How Does Angular Resolution Differ from Other Types of Resolution?

In summary: There are multiple measures of 'resolution' (e.g. Rayleigh, Sparrow, Dawes...), but the essential concept is the ability to distinguish 2 closely spaced objects.
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21joanna12
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The Wikipedia definition of angular resolution is 'Angular resolution, or spatial resolution, describes the ability of any image-forming device such as an optical or radio telescope, a microscope, a camera, or an eye, to distinguish small details of an object, thereby making it a major determinant of image resolution.'

I get this definition, however it seems to me like the definition of plain 'resolution'. Are there more different types of resolution? And if so, how do they differ?

Thank you in advance :)
 
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Methinks you are reading too much into it, and it means exactly what it sounds like. It's resolution measured in angle units, as opposed to resolution measured in some linear measure like dots per inch.
 
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Yes, you can turn angular resolution into, say, resolution in pixels, fairly easily if you know the angular resolution of the imaging system and the size of the pixels on the imaging sensor.
 
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21joanna12 said:
<snip> Are there more different types of resolution? And if so, how do they differ?

Analysis of imaging systems is often simplified by describing the system in terms of angles from the optical axis rather than distance form the optical axis, especially when the objects are very far away. Converting from angles to linear distances at the image plane is generally straightforward.

There are multiple measures of 'resolution' (e.g. Rayleigh, Sparrow, Dawes...), but the essential concept is the ability to distinguish 2 closely spaced objects.

http://www.google.com/url?sa=t&rct=...KpA6KlgKnxyHYIw&bvm=bv.83640239,d.aWw&cad=rja
 
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Andy Resnick said:
the essential concept is the ability to distinguish 2 closely spaced objects

When the term 'resolution' was first used, it referred to optical systems using the eye as the receptor. The Rayleigh Criterion was a fairly arbitrary criterion and assumed that two angularly small objects (stars etc) could be said to be resolvable if the dip in brightness between the two images went to half. That assumed that the brightness of the images (signal level) was enough to be able to detect that 'dip'. In practice, it's down to Signal to Noise Ratio, whether you can see the dip or not. With modern sensors and signal processing, the noise can be reduced by filtering and you can detect a much shallower 'dip' allowing you to resolve much better than the Rayleigh Criterion would suggest.
 

What is angular resolution?

Angular resolution is a measure of the ability of a telescope or imaging system to distinguish between two distinct objects that are close together in the sky. It represents the smallest angle between two points that can still be resolved as separate entities.

How is angular resolution calculated?

Angular resolution is calculated by taking the wavelength of light used and dividing it by the diameter of the aperture, or opening, of the telescope or imaging system. This results in a value known as the diffraction limit, which represents the smallest angle that can be resolved by the system.

What factors affect angular resolution?

The main factors that affect angular resolution are the wavelength of light used and the diameter of the aperture. Generally, shorter wavelengths and larger apertures result in better angular resolution. Atmospheric conditions and the quality of the optics can also play a role in determining the final angular resolution.

Why is angular resolution important?

Angular resolution is important because it allows us to see fine details in astronomical objects, such as distant stars and galaxies. It also helps us to distinguish between objects that are close together, which is crucial for accurately observing and studying these objects.

How does angular resolution differ from spatial resolution?

While angular resolution refers to the ability to distinguish between objects in the sky, spatial resolution is a measure of the ability to distinguish between objects on the ground or in an image. Spatial resolution takes into account factors such as pixel size, while angular resolution is primarily determined by the properties of the telescope or imaging system.

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