High-resolution spectra of Io's sodium emission

Details High-resolution spectra of Io's sodium emission High-resolution spectra of Io's sodium emission

Dec 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...202l.107t&link_type=abstract

Astrophysical Journal, vol. 202, Dec. 1, 1975, pt. 2, p. L107-L112.

Astronomy and Astrophysics

Astrophysics

14

D Lines, Emission Spectra, Io, Jupiter (Planet), Line Spectra, High Resolution, Hyperfine Structure, Red Shift, Resonance Scattering, Sodium

Scientific paper

The shape of Io's sodium D2 emission profile varies markedly with Io's
orbital phase, and its width suggests that the sodium cloud may be
expanding with velocities up to 18 km/sec. This offers an explanation
for at least part of the orbital phase asymmetry observed for the D-line
emission.

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