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Intranet
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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
suggestions / Examensarbeten (30 hp)
Suggestions for
Rosetta student projects
Student: you,
perhaps?
Supervisor: Anders Eriksson
Background
We fly a kind of
"space weather station" known as a Langmuir
probe (LAP) on ESA's
Rosetta spacecraft, launched in 2004 for arrival at comet
Churyomov-Gerasimenko in 2014. Some of our goals are to
understand the plasma processes around the comet, and to link the
nucleus properties to the plasma environment. Though there are several
year before we reach the comet, there are data to analyze, science to
understand and planning to do. We have gathered data during flybys of
the Earth (2005, 2007 and 2009), Mars (2007), the asteroids Steins (2008)
and Lutetia (2010) and at a
few other instances. But what we really look forward to of course is the
comet!
We are one of
the core teams in the international collaboration known
as the Rosetta Plasma Consortium (RPC), the other teams being located
in in
Braunschweig, Kiruna, London, Orléans, and San Antonio. Projects can
therefore sometimes include a visit at one of these places, for anything
from a week to several months, depending on circumstances and what you
want.
Project suggestions
Details of the project will depend on
your interests and skills, and on what is suitable at the time you turn
up. Here are a few possibility sketches, to set ideas in motion. Do you
have any own ideas for what to do? Come and discuss them!
- Comet plasma model. A
research team organized by the International Space Science Institute in
Bern have compiled a joint comet model, from the nucleus to the coma,
which is available for testing. This is of high interest to us, as it
offers a tool for operations planning and a baseline expectation for
what we can see. A first project on this
was done in 2009, but since
then there as been new simulations and a very much altered trajectory
strategy, so further work is needed. This means numerically flying
Rosetta through the comet environment model and see
what we can expect our measurements
to look like, to find out what measurement modes that may be most useful.
- Flyby data. More can be
done on our data from the Earth, Mars and asteroid flybys, particularly
on the science side. Our data can be compared to other spacecraft data
and to ground observations, to find out the physics in the solar wind
and magnetosphere. The work would could partly be done at one of our
RPC partners.
Contact
Anders.Eriksson@irfu.se
![[Rosetta]](http://www.space.irfu.se/rosetta/ros_lap.gif)
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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