Ahoj, What is the wavelength of the CIII line?
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The C III (Carbon III) line refers to the emission line of ionized carbon (C²⁺), where the carbon atom has lost two electrons. One of the most prominent C III emission lines is found in the ultraviolet part of the electromagnetic spectrum.

The C III line is typically observed at a wavelength of 977 Ångströms (Å), which corresponds to 97.7 nanometers (nm) in the UV spectrum. This line originates from the transition of an ionized carbon atom in the C III state.

Would you like more details about the emission or absorption processes of this line?






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a O V (kyslík V)
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The O V (Oxygen V) line corresponds to highly ionized oxygen, where the oxygen atom has lost four electrons (O⁴⁺).

One of the most prominent emission lines for O V is found at a wavelength of 629.73 Ångströms (Å), which is 62.97 nanometers (nm). This line appears in the extreme ultraviolet (EUV) region of the electromagnetic spectrum.

This line is frequently observed in astrophysical contexts, such as in solar spectra or in hot plasmas, where temperatures are high enough to ionize oxygen to this degree.

Would you like further details about its use in plasma diagnostics or spectroscopy?






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a posledni C VI ?
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The C VI (Carbon VI) line corresponds to highly ionized carbon, where the carbon atom has lost five electrons (C⁵⁺). This means only one electron remains in the atom, similar to a hydrogen-like ion.

One of the most prominent emission lines for C VI is found at a wavelength of 33.73 Ångströms (Å), or 3.373 nanometers (nm), in the X-ray region of the electromagnetic spectrum. This line is associated with transitions in very hot plasmas, such as those found in the solar corona, fusion reactors, and astrophysical plasmas.

This C VI line is often used in diagnostics of high-temperature plasmas, like those in tokamaks or astrophysical objects.