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Astronomy and Astrophysics for the 1980's, Volume 2: Reports of the Panels (1983)
Commission on Physical Sciences, Mathematics, and Applications (CPSMA)

Page
329
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Page
329
Front Matter (R1-R22)
1. High-Energy Astrophysics I. Introduction (1-1)
II. The Nature of High-Energy Astronomy and the Scope of the Report (2-8)
III. Summary of Principal Recommendations (9-11)
IV. X-Ray Astronomy (12-37)
V. Extreme-Ultraviolet Astronomy (38-42)
VI. Gamma-Ray Astronomy (43-54)
VII. Cosmic-Ray Astronomy (55-68)
VIII. High-Energy Solar Astronomy (69-83)
IX. Neutrino Astronomy (84-89)
X. Gravitational-Wave Astronomy (90-97)
2. Ultraviolet, Optical, and Infrared Astronomy I. Summary and Recommendations (98-102)
II. Highlights of Astronomy in the 1970 (103-118)
III. Science Opportunities in the 1980 (119-134)
IV. Detailed Descriptions of the UVOIR Program for the 1980 (135-177)
V. Projections into the Future (178-187)
VI. Epilogue (188-188)
Appendix 2.A: Telescopes for UVOIR (189-196)
Appendix 2.B: Focal-Plane Instrumentation and Detectors (197-210)
3. Radio Astronomy I. Introduction: Scope of the Report (211-211)
II. Summary of Recommendations (212-213)
III. Description of Recommended Projects and Facilities (214-228)
IV. Scientific Priorities (229-257)
V. Reference to List of Radio and Radar Astronomy Observatories (258-258)
4. Theoretical and Laboratory Astrophysics I. Introduction and Summary of Recommendations (259-261)
II. Theoretical Astrophysics (262-285)
III. Laboratory Astrophysics (286-301)
5. Data Processing and Computational Facilities I. Introduction (302-304)
II. Conclusions and Recommendations (305-306)
III. The Trend Toward Decentralization (307-308)
IV. Theoretical Computing (309-314)
V. Image Processing and Analysis (315-323)
VI. Data Archiving (324-325)
VII. Astronomical Databases (326-326)
VIII. Telecommunications (327-328)
IX. Specialized Architectures (329-329)
Appendix 5.A: The Canonical System (330-333)
6. Organization, Education, and Personnel I. Summary and Recommendations (334-337)
II. Maintenance of Scientific Talent (338-349)
III. Other Issues in the Practice of Astronomy (350-360)
IV. Astronomy and the Astronomers in the 1970's (361-413)
Appendix 6.A (414-438)
Appendix A: Abbreviations Used in Text (439-442)

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329 used cleverly with carefully planned observing programs, is probably adequate for both applications, although high- bandwidth lines are extremely desirable. With a 56-kbps line, it may prove cost-effective to operate telescopes from remote locations in some cases. For example, the University of California is investigating the possibility of operating a proposed 10-m telescope, located on Mauna Kea, from a control center in California. If remote operation saves only a few round trips per month between Hawaii and California, a net cost savings will be achieved. In the case of the second application, the Panel believes that an observatory operating its tele- scopes with remote observer participation must take responsibility for the terminal at the observer's end of the data link. The costs of such a scheme would there- fore be substantially greater than the costs of the communication service alone and will probably prohibit the implementation of this concept in the 1980's. I X. SPECIALI ZED ARCHITECTURES The Panel investigated the possibility that specialized computer architectures might lead to dramatic improve- ments in astronomical computing. For example, one might imagine a cubical n X n X n array of microprocessors, each able to transfer data to and from its six nearest neighbors and all synchronized by a master oscillator. Such an array would seem to be ideal for some kinds of hydrodynamical calculations and would reduce the computa- tion time by a factor of n3 since n3 operations are performed in parallel. If the top and bottom, left and right, and front and back sides of the array were con- nected, the architecture could be adapted to N-body calculations with n3 particles (one per processor). There are, in fact, several specialized architectures being investigated and/or implemented. NASA/Goddard Space Flight Center is developing the Massively Parallel Proces- sor (MPP), which will contain a 128 X 128 array of proces- sors, each connected to its nearest neighbors on the top, bottom, left, and right. Each processor will be capable of performing only simple functions. The MPP is intended to be used for pipeline processing of Landsat images. It is an interesting development in that the physics of the problem is embodied in the computer architecture. NASA/Ames is developing a specialized computer to be used in hydrodynamic calculations. The emphasis here is

Representative terms from entire chapter:

specialized computer