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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
Ion-Ion Cross-Field Instability of Lower Hybrid Waves in the Inner Coma of Comet 67P
DOI: 10.1029/2022JA030535 Bibcode: 2022JGRA..12730535O

Karlsson, Tomas; Stenberg Wieser, Gabriella; Odelstad, Elias +2 more

We show that an ion-ion cross-field streaming instability between cold newborn cometary ions and heated heavy ions that were picked up upstream is likely a contributing source of observed lower hybrid (LH) waves in the inner coma of comet 67P/Churyumov-Gerasimenko. Electric field oscillations in the LH frequency range are common here, and have pre…

2022 Journal of Geophysical Research (Space Physics)
Rosetta 1
Observations of a Solar Energetic Particle Event From Inside and Outside the Coma of Comet 67P
DOI: 10.1029/2022JA030398 Bibcode: 2022JGRA..12730398W

Coates, A. J.; Palmerio, E.; Jones, G. H. +12 more

We analyze observations of a solar energetic particle (SEP) event at Rosetta's target comet 67P/Churyumov-Gerasimenko during 6-10 March 2015. The comet was 2.15 AU from the Sun, with the Rosetta spacecraft approximately 70 km from the nucleus placing it deep inside the comet's coma and allowing us to study its response. The Eastern flank of an int…

2022 Journal of Geophysical Research (Space Physics)
Rosetta 1
The Influence of Spacecraft Charging on Low-Energy Ion Measurements Made by RPC-ICA on Rosetta
DOI: 10.1029/2019JA027478 Bibcode: 2020JGRA..12527478B

Stenberg Wieser, Gabriella; Wieser, Martin; Eriksson, Anders +2 more

Spacecraft charging is problematic for low-energy plasma measurements. The charged particles are attracted to or repelled from the charged spacecraft, affecting both the energy and direction of travel of the particles. The Ion Composition Analyzer (RPC-ICA) on board the Rosetta spacecraft is suffering from this effect. RPC-ICA was measuring positi…

2020 Journal of Geophysical Research (Space Physics)
Rosetta 33
The Influence of Varying Spacecraft Potentials and Debye Lengths on In Situ Low-Energy Ion Measurements
DOI: 10.1029/2020JA027870 Bibcode: 2020JGRA..12527870B

Stenberg Wieser, Gabriella; Wieser, Martin; Eriksson, Anders +2 more

Low-energy ions are difficult to measure, mainly due to spacecraft charging. The ions are attracted to or repelled from the charged surface prior to detection, which changes both the energy and travel direction of the ions. This results in distortions of the data, and the changed travel directions distort the effective field of view (FOV) of the i…

2020 Journal of Geophysical Research (Space Physics)
Rosetta 18
Plasma Density and Magnetic Field Fluctuations in the Ion Gyro-Frequency Range Near the Diamagnetic Cavity of Comet 67P
DOI: 10.1029/2020JA028592 Bibcode: 2020JGRA..12528592O

Nilsson, H.; André, M.; Vaivads, A. +8 more

We report the detection of large-amplitude, quasi-harmonic density fluctuations with associated magnetic field oscillations in the region surrounding the diamagnetic cavity of comet 67P. Typical frequencies are ∼0.1 Hz, corresponding to ∼10 times the water and ≲ 0.5 times the proton gyro-frequencies, respectively. Magnetic field oscillations are n…

2020 Journal of Geophysical Research (Space Physics)
Rosetta 6
Plasma Turbulence at Comet 67P/Churyumov-Gerasimenko: Rosetta Observations
DOI: 10.1029/2020JA028100 Bibcode: 2020JGRA..12528100R

Halekas, J. S.; Howes, G. G.; Ruhunusiri, S.

We perform a power spectral analysis of magnetic field fluctuations measured by the Rosetta spacecraft's magnetometer at comet 67P/Churyumov-Gerasimenko. We interpret the power spectral signatures in terms of plasma turbulent processes and discover that different turbulent processes are prominent during different active phases of the comet. During…

2020 Journal of Geophysical Research (Space Physics)
Rosetta 3
Ion Velocity and Electron Temperature Inside and Around the Diamagnetic Cavity of Comet 67P
DOI: 10.1029/2018JA025542 Bibcode: 2018JGRA..123.5870O

André, M.; Henri, P.; Rubin, M. +7 more

A major point of interest in cometary plasma physics has been the diamagnetic cavity, an unmagnetized region in the innermost part of the coma. Here we combine Langmuir and Mutual Impedance Probe measurements to investigate ion velocities and electron temperatures in the diamagnetic cavity of comet 67P, probed by the Rosetta spacecraft. We find io…

2018 Journal of Geophysical Research (Space Physics)
Rosetta 42