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Dayside-to-nightside dust coma brightness asymmetry and its implications for nightside activity at Comet 67P/Churyumov–Gerasimenko

  • Published:2020-11 Issue: Volume:351 Page:113968
  • ISSN:0019-1035
  • Container-title:Icarus
  • language:en
  • Short-container-title:Icarus

Author:

Gerig S.-B.,Pinzón-Rodríguez O.,Marschall R.,Wu J.-S.,Thomas N.

Funder

Swiss National Science Foundation

NCCR PlanetS, Switzerland

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference54 articles.

1. The scattering phase function of comet 67P/Churyumov-Gerasimenko coma as seen from the Rosetta/OSIRIS instrument;Bertini;Mon. Not. R. Astron. Soc.,2017

2. Comparison of 3D kinetic and hydrodynamic models to ROSINA-COPS measurements of the neutral coma of 67P/Churyumov-Gerasimenko;Bieler;Astron. Astrophys.,2015

3. Molecular Gas Dynamics and the Direct Simulation of Gas Flows, Vol. 5;Bird,1994

4. First observations of H2O and CO2 vapor in comet 67P/Churyumov-Gerasimenko made by VIRTIS onboard Rosetta;Bockelée-Morvan;Astron. Astrophys.,2015

5. Absorption and Scattering of Light by Small Particles;Bohren,1983

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