FOREWORD
Advancements in physics are based on the close interplay between experiment and theory.
Advancements in theory are based on the ability of theorists to explain existing experimental
results and to predict new phenomena to be confirmed by experiments. Revolutions in physics
occur when an experimental result contradicts the theoretical prediction which leads to the creation
of new theory.
There is no theory that can disprove an experimental result, whereas a theory, however logical
and elegant, cannot be valid if it does not conform to experimental observations. Careful
experimentation in physics, such as the discovery of the J particle, the
observation of CP violation in K decay, and the discovery of high temperature superconductors have
opened up new fields of research in physics. These observations were carried out by experiments even
though there was no a priori theoretical interest.
There are two kinds of particles traveling through space: neutral (light rays and neutrinos) and
charged particles.
Over the last fifty years there have been many fundamental discoveries in astrophysics from the
measurement of photons including the discovery of pulsars, microwave background radiation, binary
pulsars, and gamma ray bursts. These discoveries have fundamentally improved our knowledge in
physics and astronomy. In recent years, the addition of the ROSAT, AXAF (Advanced X-ray Astrophysics
Facility) satellites and the Hubble telescope further enrich our knowledge. The beautiful underground
experiments at Gran Sasso (MACRO, KAMIOKANDE and others) have provided us with profound insight
on cosmic neutrino physics.
However, there has never been a sensitive measurement of charged cosmic rays. This is because
charged particles are absorbed by the earth's atmosphere and therefore they cannot be measured
easily on the ground. In addition the charge of cosmic rays can only be identified by their trajectory in the
magnetic field. Up to now there has never been a magnetic detector in space.
The Space Station provides unique support for the power, weight and infrastructure required for
many precision and long duration experiments. AMS is the first example of a physics experiment on
the International Space Station. The purpose of the Alpha Magnetic Spectrometer (AMS) Experiment is
to utilize the knowledge and technology learned in particle physics to measure and to identify charged
particles as well as very high energy gamma rays to explore new unknown phenomena. This experiment
is being carried out by 200 scientists from 12 nations.
In addition to its pure physics goals, this experiment shows that science indeed has no frontiers and
scientists from different social and political backgrounds can work together.
The construction of this experiment was made possible through the strong support of NASA, the
U.S. Department of Energy (DOE) and the unique contributions of the following individuals: H. Hofer
who chairs our AMS Science Board, M. Bourquin and K. Lubelsmeyer who co-chair our AMS
International Board, R. Battiston and Y. Galaktionov who co-chair our Astrophysics Board as well as
U. Becker, J. Burger, G. Viertel and M. Capell who oversaw the detector integration. R. Sagdeev and
J. Trumper shared with us much valuable insight and experience in doing experiments in space.
A. de Rujula, J. Ellis, S. Glashow and A. Guth shared with us much of their insight on the current
theoretical understanding of astrophysics.
This brochure is intended to provide a description of this experiment in terms of science, technology
and international collaboration. I would like to take this this occasion to express on behalf of the
AMS Collaboration our appreciation to NASA and the many government leaders and agencies worldwide
whose strong support have made this experiment possible. I also want to thank the AMS
Administration and Communication Group for putting the brochure together.
Samuel C.C. Ting
![[I.S.S. ALPHA]](tumbfot2.jpg)
INTERNATIONAL SPACE STATION:Assembly Complete
The position of the AMS detector is shown. The ISS program involves the partecipation of 15
cooperating countries: the United States, Canada, Japan, Russia and 11 nations of the
European Space Agency (ESA).(NASA)