Fast and versatile diagnostic radiative transfer of 3-D models of the ISM
ISM 3D 模型的快速、多功能诊断辐射传输
基本信息
- 批准号:203090784
- 负责人:
- 金额:--
- 依托单位:
- 依托单位国家:德国
- 项目类别:Priority Programmes
- 财政年份:2011
- 资助国家:德国
- 起止时间:2010-12-31 至 2014-12-31
- 项目状态:已结题
- 来源:
- 关键词:
项目摘要
The key link between theoretical/numerical models of the interstellar medium (ISM) and observations is radiative transfer. The radiation we observe with Earth-bound and space-based telescopes is usually difficult to interpret without it. And numerical models of the ISM cannot be properly compared to observations without radiative transfer. In recent years fully 3-D numerical (radiation-)(chemo-)(magneto-)hydrodynamic (RCMHD) models of the ISM have become mainstream. What is needed now is a versatile, powerful, yet publicly available radiative transfer package that can be used to analyze fully 3-D Adaptive Mesh Refinement RCMHD models of the ISM. I have built a beta-version of such a code: RADMC-3D. It can perform dust continuum and molecular/atomic line transfer, has full 3-D AMR capabilities, is easy to use and yet is very versatile. It has an extensive manual and I have made it publicly available from the start. What is needed now is the final developing stage: (1) Much more extensive testing, (2) implementation of some more physics such as quantum-heated grains and full non-LTE line transfer and (3) a mode for handling domain-decomposed very large models on distributed memory machines.
星际介质的理论/数值模型(ISM)和观测之间的关键环节是辐射传输。我们用地球和太空望远镜观测到的辐射通常很难解释,而ISM的数值模型也不能与没有辐射传输的观测结果进行适当的比较。近年来,ISM的全三维数值(辐射)(化学)(磁)流体动力学(RCMHD)模型已成为主流。现在需要的是一个通用的,强大的,但公开可用的辐射传输包,可用于分析完全三维自适应网格细化RCMHD模型的ISM。我已经建立了这样一个代码的beta版本:RADMC-3D。它可以执行尘埃连续谱和分子/原子谱线转移,具有完整的3-D AMR功能,易于使用,但用途非常广泛。它有一个广泛的手册,我从一开始就公开了它。现在需要的是最后的开发阶段:(1)更广泛的测试,(2)实现更多的物理,如量子加热颗粒和完全非LTE线传输,以及(3)在分布式内存机器上处理域分解的超大型模型的模式。
项目成果
期刊论文数量(0)
专著数量(0)
科研奖励数量(0)
会议论文数量(0)
专利数量(0)
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Professor Dr. Cornelis Petrus Dullemond其他文献
Professor Dr. Cornelis Petrus Dullemond的其他文献
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{{ truncateString('Professor Dr. Cornelis Petrus Dullemond', 18)}}的其他基金
The Formation and Evolution of resonant planetary Systems
共振行星系统的形成和演化
- 批准号:
361764675 - 财政年份:2017
- 资助金额:
-- - 项目类别:
Priority Programmes
Composition of planets with an N-body-Monte-Carlo approach
采用 N 体蒙特卡罗方法的行星组成
- 批准号:
362460405 - 财政年份:2017
- 资助金额:
-- - 项目类别:
Priority Programmes
Chondrule formation: Nebular gas confinement of impact splashes
球粒形成:撞击飞溅的星云气体限制
- 批准号:
248600313 - 财政年份:2014
- 资助金额:
-- - 项目类别:
Priority Programmes
The role of water in the process of planet formation
水在行星形成过程中的作用
- 批准号:
211591189 - 财政年份:2012
- 资助金额:
-- - 项目类别:
Priority Programmes
FUV-Driven Photoevaporation of protoplanetary Disks
FUV 驱动的原行星盘光蒸发
- 批准号:
188379957 - 财政年份:2011
- 资助金额:
-- - 项目类别:
Research Grants
Modeling the evolution of the dust population in protoplanetary disks
模拟原行星盘中尘埃群的演化
- 批准号:
158702285 - 财政年份:2009
- 资助金额:
-- - 项目类别:
Research Units
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