The orbital decay of a low-Earth-orbit satellite having constant cross-sect
ional area in a near-circular orbit can furnish valuable information regard
ing the dynamical conditions of the atmosphere. The slope of the orbital de
cay curve gives the atmospheric density, whereas the curvature of the decay
curve can indicate the expansion, stability or contraction of the: atmosph
ere. The state of the atmosphere in 1994 was determined from the orbital de
cay of the ODERACS I spheres by employing this technique. The state of the
atmosphere in 1995 was determined from the orbital decay of the ODERACS II
spheres and reported in this study. From days 40-215, 1995, the atmosphere
was in a prolonged compression mode. During this period, ODERACS II Sphere
3 encountered progressively smaller densities as the density scale height d
iminished steadily. This was followed by a period of relatively stable atmo
sphere. During a brief period from days 280-300, the atmosphere was in a st
rong expansion mode. which was followed by another compression mode until d
ay 360. The results show great parallels between the atmospheric conditions
in 1994 and 1995, including clear indications of the semi-annual variation
. The atmosphere in 1995 was under greater compression than in 1994, consis
tent with the phase of the sunspot cycle. However, the rate of atmospheric
contraction was greater in 1994 than in 1995 in contrast to predicted model
s. The observed 10.7 cm solar fluxes at Penticton, British Columbia, strong
ly support the findings of this study. (C) 1998 Elsevier Science Ltd. All r
ights reserved.