The proton spectrum in the kinetic energy range 0.1 to 200 GeV was measured
by the Alpha Magnetic Spectrometer (AMS) during space shuttle flight STS-9
1 at an altitude of 380 km. Above the geomagnetic cutoff the observed spect
rum is parameterized by a power law. Below the geomagnetic cutoff a substan
tial second spectrum was observed concentrated at equatorial latitudes with
a flux similar to 70m(-2) s(-1) sr(-1). Most of these second spectrum prot
ons follow a complicated trajectory and originate from a restricted geograp
hic region. (C) 2000 Published by Elsevier Science B.V. All rights reserved
.