Hybrid characteristics: 3D radiative transfer for parallel adaptive mesh refinement hydrodynamics

被引:90
作者
Rijkhorst, E. -J.
Plewa, T.
Dubey, A.
Mellema, G.
机构
[1] Sterrewacht Leiden, NL-2300 RA Leiden, Netherlands
[2] Univ Chicago, Ctr Astrophys Thermonucl Flashes, Chicago, IL 60637 USA
[3] Univ Chicago, Dept Astron & Astrophys, Chicago, IL 60637 USA
[4] ASTRON, NL-7990 AA Dwingeloo, Netherlands
关键词
radiative transfer; hydrodynamics; ISM : HII regions; planetary nebulae : general;
D O I
10.1051/0004-6361:20053401
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We have developed a three-dimensional radiative transfer method designed specifically for use with parallel adaptive mesh refinement hydrodynamics codes. This new algorithm, which we call hybrid characteristics, introduces a novel form of ray tracing that can neither be classified as long, nor as short characteristics, but which applies the underlying principles, i.e. efficient execution through interpolation and parallelizability, of both. Primary applications of the hybrid characteristics method are radiation hydrodynamics problems that take into account the effects of photoionization and heating due to point sources of radiation. The method is implemented in the hydrodynamics package FLASH. The ionization, heating, and cooling processes are modelled using the DORIC ionization package. Upon comparison with the long characteristics method, we find that our method calculates the column density with a similarly high accuracy and produces sharp and well defined shadows. We show the quality of the new algorithm in an application to the photoevaporation of multiple over-dense clumps. We present several test problems demonstrating the feasibility of our method for performing high resolution three-dimensional radiation hydrodynamics calculations that span a large range of scales. Initial performance tests show that the ray tracing part of our method takes less time to execute than other parts of the calculation (e.g. hydrodynamics and adaptive mesh refinement), and that a high degree of efficiency is obtained in parallel execution. Although the hybrid characteristics method is developed for problems involving photoionization due to point sources, and in its current implementation ignores the effects of diffuse radiation and scattering, the algorithm can be easily adapted to the case of more general radiation fields.
引用
收藏
页码:907 / 920
页数:14
相关论文
共 37 条
  • [1] ABEL T, 2002, MNRAS, V330, P53
  • [2] Amanatides J., 1987, P EUROGRAPHICS, V87, P3, DOI [DOI 10.2312/EGTP.19871000, 10.2312/egtp.19871000]
  • [3] LOCAL ADAPTIVE MESH REFINEMENT FOR SHOCK HYDRODYNAMICS
    BERGER, MJ
    COLELLA, P
    [J]. JOURNAL OF COMPUTATIONAL PHYSICS, 1989, 82 (01) : 64 - 84
  • [4] ADAPTIVE MESH REFINEMENT FOR HYPERBOLIC PARTIAL-DIFFERENTIAL EQUATIONS
    BERGER, MJ
    OLIGER, J
    [J]. JOURNAL OF COMPUTATIONAL PHYSICS, 1984, 53 (03) : 484 - 512
  • [5] HST/WFPC2 and VLT/ISAAC observations of proplyds in the giant HII region NGC 3603
    Brandner, W
    Grebel, EK
    Chu, YH
    Dottori, H
    Brandl, B
    Richling, S
    Yorke, HW
    Points, SD
    Zinnecker, H
    [J]. ASTRONOMICAL JOURNAL, 2000, 119 (01) : 292 - 301
  • [6] A fast, accurate, and robust algorithm for transferring radiation in three-dimensional space
    Cen, RY
    [J]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2002, 141 (01) : 211 - 227
  • [7] COX DP, 1970, THESIS
  • [8] HEATING AND IONIZATION OF HI REGIONS
    DALGARNO, A
    MCCRAY, RA
    [J]. ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, 1972, 10 : 375 - +
  • [9] FRANK A, 1994, ASTRON ASTROPHYS, V289, P937
  • [10] Flash: An adaptive mesh hydrodynamics code for modeling astrophysical thermonuclear flashes
    Fryxell, B
    Olson, K
    Ricker, P
    Timmes, FX
    Zingale, M
    Lamb, DQ
    MacNeice, P
    Rosner, R
    Truran, JW
    Tufo, H
    [J]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2000, 131 (01) : 273 - 334