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Search indexed NASA NTRS and DOE OSTI research on propulsion, heat transfer, battery materials and energy systems. Follow report and document links to the original sources.
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Improved magnetic components for static inverters and converters - magnetic and physical properties of magnetic materials, conductors and insulation, and screening magnetic tests
Magnetic components and static inverters and converters - sine current screening and sine flux screening core tests on test program materials
This standard analysis report provides the estimates for the chemical (oxyanions and complexing agents) and cement components with a data collection cut-off date of December 31, 2023. These estimates will be included in a Performance Assessment Inventory Report developed for the U.S. Department of Energy (DOE) performance assessment (PA) for the 2026 Compliance Recertification Application (CRA).
This report documents the verification of RESRAD-OFFSITE Version 4.0 and describes, where necessary, the verification of the following: • The data comprising the standard dose and risk coefficient libraries in the RESRAD database files Master_dcf_ICRP07.mdb and Master_dcf_2k.mdb. • The extraction and transfer of the data from the selected database file to the computational code by the RESRAD-OFFSITE 4.0 interface, ResOWin.exe. • The different processes that are modeled by the main computational code in RESRAD OFFSITE 4.0, ResOMain.exe. • The data displayed in the graphical and text reports. Many verifications were performed as part of the quality assurance quality control program associated with the development and release of RESRAD-OFFSITE 4.0, namely: • developer testing, • internal independent testing, and • release testing. Some were also performed in response to questions from users regarding the performance of the code. The main text of the report focuses on summarizing a subset of those tests, both independent and developer tests that verified the computations performed by the code. The verifications included in this report served as the basis for the development of the release tests of the computational executables and provided the quantitative results to be compared with the code output. The input and output interfaces and the data transfers between the various executables of the code were tested while performing the verification testing. They were tested intentionally during release testing. This report also provides some basic information to help in understanding the activities that were verified. The report: • outlines the components of RESRAD-OFFSITE 4.0 and the interconnections between these components, • outlines the processes modeled by the computational code, • provides summary figures and tables to offer confirmation of the verification of the computational components of the code, • reproduces the verifiers’ reports, if available, in individual appendices, • refers to the previous verification report (Yu et al. 2011) for more details about some of the verifications, and • reproduces the test cases and the testers’ reports from the release testing in individual appendices, when possible.
Electronic component testing of high-shock FM TRANSMITTERS
Operation and components of density probe high voltage pulse generator, manipulator control, and pressure transducers used for flow visualization
Motion picture report of IMP-1 magnetometer observations of interplanetary magnetic field
Vacuum jacketed components on launch umbilical tower service arms at Launch Complex 39 - burst discs
Vacuum jacketed components on launch umbilical tower service arms at Launch Complex 39 - vacuum seal valves
Vacuum jacketed components on launch umbilical tower service arms at Launch Complex 39 - hose flexure lines
Vacuum jacketed components on launch umbilical tower service arms at Launch Complex 39 - repair techniques for carbon dioxide and vacuum jacketed transfer lines
Vacuum jacketed components on launch umbilical tower service arms at Launch Complex 39 - low heat cryogenic rotary joint
Vacuum jacketed components on launch umbilical tower service arms at Launch Complex 39 - vacuum probes
Vacuum jacketed components on launch umbilical tower service arms at Launch Complex 39 - central vacuum pulldown system
Vacuum jacketed components on launch umbilical tower service arms at Launch Complex 39 - bayonet joints in cryogenic propellant and vent lines
The paper reports on a synthesis of the silicate mineralogy of a planetary basalt suite, which concerns itself only with specific aspects of pyroxene cation substitutional couples. Consideration is given to the mineral chemistry and the basalt suites in an overview fashion. Attention is given to those characteristics of pyroxene chemistry that reflect planetary constraints on the host basalts from which the pyroxenes crystallized. It is concluded that the inspection of a large number of high quality silicate analyses of pyroxenes demonstrates conclusively that these phases carry a signature of the planetary body in which they evolved. In addition, it is noted that there are planetary probes capable of constraining thermodynamic parameters that were obtained during the petrogenesis of their host basaltic liquids
This annual report summarizes the work completed during the third year of technical effort on the referenced contract. Principal developments continue to focus on the Probabilistic Finite Element Method (PFEM) which has been under development for three years. Essentially all of the linear capabilities within the PFEM code are in place. Major progress in the application or verifications phase was achieved. An EXPERT module architecture was designed and partially implemented. EXPERT is a user interface module which incorporates an expert system shell for the implementation of a rule-based interface utilizing the experience and expertise of the user community. The Fast Probability Integration (FPI) Algorithm continues to demonstrate outstanding performance characteristics for the integration of probability density functions for multiple variables. Additionally, an enhanced Monte Carlo simulation algorithm was developed and demonstrated for a variety of numerical strategies.
The emission components of spiral galaxies between 12 microns and 90 cm are identified. Additionally, an attempt to understand the relationships between them was made. The specific goal was to gain some understanding on the nature of the radio-infrared correlation. The results are summarized.