Figure 1 from ON THE ORIGIN OF INNER COMA STRUCTURES OBSERVED BY ROSETTA DURING A DIURNAL ROTATION OF COMET 67P/CHURYUMOV

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ON THE ORIGIN OF INNER COMA STRUCTURES OBSERVED BY ROSETTA DURING A DIURNAL ROTATION OF COMET 67P/CHURYUMOV–GERASIMENKO

Authors: Tobias Kramer, and Matthias Noack

2016 The Astrophysical Journal Letters 823 L11.

Provider: AAS Journals

Caption: Figure 1.

Dust trajectories above concave areas. Homogeneously seeded dust particles are entrenched and accelerated by outflowing gas within the outer mantle. Concavely shaped surface areas lead to the collimation of dust.

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