SALT EFFECTS IN SOLUTIONS OF PEPTIDES AND NUCLEIC ACIDS

肽和核酸溶液中的盐效应

• 批准号: 7601280
• 负责人: Bernard MONTGOMERY PETTITT
• 金额: $ 0.03万
• 依托单位: CARNEGIE-MELLON UNIVERSITY
• 依托单位国家: 美国
• 财政年份: 2007
• 资助国家: 美国
• 起止时间: 2007-08-01 至 2008-07-31
• 项目状态: 已结题
• 来源: https://reporter.nih.gov/project-details/7601280
• 关键词: Basic Science; Code; Computer Retrieval of Information on Scientific Projects Database; Coupled; Funding; Grant; Individual; Institution; Modeling; Numbers; Peptide Nucleic Acids; Production; Research; Research Personnel; Resources; Running; Site; Sodium Chloride; Solutions; Source; Time; United States National Aeronautics and Space Administration; United States National Institutes of Health; Weather; experience; member; planetary Atmosphere; simulation

This subproject is one of many research subprojects utilizing the resources provided by a Center grant funded by NIH/NCRR. The subproject and investigator (PI) may have received primary funding from another NIH source, and thus could be represented in other CRISP entries. The institution listed is for the Center, which is not necessarily the institution for the investigator. We request in this renewal proposal to the LRAC continued support for the computational needs of the Center for Integrated Space Weather Modeling, CISM, as well as other NSF and NASA grants held by team members. From our previous experience, we have deemed it appropriate to combine the research of our CISM colleagues for the grants listed into this single large request, and thus limit the number of submission to the committee. The bulk of the requested time will support basic science studies with large-scale production runs of our massive parallel solar corona, heliosphere, and magnetosphere run primarily individually, but also coupled with one or two other CISM codes. As discussed below, there are many scientific issues that must be resolved, especially in the solar atmosphere and earths magnetosphere, to increase the scientific accuracy of the fully coupled runs. Furthermore, our other grants (besides CISM) require basic scientific studies of the solar atmosphere and the earths magnetosphere. In this year, we will also attempt to use the resources of the TeraGrid to perform a limited number of fully coupled code simulations, with individual codes running on the (distributed) TeraGrid sites.

该子项目是利用该技术的众多研究子项目之一 资源由 NIH/NCRR 资助的中心拨款提供。子项目及 研究者 (PI) 可能已从 NIH 的另一个来源获得主要资金， 因此可以在其他 CRISP 条目中表示。列出的机构是 对于中心来说，它不一定是研究者的机构。 在这份更新提案中，我们请求 LRAC 继续支持综合空间天气建模中心、CISM 以及团队成员持有的其他 NSF 和 NASA 拨款的计算需求。根据我们之前的经验，我们认为将 CISM 同事的研究成果合并到这个单一的大型请求中是适当的，从而限制了向委员会提交的数量。所要求的大部分时间将支持基础科学研究，大规模并行太阳日冕、日光层和磁层的大规模生产运行主要单独运行，但也与一两个其他 CISM 代码结合使用。如下所述，有许多科学问题必须解决，特别是在太阳大气层和地球磁层中，以提高全耦合运行的科学准确性。此外，我们的其他拨款（除 CISM 之外）需要对太阳大气层和地球磁层进行基础科学研究。今年，我们还将尝试使用 TeraGrid 的资源来执行有限数量的完全耦合代码模拟，并在（分布式）TeraGrid 站点上运行单独的代码。