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INSTITUTET FÖR RYMDFYSIK |
UPPSALA |
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Swedish Institute of Space Physics |
(59°50.272′N, 17°38.786′E) |
Student project at IRF Uppsala
Project work / Examensarbete (30 hp)
Simulations of Langmuir probes in space
Student: vacant
Supervisor: Anders Eriksson
Period: 20 weeks, starting soon as possible!
Background
Langmuir probes are conceptually simple instruments for the
characterization of space plasma parameters like density, temperature
and flow speed. During the years, we have built Langmuir probes for a
number of spacecraft, of which the most recent are NASA's Cassini (at Saturn) and ESA's Rosetta (on its way to a
comet).
There are a lot of theoretical investigations showing how to interpret
Langmuir probe data and derive the plasma parameters from the primary
current measurements. However, the detailed influence of perturbations
from the spacecraft depends on the configuration on each spacecraft,
and here no general theory exists. Numerical simulations are needed in
most cases.
Project
Use the
ESA-sponsored open-source package SPIS
(Spacecraft Plasma Interaction System) to simulate the measurements on
Rosetta and/or Cassini, and compare the simulations to actual data. The
project will involve interactions with other scientists at IRF Uppsala
and at KTH in Stockholm, and possibly with other research groups,
particularly in France and at ESA's technical facility in Holland,
ESTEC.
Completed and ongoing projects
There has been a series of students working on these kind of simulations,
often working closely together and with other scientists abroad:
Contact
Anders.Eriksson@irfu.se
ESA's comet hunter Rosetta, with the two Langmuir probes from IRF
Uppsala at the end of the booms protruding from the spacecraft. Each
probe is a sphere of 50 mm diameter.
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