Detecting the dynamical state of the atmosphere from the orbital decay of the ODERACS spheres

Autor: G.D. Badhwar, A. Tan
Rok vydání: 1997
Předmět:
Zdroj: Journal of Atmospheric and Solar-Terrestrial Physics. 59:431-437
ISSN: 1364-6826
DOI: 10.1016/s1364-6826(96)00020-x
Popis: The orbital decay curve of a satellite having constant cross-sectional area and in circular orbit can furnish valuable information regarding the dynamical state of the atmosphere. It is shown that a rectilinear decay curve having constant downward slope (zero curvature) should indicate that the atmosphere was undergoing compression during that period. A decay curve having concavity upwards (positive curvature) will strongly indicate that the atmosphere was in a contracting phase. A decay curve with downward concavity (negative curvature) may indicate an expanding, a stable or a contracting atmosphere. This theory, when applied to the orbital decay of the Orbital Debris Radar Calibration Spheres (ODERACS) satellites, indicates that, during the period from Day 90 through Day 240 in the year 1994, the atmosphere was very definitely in a compression mode. During this period, ODERACS Sphere 1 faced nearly constant densities while Sphere 6 actually encountered progressively smaller air densities as they descended. The atmospheric scale height as calculated from the orbital data of Spheres 1 and 6 diminished steadily during the same period. It is shown that Spheres 1 and 6 descended faster and slower, respectively, than the level of constant air density equal to 5 × 10−2kg/m3. During a brief period from Day 240 through Day 290, the atmosphere reversed to a strongly expanding mode. Thereafter, the atmosphere reverted back to a compression mode from Day 290 through Day 390, 1994–1995. The measured F10.7 solar flux at Penticton, British Columbia, generally supports the findings of this study.
Databáze: OpenAIRE