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Roussel-Dupre, Diane

Publications and source records attributed to Roussel-Dupre, Diane.

Constellation Study for Optimized Target Access and Coverage

We have performed a low earth orbiting satellite constellation design parameter space study to determine optimized constellations that satisfies mission goals while minimizing total system costs. Because this is a generic study, we developed a generalized set of mission requirements that would meet the needs of several different types of space missions. Figure of merit parameters were defined to help rank the different constellations under study. Instead of performing a full, multi-dimensional parameter space study, we instead focused on a few exemplar cases. For this generic mission, the baseline requirements were as follows: altitude: 700km, total number of satellites per constellation: 40-100, world coverage: 100% coverage or maximize coverage of populated latitudes, polar coverage: some but not 100% required, multi-ball observations: 2- & 3-ball coverage desired, and target coverage: full coverage or up to 5 minute observing gap for 1-ball coverage at all latitudes. For added conservatism, the minimum target observing elevation angle was 10-degrees and the minimum acceptable time on target was 1 minute. We also only performed the calculations for a Walker constellation (defined as M/M/IP or #planes/# satellites per plane/interplane satellite spacing) instead of “streets-of-coverage” constellations, which at high inclinations can satisfy coverage requirements with slightly fewer satellites.

47 OTHER INSTRUMENTATION↗

Recurrence times and periodicities in 4U 1608-52 as observed by Vela 5B

We report on the Vela 5B 10 year history of the soft X-ray transient 4U 1608-52, and on the characteristics of its soft X-ray outbursts. The Vela 5B satellite observed the four known outbursts in 1975, 1977, and 1979, and four new outbursts in 1970 and 1971, altering the recurrence pattern of outbursts from this source. One of the 1970 outbursts is symmetric in its intensity profile, while the two outbursts in 1971 have short exponential profiles separated by 80 days. Despite suggestive recurrence periods of approximately 85 and approximately 150 days evident in the time intervals between the outbursts, there is no single statistically significant recurrence time on which the outbursts recur consistently. In the 1970 symmetric event, there is evidence for a period of either 4.10 or 5.19 days. Drawing upon the analogy with SU Ursa Majoris dwarf novae, we suggest that the short period is orbital and any longer period would be associated with a precession period of the accretion disk.

Lochner, James C.↗

High-resolution Elemental Mapping of the Lunar Surface

New instruments and missions are being proposed to study the lunar surface as a result of the resurgence of interest in returning to the Moon. One instrument recently proposed is similar in concept to the x-ray fluorescence detectors flown on Apollo, but utilizes fluorescence from the L- and M-shells rather than the K-shell. This soft X-Ray Flourescence Imager (XRFI) is discussed.

Edwards, Bradley C.↗

The high-energy transient experiment (HETE) - An international multiwavelength mission

The High Energy Transient Experiment (HETE), an international mission scheduled by NASA for launch on a Pegasus rocket in July 1994, is described. The prime objective of HETE is to carry out the first multiwavelength study of gamma-ray bursts with UV, X-ray, and gamma-ray instruments mounted on a single, compact spacecraft. A unique feature of the HETE mission is its capability to localize GRBs with about 10 arc second accuracy, in near real time aboard the spacecraft, and to transmit these positions directly to a network of receivers at existing ground-based observatories, enabling rapid, sensitive follow-up studies in the radio, IR, and optical bands.

Ricker, George R.↗