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| Content Provider | IEEE Xplore Digital Library |
|---|---|
| Author | Sjogren, A. Eriksson, A.I. Cully, C.M. |
| Copyright Year | 1973 |
| Abstract | Plasma measurements by electrostatic probes are influenced by the spacecraft-plasma interaction, including the photoelectrons emitted by the spacecraft. Such effects get particularly important in tenuous plasmas with large Debye lengths. We have used the particle-in-cell code package SPIS to study the close environment of the Rosetta spacecraft, and the impact of the spacecraft-plasma interaction on the electrostatic potential at the position of the Langmuir probes onboard. The simulations show that in the solar wind, photoemission has a bigger impact than wake formation. Spacecraft potential estimates based on Langmuir probe data in the solar wind need to be compensated for these effects when the spacecraft attitude varies. The SPIS simulations are validated by comparison to an independent code. |
| Sponsorship | IEEE Nuclear and Plasma Sciences Society |
| Starting Page | 1257 |
| Ending Page | 1261 |
| Page Count | 5 |
| File Size | 938620 |
| File Format | |
| ISSN | 00933813 |
| Volume Number | 40 |
| Issue Number | 4 |
| Language | English |
| Publisher | Institute of Electrical and Electronics Engineers, Inc. (IEEE) |
| Publisher Date | 2012-04-01 |
| Publisher Place | U.S.A. |
| Access Restriction | One Nation One Subscription (ONOS) |
| Rights Holder | Institute of Electrical and Electronics Engineers, Inc. (IEEE) |
| Subject Keyword | Probes Space vehicles Plasmas Plasma measurements Electric potential Photoelectricity Computational modeling SPIS Rosetta mission spacecraft charging |
| Content Type | Text |
| Resource Type | Article |
| Subject | Nuclear and High Energy Physics Condensed Matter Physics |
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