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NASA Scientific and Technical Aerospace Reports

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component of gamma spectra resulting from radiative capture of fast nucleons; i.e., the part of the spectrum that is not<br />

amenable to st<strong>and</strong>ard statistical model (Hauser-Feshbach) treatments. We describe recent results on the extension of the DSD<br />

model to unbound final states, including comparison with proton <strong>and</strong> neutron capture data. The importance of including<br />

convective-current magnetic radiation to explain proton capture angular distributions in the 30 MeV region is shown. We<br />

conclude with a brief discussion of a model closely related to the DSD, the pure-resonance model.<br />

NTIS<br />

Gamma Ray Spectra; Nucleons<br />

74<br />

OPTICS<br />

Includes light phenomena <strong>and</strong> the theory of optical devices; for specific optical devices see also 35 Instrumentation <strong>and</strong> Photography.<br />

For lasers see 36 Lasers <strong>and</strong> Masers.<br />

20040046893 Smithsonian Astrophysical Observatory, Cambridge, MA, USA<br />

Spectroscopic Determination of the Physical Conditions in Hot Optically Thin Sources<br />

Oliversen, Ronald J., <strong>Technical</strong> Monitor; Brickhouse, Nancy; March 2004; 7 pp.; In English<br />

Contract(s)/Grant(s): NAG5-3559; No Copyright; Avail: CASI; A02, Hardcopy<br />

Astrophysical Plasma Emission Database - APED consists of atomic data, primarily theoretical, needed to calculate X-ray<br />

through optical emission spectra of hot thermal plasmas. These data are supplemented by experimental values, such as<br />

laboratory plasma wave- lengths, <strong>and</strong> are validated by experiment only rarely. Thus the comparison of predicted spectra to<br />

astrophysical spectra serves as invaluable feedback on the quality of the models. Following up on unfavorable comparisons,<br />

we have communicated atomic data needs to atomic theorists <strong>and</strong> experimental plasma physicists so that improvements can<br />

be made to the database. The database is now reasonably complete from approx. 1 to 30 A, <strong>and</strong> from - 90 to 180 A, with<br />

significant gaps remaining in the range 30 to 90 A. Astrophysical Plasma Emission Code - APEC uses the APED data as inputs<br />

<strong>and</strong> computes level populations <strong>and</strong> line emissivities using a rate matrix solver. Tabulated models for a fine grid of<br />

temperatures <strong>and</strong> densities can be applied to observational data. The current public version of APEC output uses an input<br />

ionization balance model, assuming CIE; however, we have a working version to calculate the ionization state of the gas. We<br />

will begin testing non-equilibrium ionization (NEI) models over the next year - we are now finalizing the atomic database<br />

needed to perform the ionization state calculations. At that time, the code will be made public. We have developed optimized<br />

error codes, additional testing protocols <strong>and</strong> substantial documentation, in preparation for this public release. Secondarily, we<br />

have begun to investigate the use of APED <strong>and</strong> APEC for X-ray photoionized plasma, beginning with opacity modeling (e.g.<br />

warm absorbers). Application to bright AGN Ch<strong>and</strong>ra grating spectra suggests that the accurate wavelengths in APED are of<br />

great importance to fitting the data. We are exploring additional subroutines to APEC to extend its usefulness for X-ray<br />

photoionized plasma, e.g. to include collisional or photo-excitation of metastable levels for absorption.<br />

Derived from text<br />

Spectroscopy; High Temperature Plasmas; Optical Materials; Thin Plates; X Rays; Photoionization<br />

20040046961 Lawrence Livermore National Lab., Livermore, CA<br />

Mechanical Engineering Safety Note - PEPC Spreader Bar Assembly<br />

Mason, D.; Aug. 26, 2001; 50 pp.; In English<br />

Report No.(s): DE2004-15005720; UCRL-ID-145895; No Copyright; Avail: Department of Energy Information Bridge<br />

The PEPC Spreader Bar Assembly consists of a spreader bar that will be attached to the PEPC Cell Housing or the<br />

Midplane Transportation Fixture during operation. While in use in the OAB (Optics Assembly Building), the Spreader Bar<br />

Assembly will be manipulated by the NOID (New Optics Insertion Device). The other critical components of the assembly<br />

are the three angular contact bearing swivels that attach the spreader bar to the lifting mechanism <strong>and</strong> the corner clamps which<br />

are used to capture the Cell Housing.<br />

NTIS<br />

Mechanical Engineering; Fixtures<br />

20040046967 Lawrence Livermore National Lab., Livermore, CA<br />

Lasershot(sm) Marking System: High-Volume Labeling for Safety-Critical Parts<br />

Dane, C. B.; Hackel, L.; Honig, J.; Halpin, J.; Chen, H. L.; Feb. 16, 2001; 60 pp.; In English<br />

Report No.(s): DE2004-15005707; UCRL-ID-142507; No Copyright; Avail: Department of Energy Information Bridge<br />

185

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