the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
Flying through the plasmasphere to optimize low-energy ion measurements
Gabriella Stenberg Wieser
Martin Wieser
Stas Barabash
Philipp Wittmann
Leif Kalla
Markus Fränz
Elias Roussos
Audrey Vorburger
Peter Wurz
Jan-Erik Wahlund
Pontus C. Brandt
Yoshifumi Futaana
Manabu Shimoyama
Angèle Pontoni
André Galli
Andreas Riedo
George Ho
Donald G. Mitchell
George Clark
Peter Kollmann
Malamati Gkioulidou
Leonardo Regoli
Norbert Krupp
Robert Wimmer-Schweingruber
Kazushi Asamura
Esa Kallio
Andrea Opitz
Manuel Grande
Andrew Coates
Geraint Jones
Theodoros Sarris
Andrey Fedorov
Nicolas André
Ján Baláž
Download
- Final revised paper (published on 17 Sep 2026)
- Preprint (discussion started on 22 Apr 2026)
Interactive discussion
Status: closed
-
RC1: 'Comment on egusphere-2026-2039', Anonymous Referee #1, 22 May 2026
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2039/egusphere-2026-2039-RC1-supplement.pdfCitation: https://doi.org/
10.5194/egusphere-2026-2039-RC1 -
AC1: 'Reply on RC1', Gabriella Stenberg Wieser, 28 Jun 2026
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2039/egusphere-2026-2039-AC1-supplement.pdf
-
AC1: 'Reply on RC1', Gabriella Stenberg Wieser, 28 Jun 2026
-
RC2: 'Comment on egusphere-2026-2039', Anonymous Referee #2, 23 May 2026
The authors of "Flying through the plasmasphere to optimize low energy ion measurements" utilize the Juice spacecraft's flyby of Earth to improve the measurement scheme of the JDC instrument. Observations from the low-energy plasmasphere revealed that the voltage stepping of the instrument differed substantially from expectation. Performing laboratory experiments with the ground-copy of the instrument, the authors demonstrate that the observations can be correctly re-ordered to remove these stepping artifacts, which are further validated by a simple numerical model of the expected plasmasphere observations. Understanding the origins of the stepping issue, the authors present new voltage stepping patterns to maximize the scientific return of the JDC instrument during Juice's primary science mission at the Jovian moons. This work highlights the value of in-flight calibration to identify, understand, and correct for instrument artifacts, and with the Juice spacecraft en route to the Jovian system, is timely. A few minor revisions are suggested.
- In section 2, the authors are recommended to describe how JDC makes measurements of negative ion and electrons. Although the focus of the work is on the positive ions observed during the Earth flyby, the manuscript makes mention in several places about the negative-charged particle measurements, including how the voltage stepping will affect them too (e.g., lines 261-263). A sentence or two description early in the work would help readers that are less familiar with this type of instrumentation.
- Can the authors comment on the systematically low count rate below ~1 eV in Figure 5? The numerical simulation of the plasmasphere (Figure 7) suggests large fluxes may be present at these energies. Since the manuscript discusses the comparison between the re-ordered observations and the numerical simulation results, including the "holes" in the flux (line 225), it would be valuable for readers to understand if the low count rate in Figure 5 below ~1 eV is expected to be related to the actual plasmasphere (e.g., differences in ion species and temperatures) or an instrumental feature (e.g., related to geometric factor).
- A distinction between JDC's capability to resolve mass versus mass-per-charge would be beneficial to include in section 2. Traditionally, reflectron instruments are primarily capable of distinguishing species of different mass-per-charge. Does JDC enable resolution of mass and charge state? If so, that would be valuable to clarify since the plasmasphere can contain multiply charged species (e.g., line 104). If JDC only resolves mass-per-charge then it should be clarified if these plasmasphere observations are assumed to contain only singly charged species.
- To aid in readers' mapping the different voltage stepping presented in Figures 3-5 it is recommended that the vertical range in Figure 4 is lowered. Comparing Figures 3 and 5, voltage step 73 exhibits a substantial re-ordering from ~0.1 eV in Figure 3 to ~4 eV in Figure 4. Since this step contains some of the highest count rates it would be valuable for readers to compare the expected vs. actual voltages in Figure 4, however, this is below the vertical axis of the plot.
Technical corrections:
- It should be clarified if Figures 3 and 5 show counts (as listed in the figure caption) or counts-per-second (as suggested by the "cps" label). Showing counts would be helpful to readers since it illustrates the instrument sensitivity (e.g., the 1-count limit) and uncertainty (e.g., Poisson).
Citation: https://doi.org/10.5194/egusphere-2026-2039-RC2 -
AC2: 'Reply on RC2', Gabriella Stenberg Wieser, 28 Jun 2026
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2039/egusphere-2026-2039-AC2-supplement.pdf