We lose only a factor of two in angular resolution.

The angular resolution of these devices is typically very poor.

The sharpness of images is what astronomers call angular resolution.

The angular resolution was less than 5 arcsec at half energy width.

As a result, it will have angular resolutions between a few arcminutes and several degrees.

The angular resolution of the naked eye is about 1'; however, some people have sharper vision than that.

The ability to determine parallax is limited by the angular resolution of the instrument used.

Optic choices affect the angular resolution and range that can be detected.

The equation shows that, all else being equal, the larger the aperture, the better the angular resolution.

The human eye in its best years has a maximum angular resolution of one minute of arc.

Current missions cannot do this because the required Angular resolution is limited and magnetic fields are invisible.

This means that the angular resolution of a diffraction limited system is given by the same formulae.

However, the low angular resolution can introduce some unwanted aliasing artifacts.

Angular resolution at short ranges is better than radar due to the shorter wavelength.

Angular resolution is a measure of the sharpest angles in a graph drawing.

They are often used separately, but they can be used together to get a very high angular resolution.

When all the telescopes are combined, the facility can achieve an angular resolution of about 0.001 arc-second.

Point-like sources separated by an angle smaller than the angular resolution cannot be resolved.

It combines the light from four telescopes simultaneously and provide the equivalent angular resolution of a 100 m telescope.

The angular resolution was 5.5 degrees, with a temperature resolution of 0.6 mK.

It can be viewed as serial topography with additional angular resolution in the exit beam.

The tightly packed array of narrow individual beams provides very high angular resolution and accuracy.

The angular resolution and field of view at each resolution were as follows:

The smallest angular resolution that can be reached is about 0.05 arcseconds at a wavelength of 7 mm.

To achieve higher angular resolution, some infrared telescopes are combined to form astronomical interferometers.