Emission spectrum (IMAGE)

University of Leicester

Emission spectrum

Caption

Averaged emission spectrum between 3.4 and 4.0μm, with annotated positions of valuable H3+ emission lines (known as Q lines) found at specific wavelength locations, the brightness of each line is determined by both temperature and density of the H3+ particles in a planet's atmosphere

Credit

Source: University of Leicester

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Use only with credit.

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Original content

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