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AMS,
the Alpha Magnetic Spectrometer,
is a space borne experiment scheduled for a three years
mission on the International
Space Station. It is designed to study:
- the presence
or absence of antimatter in distant galaxies through
the detection of cosmic anti-nuclei as anti-Helium
and anti-Carbon.
- the origin and
structure of dark matter which is believed to make
up 90% of the known universe
- the origin
and the composition of charged cosmic rays as well
as other phenomena which may exist in nature which
we have not yet imagined or had the tools to discover
The same technology
used for research in particle physics is adapted in
AMS for space application.
The charge sign and magnetic rigidity of cosmic rays
will be determined by the deflection of their trajectory
in the magnetic field of the instrument, while an array
of precision particle detectors will perform redundant
measurements of charge magnitude, velocity and energy.
With an acceptance of 0.7m2sr, AMS will be
one of a kind detector operating in space.
The operation principles
of the apparatus have been tested in the space environment
during a precursor flight of the experiment , 10 days
of successful data taking onboard of the shuttle DISCOVERY
in June 1998. A limit of 10E-6 on the ratio
as well as accurate measurements of proton, helium,
lepton and deuteron energy spectra are among the physics
results already published from the analysis of the data
taken during the precursor flight.
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AMS Collaboration |
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AMS 01
the Detector |
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AMS 01 the Shuttle flight |
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AMS 02 the Physics goals |
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AMS 02 the Detector |
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