Astrophysics (Index)About

disperser

(dispersing element)
(prism, grating, or grism within a spectrometer)

The term disperser (or dispersing element) refers to the part of a spectrometer that disperses incoming light by wavelength, i.e., directs the light differently according to its wavelength so that the spectrum is evident. Bending the light's direction according to wavelength to spread it out in such manner is termed dispersion, or more specifically, chromatic dispersion. Example dispersers are prisms, gratings, grisms, and Fabry-Pérot interferometers.


(telescopes,spectrometers)
Further reading:
https://en.wikipedia.org/wiki/Prism
https://en.wikipedia.org/wiki/Diffraction_grating
https://en.wikipedia.org/wiki/Grism
https://en.wikipedia.org/wiki/Dispersion_(optics)
https://e-l.unifi.it/pluginfile.php/1082493/mod_resource/content/1/APPUNTI_2020_lezione_16_slide%20A.Bianco..pdf
https://science.uct.ac.za/sites/default/files/content_migration/science_uct_ac_za/1471/files/spec1.pdf
http://www2.lowell.edu/users/massey/Massey_Hanson.pdf
https://sites.astro.caltech.edu/~george/ay122/Ay122a_Spectroscopy.pdf
https://slideplayer.com/slide/12583322/
http://astronomy.nmsu.edu/cwc/Teaching/ASTR605/Lectures/spectra.pdf

Referenced by pages:
absorption line
back end instrument
chromatic aberration
cross dispersion spectrograph
emission line
European Extremely Large Telescope (E-ELT)
European Southern Observatory Very Large Telescope (ESO VLT)
Fabry-Pérot interferometer (FPI)
front end instrument
grating
grism
HRS
immersion grating
Isaac Newton Telescope (INT)
NIRSpec
refractive index
slitless spectrograph
spectrograph
spectroscope
spectroscopy
velocity dispersion (σ)
William Herschel Telescope (WHT)

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