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  2. Free-air gravity anomaly - Wikipedia

    en.wikipedia.org/wiki/Free-air_gravity_anomaly

    Calculation. The free-air gravity anomaly is given by the equation: = (+) Here, is observed gravity, is the free-air correction, and is theoretical gravity.

  3. Prism correction - Wikipedia

    en.wikipedia.org/wiki/Prism_correction

    Prism correction is commonly specified in prism dioptres, a unit of angular measurement that is loosely related to the dioptre. Prism dioptres are represented by the Greek symbol delta (Δ) in superscript.

  4. Fresnel equations - Wikipedia

    en.wikipedia.org/wiki/Fresnel_equations

    In the above formula for r s ‍, if we put = ⁡ / ⁡ (Snell's law) and multiply the numerator and denominator by 1 / n 1 sin θ t ‍, we obtain r s = − sin ⁡ ( θ i − θ t ) sin ⁡ ( θ i + θ t ) . {\displaystyle r_{\text{s}}=-{\frac {\sin(\theta _{\text{i}}-\theta _{\text{t}})}{\sin(\theta _{\text{i}}+\theta _{\text{t}})}}.}

  5. Minimum deviation - Wikipedia

    en.wikipedia.org/wiki/Minimum_deviation

    The formula for minimum deviation can be derived by exploiting the geometry in the prism. The approach involves replacing the variables in the Snell's law in terms of the Deviation and Prism Angles by making the use of the above properties.

  6. Brewster's angle - Wikipedia

    en.wikipedia.org/wiki/Brewster's_angle

    For a glass medium ( n2 ≈ 1.5) in air ( n1 ≈ 1 ), Brewster's angle for visible light is approximately 56°, while for an air-water interface ( n2 ≈ 1.33 ), it is approximately 53°. Since the refractive index for a given medium changes depending on the wavelength of light, Brewster's angle will also vary with wavelength.

  7. Two-body problem in general relativity - Wikipedia

    en.wikipedia.org/wiki/Two-body_problem_in...

    e. The two-body problem in general relativity (or relativistic two-body problem) is the determination of the motion and gravitational field of two bodies as described by the field equations of general relativity. Solving the Kepler problem is essential to calculate the bending of light by gravity and the motion of a planet orbiting its sun.

  8. Eötvös effect - Wikipedia

    en.wikipedia.org/wiki/Eötvös_effect

    The mathematical derivation for the Eötvös effect for motion along the Equator explains the factor 2 in the first term of the Eötvös correction formula. What remains to be explained is the cosine factor. Because of its rotation, the Earth is not spherical in shape, there is an Equatorial bulge.

  9. Spherical aberration - Wikipedia

    en.wikipedia.org/wiki/Spherical_aberration

    Correction. In lens systems, aberrations can be minimized using combinations of convex and concave lenses, or by using aspheric lenses or aplanatic lenses. Lens systems with aberration correction are usually designed by numerical ray tracing. For simple designs, one can sometimes analytically calculate parameters that minimize spherical aberration.

  10. Newton's law of universal gravitation - Wikipedia

    en.wikipedia.org/wiki/Newton's_law_of_universal...

    In spiral galaxies, the orbiting of stars around their centers seems to strongly disobey both Newton's law of universal gravitation and general relativity. Astrophysicists, however, explain this marked phenomenon by assuming the presence of large amounts of dark matter.

  11. Dispersion (optics) - Wikipedia

    en.wikipedia.org/wiki/Dispersion_(optics)

    In particular, for non-magnetic materials ( μ = μ0 ), the susceptibility χ that appears in the Kramers–Kronig relations is the electric susceptibility χe = n2 − 1. The most commonly seen consequence of dispersion in optics is the separation of white light into a color spectrum by a prism.