Particle environment surrounding the Midcourse Space Experiment spacecraft

Particle occurrence rates, velocities, size distributions, and trends in the environment have been measured above the Midcourse Space Experiment spacecraft using optical sensors. Results from the spacecraft's first 11 months on orbit are presented. Particles were detected both in association wi...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:Journal of spacecraft and rockets 1999-07, Vol.36 (4), p.561-565
Hauptverfasser: Galica, Gary E, Green, B. David, Boies, Mark T, Uy, O. Manuel, Silver, David M, Benson, Richard C, Erlandson, Robert E, Wood, Bob E, Hall, David F
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
Beschreibung
Zusammenfassung:Particle occurrence rates, velocities, size distributions, and trends in the environment have been measured above the Midcourse Space Experiment spacecraft using optical sensors. Results from the spacecraft's first 11 months on orbit are presented. Particles were detected both in association with known particle-generating activities and during comparatively quiescent times. In general, the optical environment is quite benign. The on-orbit environment appears to be dominated by particles remaining from ground-processing operations. That environment is consistent with prelaunch cleanliness level measurements. Particulates were detected during quiescent periods as the spacecraft passed through the terminator from eclipse into daylight. Particle evolution occurs within minutes of solar heating onset. At Midcourse Space Experiment altitudes, drag effects are not significant until comparatively long times (10 exp 3 to 10 exp 4 s); therefore, the observed velocities of the near-field particles, in the 1- to 10-cm/s range, are representative of the surface release velocity. The particles are observed in the 1- to 100-micron-size range. The size distribution scales approximately as r exp -1.5 down to the sensitivity limit. (Author)
ISSN:0022-4650
1533-6794
DOI:10.2514/3.27200