Use Formula Resolution For Free

In order to increase the resolution, d = ?/(2NA), the specimen must be viewed using either a shorter wavelength (?) of light or through an imaging medium with a relatively high refractive index or with optical components which have a high NA (or, indeed, a combination of all of these factors).

As the wavelength of light is 400?700 nm, the resolution of a light microscopes is ~250?420 nm. For electron microscopes, the electron wavelength ? depends on the h2 accelerating voltage V. Within the classical approximation, ? = h 2 2 meV , where h is Planck's constant, m is the mass and e the charge of the electron.

Resolution is a proof technique that works on conjunctive normal form expressions by (1) selecting two clauses that contain conflicting terms, (2) combining the terms contained in those two clauses, and then (3) canceling the terms that conflict.

The resolution rule is applied to all possible pairs of clauses that contain complementary literals. After each application of the resolution rule, the resulting sentence is simplified by removing repeated literals. If the clause contains complementary literals, it is discarded (as a tautology).

Resolution rules are a set of criteria that the system uses to define how compared entities resolve (if they are or are not the same entity) and relate (if entities are not resolved to the same entity, how many attributes they share).

In our lab a 10x objective has a resolution of 0.7 microns and a 100x objective has a resolution of 0.2 microns. One other tradeoff to consider: higher magnification lenses look at smaller fields of view, in proportion to their magnification.

In order to increase the resolution, d = ?/(2NA), the specimen must be viewed using either a shorter wavelength (?) of light or through an imaging medium with a relatively high refractive index or with optical components which have a high NA (or, indeed, a combination of all of these factors).

The Rayleigh criterion stated in the equation ?=1.22?D ? = 1.22 ? D gives the smallest possible angle ? between point sources, or the best obtainable resolution. Once this angle is found, the distance between stars can be calculated, since we are given how far away they are.