| pubmed-article:12539754 | rdf:type | pubmed:Citation | lld:pubmed |
| pubmed-article:12539754 | lifeskim:mentions | umls-concept:C1254183 | lld:lifeskim |
| pubmed-article:12539754 | lifeskim:mentions | umls-concept:C0026336 | lld:lifeskim |
| pubmed-article:12539754 | lifeskim:mentions | umls-concept:C0005528 | lld:lifeskim |
| pubmed-article:12539754 | lifeskim:mentions | umls-concept:C0302583 | lld:lifeskim |
| pubmed-article:12539754 | lifeskim:mentions | umls-concept:C0220825 | lld:lifeskim |
| pubmed-article:12539754 | lifeskim:mentions | umls-concept:C1707455 | lld:lifeskim |
| pubmed-article:12539754 | lifeskim:mentions | umls-concept:C0242776 | lld:lifeskim |
| pubmed-article:12539754 | lifeskim:mentions | umls-concept:C0681814 | lld:lifeskim |
| pubmed-article:12539754 | lifeskim:mentions | umls-concept:C0183251 | lld:lifeskim |
| pubmed-article:12539754 | lifeskim:mentions | umls-concept:C1883067 | lld:lifeskim |
| pubmed-article:12539754 | pubmed:issue | 4 | lld:pubmed |
| pubmed-article:12539754 | pubmed:dateCreated | 2003-1-22 | lld:pubmed |
| pubmed-article:12539754 | pubmed:abstractText | Deep-space manned flight as a reality depends on a viable solution to the radiation problem. Both acute and chronic radiation health threats are known to exist, with solar particle events as an example of the former and galactic cosmic rays (GCR) of the latter. In this experiment Iron ions of 1A GeV are used to simulate GCR and to determine the secondary radiation field created as the GCR-like particles interact with a thick target. A NASA prepared food pantry locker was subjected to the iron beam and the secondary fluence recorded. A modified version of the Monte Carlo heavy ion transport code developed by Zeitlin at LBNL is compared with experimental fluence. The foodstuff is modeled as mixed nuts as defined by the 71st edition of the Chemical Rubber Company (CRC) Handbook of Physics and Chemistry. The results indicate a good agreement between the experimental data and the model. The agreement between model and experiment is determined using a linear fit to ordered pairs of data. The intercept is forced to zero. The slope fit is 0.825 and the R2 value is 0.429 over the resolved fluence region. The removal of an outlier, Z=14, gives values of 0.888 and 0.705 for slope and R2 respectively. | lld:pubmed |
| pubmed-article:12539754 | pubmed:keyword | http://linkedlifedata.com/r... | lld:pubmed |
| pubmed-article:12539754 | pubmed:keyword | http://linkedlifedata.com/r... | lld:pubmed |
| pubmed-article:12539754 | pubmed:language | eng | lld:pubmed |
| pubmed-article:12539754 | pubmed:journal | http://linkedlifedata.com/r... | lld:pubmed |
| pubmed-article:12539754 | pubmed:citationSubset | S | lld:pubmed |
| pubmed-article:12539754 | pubmed:chemical | http://linkedlifedata.com/r... | lld:pubmed |
| pubmed-article:12539754 | pubmed:status | MEDLINE | lld:pubmed |
| pubmed-article:12539754 | pubmed:issn | 0273-1177 | lld:pubmed |
| pubmed-article:12539754 | pubmed:author | pubmed-author:MillerJJ | lld:pubmed |
| pubmed-article:12539754 | pubmed:author | pubmed-author:TownsendL WLW | lld:pubmed |
| pubmed-article:12539754 | pubmed:author | pubmed-author:ZeitlinCC | lld:pubmed |
| pubmed-article:12539754 | pubmed:author | pubmed-author:HeilbronnLL | lld:pubmed |
| pubmed-article:12539754 | pubmed:author | pubmed-author:StephensD... | lld:pubmed |
| pubmed-article:12539754 | pubmed:copyrightInfo | c2002 COSPAR. Published by Elsevier Science Ltd. All rights reserved. | lld:pubmed |
| pubmed-article:12539754 | pubmed:issnType | Print | lld:pubmed |
| pubmed-article:12539754 | pubmed:volume | 30 | lld:pubmed |
| pubmed-article:12539754 | pubmed:owner | NASA | lld:pubmed |
| pubmed-article:12539754 | pubmed:authorsComplete | Y | lld:pubmed |
| pubmed-article:12539754 | pubmed:pagination | 901-5 | lld:pubmed |
| pubmed-article:12539754 | pubmed:dateRevised | 2007-4-16 | lld:pubmed |
| pubmed-article:12539754 | pubmed:meshHeading | pubmed-meshheading:12539754... | lld:pubmed |
| pubmed-article:12539754 | pubmed:meshHeading | pubmed-meshheading:12539754... | lld:pubmed |
| pubmed-article:12539754 | pubmed:meshHeading | pubmed-meshheading:12539754... | lld:pubmed |
| pubmed-article:12539754 | pubmed:meshHeading | pubmed-meshheading:12539754... | lld:pubmed |
| pubmed-article:12539754 | pubmed:meshHeading | pubmed-meshheading:12539754... | lld:pubmed |
| pubmed-article:12539754 | pubmed:meshHeading | pubmed-meshheading:12539754... | lld:pubmed |
| pubmed-article:12539754 | pubmed:meshHeading | pubmed-meshheading:12539754... | lld:pubmed |
| pubmed-article:12539754 | pubmed:meshHeading | pubmed-meshheading:12539754... | lld:pubmed |
| pubmed-article:12539754 | pubmed:meshHeading | pubmed-meshheading:12539754... | lld:pubmed |
| pubmed-article:12539754 | pubmed:meshHeading | pubmed-meshheading:12539754... | lld:pubmed |
| pubmed-article:12539754 | pubmed:year | 2002 | lld:pubmed |
| pubmed-article:12539754 | pubmed:articleTitle | Monte Carlo transport model comparison with 1A GeV accelerated iron experiment: heavy-ion shielding evaluation of NASA space flight-crew foodstuff. | lld:pubmed |
| pubmed-article:12539754 | pubmed:affiliation | University of Tennessee, Knoxville, TN 37996-2300, USA. | lld:pubmed |
| pubmed-article:12539754 | pubmed:publicationType | Journal Article | lld:pubmed |
| pubmed-article:12539754 | pubmed:publicationType | Comparative Study | lld:pubmed |
| pubmed-article:12539754 | pubmed:publicationType | Research Support, U.S. Gov't, Non-P.H.S. | lld:pubmed |
| pubmed-article:12539754 | pubmed:publicationType | Research Support, Non-U.S. Gov't | lld:pubmed |
