April-June 1996, Volume 17, Number 2


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Midcourse Space Experiment: Technology

   Midcourse Space Experiment: Guest Editor's Introduction
   M. R. Peterson

   The MSX Tracking, Attitude, and UVISI Processors
   L. J. Frank, C. B. Hersman, S. P. Williams, and R. F. Conde

   The MSX Command and Data Handling System
   D. D. Stott, R. K. Burek, P. Eisenreich, J. E. Kroutil, P. D. Schwartz, and G. F. Sweitzer

   MSX Attitude Determination and Control Hardware
   F. F. Mobley, W. E. Radford, and L. R. Kennedy

   A Testbed for the MSX Attitude and Tracking Processors
   D. S. Wilson

   MSX Ground Operations
   J. F. Smola, M. H. Barbagallo, J. H. Cranmer, C. C. DeBoy, M. J. Harold, J. A. Krein, H. M. Kreitz, Jr., A. C. Sadilek, and H. K. Utterback

   The MSX Performance Assurance Program
   M. E. Goss

   The UVISI Instrument
   K. J. Heffernan, J. E. Heiss, J. D. Boldt, E. H. Darlington, K. Peacock, T. J. Harris, and M. J. Mayr

   The Spatial Infrared Imaging Telescope III
   B. Y. Bartschi, D. E. Morse, and T. L. Woolston

   The Space-Based Visible Sensor
   D. C. Harrison and J. C. Chow

   Technology Demonstration by the Onboard Signal and Data Processor
   C. G. Pfeiffer and B. L. Masson

   MSX Reference Objects
   S. V. Burdick, J. Chalupa, C. L. Hamilton, T. L. Murdock, and R. Russell



   Publications, Presentations, and Colloquia --Patents

The cover: Designers of future operational space- and ground-based surveillance and tracking systems require simultaneous wideband optical data on midcourse missile flight, as well as space background phenomena. The precision Midcourse Space Experiment (MSX) platform will collect such data over a wide wavelength range during its long-duration mission, building on previous short-term Ballistic Missile Defense Organization tests. During the "cryogen" phase, MSX experiments will provide critical first-time observations of missile target signatures against Earth-limb, auroral, and celestial-cluttered backgrounds. The "post-cryogen" phase will focus on celestial and terrestrial backgrounds, surveillance demonstrations, and environmental research. Contamination information will be gathered during all phases to aid the future design of spacecraft carrying optical instruments. (Cover illustration by Kenneth R. Moscati.)

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© 1996 by The Johns Hopkins University Applied Physics Laboratory

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