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Solar Wind Protons Forming Partial Ring Distributions at Comet 67P
DOI: 10.1029/2022JA031082 Bibcode: 2023JGRA..12831082M

Gunell, H.; Nilsson, H.; Richter, I. +5 more

We present partial ring distributions of solar wind protons observed by the Rosetta spacecraft at comet 67P/Churyumov-Gerasimenko. The formation of ring distributions is usually associated with high activity comets, where the spatial scales are larger than multiple ion gyroradii. Our observations are made at a low-activity comet at a heliocentric …

2023 Journal of Geophysical Research (Space Physics)
Rosetta 3
Indirect Observations of Electric Fields at Comet 67P
DOI: 10.1029/2023JA031746 Bibcode: 2023JGRA..12831746M

Gunell, H.; Nilsson, H.; Goetz, C. +2 more

No spacecraft visiting a comet has been equipped with instruments to directly measure the static electric field. However, the electric field can occasionally be estimated indirectly by observing its effects on the ion velocity distribution. We present such observations made by the Rosetta spacecraft on 19 April 2016, 35 km from the nucleus. At thi…

2023 Journal of Geophysical Research (Space Physics)
Rosetta 2
Solar Wind Protons in the Diamagnetic Cavity at Comet 67P/Churyumov-Gerasimenko
DOI: 10.1029/2022JA031249 Bibcode: 2023JGRA..12831249G

Nilsson, Hans; Goetz, Charlotte; Volwerk, Martin +5 more

The plasma environment at a comet can be divided into different regions with distinct plasma characteristics. Two such regions are the solar wind ion cavity, which refers to the part of the outer coma that does not contain any solar wind ions anymore; and the diamagnetic cavity, which is the region of unmagnetized plasma in the innermost coma. Fro…

2023 Journal of Geophysical Research (Space Physics)
Rosetta 1