Diurnal variation of dust and gas production in comet 67P/Churyumov-Gerasimenko at the inbound equinox as seen by OSIRIS and VIRTIS-M on board Rosetta

Rosetta mission full comet phase results

Open Access

Fig. 8

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Azimuthal profiles of dust brightness and gas band intensity. OSIRIS dust is shown as blue triangles, VIRTIS-M H₂O as red squares, and VIRTIS-M CO₂ as green circles. For displaying purposes, the VIRTIS-M H₂O and CO₂ band area intensities are scaled to the OSIRIS dust values.

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