2017
DOI: 10.1093/mnras/stx1540
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Diamagnetic region(s): structure of the unmagnetized plasma around Comet 67P/CG

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Cited by 65 publications
(118 citation statements)
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“…Also, the red and dark blue points, obtained at the very beginning and end of the 300‐day period of cavity crossings, respectively, do not follow the general trend. We note here that the plasma density is distributed similarly to the neutral density in Figure c, a result of the close relationship between n e and n n inside the cavity observed by Henri et al (), though the plasma density seems to have less variance within each subinterval. Thus, the plasma density does not really provide any new information by which to organize the data.…”
Section: Resultssupporting
confidence: 80%
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“…Also, the red and dark blue points, obtained at the very beginning and end of the 300‐day period of cavity crossings, respectively, do not follow the general trend. We note here that the plasma density is distributed similarly to the neutral density in Figure c, a result of the close relationship between n e and n n inside the cavity observed by Henri et al (), though the plasma density seems to have less variance within each subinterval. Thus, the plasma density does not really provide any new information by which to organize the data.…”
Section: Resultssupporting
confidence: 80%
“…Together with the intermittent nature of the signatures in LAP data, this was taken as evidence for strong filamentation of the cold plasma close to the nucleus, with individual filaments extending far outside the collisionally dominated region, perhaps even detaching from it entirely. Similar structures were observed to develop in connection to the diamagnetic cavity in global 3‐D hybrid simulations by Koenders et al () and have been proposed to result from the instability of the cavity boundary (e.g., Henri et al, ). However, observations of cold electrons are not limited to the diamagnetic cavity, so the relationship (if any) between the structure and dynamics of cold and unmagnetized plasma, respectively, is not clear.…”
Section: Introductionsupporting
confidence: 76%
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“…When the gas production rate is high enough, plasma-neutral collisions eventually carve out a nonmagnetized region near the cometary nucleus [56]. This region is shaped by electron-neutral collisions [57]. Taking into account collisions will be necessary to extend this study for more active comets.…”
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confidence: 99%