
The Solar System Physics and Space Technology
(SSPT) research program at the
Swedish Institute of Space Physics (IRF) in Kiruna is
devoted to
Comparative research on the evolution and dynamics of the solar
system objects (planets, asteroids, comets, meteoroids) and their interaction
with the solar wind.
We design and build instruments for space missions, analyze received
data and develop computer models simulating planetary environments. Traditionally,
the main focus of the group is experimental physics. We manufacture ion
mass spectrometers, electron spectrometers, energetic particle detectors,
and energetic neutral atom (ENA) imagers to study Mercury, Venus, Earth, Mars,
and comets. We use the state-of-the-art parallel computers (
HPC2N) to run our numerical
models. Beside space missions, we use the ground-based radars (
EISCAT) to investigate
distribution and characteristics of the interplanetary dust and meteoroids.
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Last update 29 May 2010
by Shahab Fatemi