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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)
The electrostatic
potential of the Rosetta spacecraft
Student: Jonny
Jansson,
Uppsala University
Supervisor:
Anders Eriksson
Period: Autumn
2007
Background
Rosetta is an
ESA spacecraft launched in 2004, presently en route to comet
Churyomov-Gerasimenko, which it will reach in 2014. The Swedish
Institute of Space Physics in Uppsala has contributed a Langmuir probe
instrument (LAP) to Rosetta, for measurement of plasma parameters like
density and electron temperature. Until reaching the fully developed
cometary coma, the plasma environment for most Rosetta operations is
the solar wind, characterized by densities in the range of a few to a
few tens of particles per cm3. The potentially best method
for LAP to measure these low densities is by measurement of the
spacecraft potential, which is related to the plasma density,
usually by an exponential relation. However, as Rosetta has solar
panels with large exposed areas at varying positive potential, the
exact form of the relation relevant for Rosetta is not known. This is
the topic for the present investigation.
Project
Construct an
analytical model for the density-potential relation, n = f(V). Compare predictions from
this model to data available from Rosetta's Earth and Mars swing-by
maneouvres, and to solar wind data. Investigate the relation between
the potential measured by the LAP probes and the spacecraft potential
to infinity. A possible extension could be the use of numerical
modelling, using the SPIS software package (www.spis.org), for
investigations of how the potential measured by LAP relates to the true
spacecraft potential for different attitudes, in vacuum (due to solar
panel orientation) and possibly in a plasma (including the spaceraft
photoelectron cloud).
![[Rosetta]](../../rosetta/fig/rosetta1_sm.jpg)
The Rosetta
spacecraft, with LAP probes mounted at the tips of the two solid booms
and the large (32 m wing span) solar panels clearly visible.
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