends on the angle made with the optic axis. Hence systems with a higher numerical aperture (or acceptance angle) are capable of higher resolution in the transverse (image) plane because they can transmit a higher range of spatial frequencies (parallel to that plane).

- Shorter wavelengths are capable of higher resolution because the overall magnitude of the wave-vector is larger (k = 2*pi/wavelength).

- Even free-space limits resolution. To obtain a transverse frequency component greater than the magnitude of the wave-vector, one of the components must become imaginary. This results in wave components that are evanescent. Evanescent waves are bound the surface (or source) that generates them and do not propagate through free-space. The decay length of these waves is on the scale of one wavelength or less.

- The diffraction limit can therefore be circumvented if the evanescent waves can somehow be detected. This is the basic principle behind most near-field imaging and super-resolution imaging methods.

- For most definitions of resolution, the diffraction limit is around half the wavelength, i.e. for a wavelength of 590 nm, the smallest detail that can be transmitted to the far-field (i.e. beyond a few wavelengths) is around 295 nm.

Claude.
 
X2 on all Claude said, It helps me to think about it in terms of waves and phase.
When you only have one detector, you can tell when a reflection occurred only within one wavelength. The only way to get better is to bring in some phase info, which cannot be done with a single detector. Think of the wavelengths as integer measuring sticks, you can only measure something in whole stick units, The smaller the stick unit, the more accurate the measurement.
 

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