TERAPIXEL IMAGING OF COSMOLOGICAL SIMULATIONS

被引:10
作者
Feng, Yu [1 ,2 ]
Croft, Rupert A. C. [1 ,2 ]
Di Matteo, Tiziana [1 ,2 ]
Khandai, Nishikanta [1 ,2 ]
Sargent, Randy [3 ]
Nourbakhsh, Illah [3 ]
Dille, Paul [3 ]
Bartley, Chris [3 ]
Springel, Volker [4 ,5 ]
Jana, Anirban [6 ]
Gardner, Jeffrey [7 ]
机构
[1] Carnegie Mellon Univ, Bruce & Astrid McWilliams Ctr Cosmol, Pittsburgh, PA 15213 USA
[2] Carnegie Mellon Univ, Dept Phys, Pittsburgh, PA 15213 USA
[3] Carnegie Mellon Univ, Inst Robot, Pittsburgh, PA 15213 USA
[4] Heidelberger Inst Theoret Studien, D-69118 Heidelberg, Germany
[5] Heidelberg Univ, Zentrum Astron, Astron Recheninst, D-69120 Heidelberg, Germany
[6] Pittsburgh Supercomp Ctr, Pittsburgh, PA 15213 USA
[7] Univ Washington, Dept Phys, Seattle, WA 98195 USA
基金
美国国家科学基金会;
关键词
cosmology: observations; large-scale structure of universe; BUBBLE-GROWTH; BLACK-HOLES; DARK-MATTER; CODE; EVOLUTION; GALAXIES; MODEL;
D O I
10.1088/0067-0049/197/2/18
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The increasing size of cosmological simulations has led to the need for new visualization techniques. We focus on smoothed particle hydrodynamic (SPH) simulations run with the GADGET code and describe methods for visually accessing the entire simulation at full resolution. The simulation snapshots are rastered and processed on supercomputers into images that are ready to be accessed through a Web interface (GigaPan). This allows any scientist with a Web browser to interactively explore simulation data sets in both spatial and temporal dimensions and data sets which in their native format can be hundreds of terabytes in size or more. We present two examples, the first a static terapixel image of the MassiveBlack simulation, a P-GADGET SPH simulation with 65 billion particles, and the second an interactively zoomable animation of a different simulation with more than 1000 frames, each a gigapixel in size. Both are available for public access through the GigaPan Web interface. We also make our imaging software publicly available.
引用
收藏
页数:8
相关论文
共 29 条
  • [1] Resolving cosmic structure formation with the Millennium-II Simulation
    Boylan-Kolchin, Michael
    Springel, Volker
    White, Simon D. M.
    Jenkins, Adrian
    Lemson, Gerard
    [J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2009, 398 (03) : 1150 - 1164
  • [2] EMBEDDING REALISTIC SURVEYS IN SIMULATIONS THROUGH VOLUME REMAPPING
    Carlson, Jordan
    White, Martin
    [J]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2010, 190 (02) : 311 - 314
  • [3] Intercluster filaments in a ΛCDM Universe
    Colberg, JM
    Krughoff, KS
    Connolly, AJ
    [J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2005, 359 (01) : 272 - 282
  • [4] DEGRAF C, 2011, MNRAS UNPUB
  • [5] Cold streams in early massive hot haloes as the main mode of galaxy formation
    Dekel, A.
    Birnboim, Y.
    Engel, G.
    Freundlich, J.
    Goerdt, T.
    Mumcuoglu, M.
    Neistein, E.
    Pichon, C.
    Teyssier, R.
    Zinger, E.
    [J]. NATURE, 2009, 457 (7228) : 451 - 454
  • [6] Energy input from quasars regulates the growth and activity of black holes and their host galaxies
    Di Matteo, T
    Springel, V
    Hernquist, L
    [J]. NATURE, 2005, 433 (7026) : 604 - 607
  • [7] Direct cosmological simulations of the growth of black holes and galaxies
    Di Matteo, Tiziana
    Colberg, Joerg
    Springel, Volker
    Hernquist, Lars
    Sijacki, Debora
    [J]. ASTROPHYSICAL JOURNAL, 2008, 676 (01) : 33 - 53
  • [8] DIMATTEO T, 2011, APJL UNPUB
  • [9] Simulating the physical properties of dark matter and gas inside the cosmic web
    Dolag, K.
    Meneghetti, M.
    Moscardini, L.
    Rasia, E.
    Bonaldi, A.
    [J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2006, 370 (02) : 656 - 672
  • [10] Exploring the Millennium Run - Scalable Rendering of Large-Scale Cosmological Datasets
    Fraedrich, Roland
    Schneider, Jens
    Westermann, Ruediger
    [J]. IEEE TRANSACTIONS ON VISUALIZATION AND COMPUTER GRAPHICS, 2009, 15 (06) : 1251 - 1258