Bibcode
Cibils, R. M.; Busto, A.; Gonella, J. L.; Martinez, R.; Chielens, A. J.; Otero, J. M.; Nuñez, M.; Tropea, S. E.
Bibliographical reference
SPACE TECHNOLOGY AND APPLICATIONS INTERNATIONAL FORUM-STAIF 2008: 12th Conference on Thermophysics Applications in Microgravity; 1st Symposium on Space Resource Utilization; 25th Symposium on Space Nuclear Power and Propulsion; 6th Conference on Human/Robotic Technology and the Vision for Space Exploration; 6th Symposium on Space Colonization; 5th Symposium on New Frontiers and Future Concept. AIP Conference Proceedings, Volume 969, pp. 316-325 (2008).
Advertised on:
1
2008
Citations
2
Refereed citations
2
Description
The use of classical techniques for neutron flux measurements in nuclear
reactors involves the switching between several detection chains as the
power grows up to 10 decades. In space applications where mass and size
constraints are of key significance, such volume of hardware represents
a clear disadvantage. Instead of requiring different instruments for
each reactor operating range (start-up, ramping-up, and nominal power),
a single instrument chain should be desirable. A Wide Range Neutron
Detector (WRND) system, combining a classic pulse Counting Channel with
a Campbell's theorem based Fluctuation Channel can be implemented for
the monitoring and control of a space nuclear reactor. Such an
instrument will allow for a reduction in the complexity of space-based
nuclear instrumentation and control systems. In this presentation we
will discuss the criteria and tradeoffs involved in the development of
such a system. We will focus particularly on the characteristics of the
System On Chip (SOC) and the DSP board used to implement this
instrument.