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  2. Fluorescence anisotropy - Wikipedia

    en.wikipedia.org/wiki/Fluorescence_anisotropy

    The grating factor G is an instrumental preference of the emission optics for the horizontal orientation to the vertical orientation. It can be measured by moving the excitation polarizer to the horizontal orientation and comparing the intensities when the emission polarizer is vertically and horizontally polarized respectively.

  3. Blazed grating - Wikipedia

    en.wikipedia.org/wiki/Blazed_grating

    A special form of a blazed grating is the echelle grating. It is characterized by particularly large blaze angle (>45°). Therefore, the light hits the short legs of the triangular grating lines instead of the long legs. Echelle gratings are mostly manufactured with larger line spacing but are optimized for higher diffraction orders.

  4. Diffraction grating - Wikipedia

    en.wikipedia.org/wiki/Diffraction_grating

    A blazed diffraction grating reflecting only the green portion of the spectrum from a room's fluorescent lighting. For a diffraction grating, the relationship between the grating spacing (i.e., the distance between adjacent grating grooves or slits), the angle of the wave (light) incidence to the grating, and the diffracted wave from the grating is known as the grating equation.

  5. Grating - Wikipedia

    en.wikipedia.org/wiki/Grating

    A grating can be defined by six parameters: Spatial frequency is the number of cycles occupying a particular distance (e.g. 10 line pairs per millimeter). The period of the grating is the inverse of the spatial frequency, measured in distance (e.g. 0.1 mm). Duty Cycle is the relative thickness of high and low lines. The duty cycle is the ratio ...

  6. Observational error - Wikipedia

    en.wikipedia.org/wiki/Observational_error

    Systematic errors can also be detected by measuring already known quantities. For example, a spectrometer fitted with a diffraction grating may be checked by using it to measure the wavelength of the D-lines of the sodium electromagnetic spectrum which are at 600 nm and 589.6 nm. The measurements may be used to determine the number of lines per ...

  7. Why do we leave Christmas cookies for Santa? Chef ... - AOL

    www.aol.com/why-leave-christmas-cookies-santa...

    How did families come to leave cookies and milk for Santa Claus on Christmas? A celebrity chef told Fox News Digital how the tradition got its start and why a chocolate chip cookie is the best.

  8. The Fastest Way to Debloat After a Big Meal, According to ...

    www.aol.com/fastest-way-debloat-big-meal...

    Well, it comes down to simple biology. Natalie Rizzo, M.S., RD, author of Planted Performance and founder of Greenletes, shares, “Gentle movement, like walking, may reduce bloating after a meal ...

  9. Acousto-optics - Wikipedia

    en.wikipedia.org/wiki/Acousto-optics

    which is known as the Klein–Cook parameter. Since, in general, only the first order diffraction maximum is used in acousto-optic devices, Bragg diffraction is preferable due to the lower optical losses. However, the acousto-optic requirements for Bragg diffraction limit the frequency range of acousto-optic interaction. As a consequence, the ...

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