The helium spectrum from 0.1 to 100 GeV/nucleon was measured by the Alpha M
agnetic Spectrometer (AMS) during space shuttle flight STS-91 at altitudes
near 380 km. Above the geomagnetic cutoff the spectrum is parameterized by
a power law. Below the geomagnetic cutoff a second helium spectrum was obse
rved. In the second helium spectra over the energy range 0.1 to 1.2 GeV/nuc
leon the flux was measured to be (6.3 +/- 0.9) x 10(-3) (m(2) sec sr)(-1) a
nd more than ninety percent of the helium was determined to be He-3 (at the
90% CL). Tracing helium from the second spectrum shows that about half of
the 3He travel for an extended period of time in the geomagnetic field and
that they originate from restricted geographic regions similar to protons a
nd positrons. (C) 2000 Published by Elsevier Science B.V.