Spectrohelioscope

A spectrohelioscope is a type of <a href="/facts/Solar_telescope/5DNFP5r6">solar telescope</a> designed by <a href="/facts/George_Ellery_Hale/WWnVuHra">George Ellery Hale</a> in 1924 to allow the Sun to be viewed in a selected <a href="/facts/Wavelength/kcJU0ymz">wavelength</a> of light. The name comes from Latin- and Greek-based words: "Spectro," referring to the <a href="/facts/Optical_spectrum/frPBh8o5">optical spectrum</a>, "helio," referring to the Sun, and "scope," as in telescope.

The basic spectrohelioscope is a complex machine that uses a <a href="/facts/Spectroscope/BjshQbA8">spectroscope</a> to scan the surface of the Sun. The image from the <a href="/facts/Objective_lens/6smChS48">objective lens</a> is focused on a narrow slit revealing only a thin portion of the Sun's surface. The light is then passed through a <a href="/facts/Prism_(optics)/eodBFF70">prism</a> or <a href="/facts/Diffraction_grating/TUcyt7Do">diffraction grating</a> to spread the light into a spectrum. The spectrum is then focused on another slit that allows only a narrow part of the spectrum (the desired wavelength of light for viewing) to pass. The light is finally focused on an eyepiece so the surface of the Sun can be seen. The view, however, would be only a narrow strip of the Sun's surface. The slits are moved in unison to scan across the whole surface of the Sun giving a full image. Independently nodding mirrors can be used instead of moving slits to produce the same scan: the first mirror selects a slice of the Sun, the second selects the desired wavelength.
The <a href="/facts/Spectroheliograph/aghfzYmj">spectroheliograph</a> is a similar device, but images the Sun at a particular wavelength photographically and is still in use in professional observatories.

Spectrohelioscope open-in-new

Spectrohelioscope