A methodology for real time fault detection, isolation andcorrection

Mission critical timelines and availability requirements of large, complex ground stations demand some form of a distributed real-time system with an embedded rule-based expert advisor for recognizing and responding to changes within the system. The failure management optimization support system (FMOSS), which develops unique sets of status values, is discussed. The live status returned from the segment hardware forms a set of values, or signature vector, for each equipment string. The signature vector is compared to the signature that occurs when the equipment string is operational. If the processed status signatures do not match the signature that indicates the equipment string is operational, the expert advisor notifies the command center that a fault has been detected. The expert advisor continues processing until it has found a match from the pool of preengineered failure-mode signature vectors. Based on the match, Boolean logic is used to perform fault isolation and correction, with results provided to the command center     

Intersatellite laser crosslinks

Intersatellite laser crosslinks (ISL) provide a method of communication that has significantly increased the data throughput that can be managed over typical RF communication systems, and has significant growth potential. Optical communications offer very wide bandwidths which can be effectively utilized with wavelength division multiplexing techniques. The data rate growth potential is well beyond the few gigabit per second range of RF technology. The use of lasers in transmitting optical data takes advantage of its small wavelength and low beam divergence to send highly directed signals over significant distances with controlled losses in intensity. The high directivity of the laser aids in resistance to jamming communications between satellites, or between satellites and ground stations. Various intersatellite laser optical crosslink system are discussed including the Massachusetts Institute of Technology's Laser Intersatellite Transmission Experiment (LITE), the McDonnell Douglas Electronic Systems Company Laser Crosslink System, and The Ball Aerospace Optical Intersatellite Link,in order to display the various subsystem and their implementations. Link budget calculations are performed on the most commonly used modulation formats to determine system parameters necessary to close the crosslink. Background is provided on primal system architectures and methods of laser communication, as well as presently implemented systems. The authors provide some insights on where ISL systems have opportunity to increase their data throughput and reduce acquisition time     

First spatio-temporal results from the LDEF interplanetary dust experiment

The LDEF Interplanetary Dust Experiment was unique in providing a time history of impacts of micron-sized particles on six orthogonal faces of the vehicle over a span of nearly a full year. Over 15000 hits were recorded, representing a mix of zodiacal dust, meteor stream grains, orbital debris, perhaps beta-meteoroids, and possibly interstellar matter. Although the total number was higher than predicted, the relative panel activity distribution was near expectations. Detailed deconvolution of the impact record with orbital data is underway, to examine each of these populations. Very preliminary results of the fairly crude “first look” analysis suggest that debris is the major particle component at 500 km. The data show clear evidence of some known meteor streams as sharp, tightly-focused events, unlike their visible counterparts. Some apparent debris events show similar signatures. Data from the leading and trailing edges suggest a detection of beta-meteoroids, but the analysis is not yet conclusive. Absolute fluxes and flux ratios are not yet known, since the detector status analysis is yet incomplete.     

Stereographic Projection in the National Airspace System

Consideration is given to the calculation of stereographic representations of airborne targets from observations of slant range, azimuth, amd altitude in a multiple radar tracking system. Emphasis is placed upon the translation of the accuracy of the surveillance information into the stereographic plane. Applications include air traffic control operations in which calculations must be performed repeatedly in real time for numerous targets without overtaxing available computational resources.     

Approximation of Corrected Slant Range in a Radar Surveillance System

Consideration is given to numerical procedures for evaluating the corrected slant range in a radar surveillance system. Applications include air traffic control operations in which such calculations must be performed repeatedly in real time for a multitude of targets without overtaxing available computational resources.     

Low cost satellite ground control facility design

A design approach common to the areas of satellite operations command and control, tracking, subsystem analysis, system planning and scheduling, orbit determination and maintenance, and data routing and control is discussed. Specific satellite mission applications and operations are isolated from the remainder of the design to allow application to a broad variety of satellite systems. Discussions of specific satellite missions are limited to the context of understanding the general magnitude and scope of what a ground control facility is required to support. By isolating the common satellite operational functions, a low cost generic approach that allows for phased implementation of system changes with minimal impact to on-orbit assets and mission performance is developed. The goals of this approach are to provide the capability for growth, maintainability, and operability of the satellite system. A brief discussion of satellite systems followed by the introduction of the general function of any satellite control facility sets the stage for the overall design approach. The factors that define the design along with the key design features are presented, with a discussion of each product available in each functional area     

Spacecraft telemetry link performance in a transfer orbit

There are several critical periods early in the mission of a geo-stationary communication satellite. The first is the period from launch vehicle ignition until the upper stage final successful burn. The second is after the above span until the vehicle reaches its final altitude of a synchronous orbit. For a nominal low thrust apogee boost ascent subsystem during that later time, almost continuous telemetry is mandatory. This is especially true during the crucial periods of main engine burns and attitude correction phases. Maintaining a strong telemetry link throughout this phase requires an adequate RF signal link from the spacecraft to a ground station in the telemetry RF channel. An analysis of this link performance during each orbit until final position has two major aspects. One, the location of the spacecraft in relation to the ground tracking station at each moment in the mission is a matter of geometry and Keplerian physics. The other is the RF signal and its supporting subsystems, both on the ground and aboard the vehicle. The fundamental theoretical considerations or both the orbit parameters and radio link components are examined and then the individual parameter sensitivities are analyzed. Next, a nominal cast for a generic mission is studied. This survey considers the telemetry performance during each major stage of the flight from the launch through the transfer orbit to the postinjection period to the final orbit. Then abnormal situations due to both orbit and RF faults are examined. Finally, some design and operation concepts which may lessen the impact of the previous anomalies, are presented     

A Space Debris Primer for Astronomers

In this journal, 'space debris' usually carries implications of aerospace activities, but it was not always thus. Humankind has been concerned with sky debris (often not knowing it was that) since eyes were turned skyward. Before space exploration began, astronomers specialized in comet tails, asteroids, meteorites, aurorae and zodiacal light. It was inevitable that they stay near the forefront of the new space technologies, even before Explorer I explained the aurorae. Now, the emphasis is on manmade debris, for the simple reason that an astronomical experiment proved that to be the preponderant component of the total debris environment. We present here a review survey of the total near-Earth debris complex, artificial and cosmic. Our goal is three-fold: (1) To detail to both astronomers and spaceflight specialists the long and heavy astronomical activity, (2) to give an overview of what has been and is being done, and (3) to suggest some possible directions for the future.