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Changes in the Physical Environment of the Inner Coma of 67P/Churyumov-Gerasimenko with Decreasing Heliocentric Distance
DOI: 10.3847/0004-6256/152/5/130 Bibcode: 2016AJ....152..130B

Jorda, L.; Lamy, P. L.; Lara, L. M. +43 more

The Wide Angle Camera of the OSIRIS instrument on board the Rosetta spacecraft is equipped with several narrow-band filters that are centered on the emission lines and bands of various fragment species. These are used to determine the evolution of the production and spatial distribution of the gas in the inner coma of comet 67P with time and helio…

2016 The Astronomical Journal
Rosetta 35
Model-Observation Comparisons of Electron Number Densities in the Coma of 67P/Churyumov-Gerasimenko during January 2015
DOI: 10.3847/0004-6256/152/3/59 Bibcode: 2016AJ....152...59V

Altwegg, K.; Henri, P.; Edberg, N. J. T. +7 more

During 2015 January 9-11, at a heliocentric distance of ∼2.58-2.57 au, the ESA Rosetta spacecraft resided at a cometocentric distance of ∼28 km from the nucleus of comet 67P/Churyumov-Gerasimenko, sweeping the terminator at northern latitudes of 43°N-58°N. Measurements by the Rosetta Orbiter Spectrometer for Ion and Neutral Analysis/Comet Pressure…

2016 The Astronomical Journal
Rosetta 28