Wavelength and precision of observation

In summary, Claude X2 said that the diffraction limit is the size of the wave-vector that can be transmitted with a focusing system. If you only have a single detector, you can only tell when a reflection occurred within one wavelength. Bringing in phase info would be necessary to improve the resolution.
  • #1
annie122
51
0
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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  • #2
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.
 
  • #3
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.
 

Related to Wavelength and precision of observation

1. What is the relationship between wavelength and precision of observation?

The shorter the wavelength, the higher the precision of observation. This is because shorter wavelengths can provide more detailed and accurate information about an object or phenomenon.

2. How do different wavelengths affect the precision of observation?

Different wavelengths can have varying levels of precision in observation. Generally, shorter wavelengths (such as X-rays and gamma rays) have higher precision, while longer wavelengths (such as radio waves) have lower precision.

3. Can the precision of observation be improved by using multiple wavelengths?

Yes, using multiple wavelengths can improve the precision of observation. By combining data from different wavelengths, scientists can get a more complete and accurate understanding of an object or phenomenon.

4. How does the type of instrument used impact the precision of observation?

The type of instrument used can have a significant impact on the precision of observation. For example, telescopes with larger apertures can collect more light and provide higher precision observations of objects in the night sky.

5. What factors can affect the precision of observation besides wavelength?

Besides wavelength, other factors that can affect the precision of observation include atmospheric conditions, instrument calibration, and the skill of the observer. These factors should be taken into consideration when interpreting data and results.

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