Exploitation of Space Data for Innovative Helio- and Asteroseismology

    Helioseismology












    Simulated Data

    Index:

    • 1. Spherical-shell simulations of magnetoconvection
    • 2. Numerical Simulations of linear waves/modes in complex media
    • 3. Box simulations of compressible magnetoconvection

    1. Spherical-shell simulations of magnetoconvection

    NamesLink/Contact personComments and References
    ASH (anelastic spherical harmonic) simulation website

    Contact: S. Brun (CEA)
    contact    		 3D anelastic HD and MHD simulations, shell up to 0.98 Rsun, full sphere (r=0) now possible.
    Availability:
    Data available on demand (Any of Sacha Brun's 2-D or 3-D data are available on demand, HD or MHD).
    Contact Sacha Brun.
    References:
    e.g.,Brun, Miesch & Toomre 2004 ApJ
    more reference info
    MagICwebsite

    Contact:
    Johannes Wicht
    contact
    Thomas Gastine
    contact
    Ankit Barik
    contact     		Anelastic stellar simulation.
    Availability: Can be used, modified and redistributed under the terms of the GPL v3 licence (see here )
    References: (see the website for more details)
    e.g., Wicht 2002 Physics of the Earth and Planetary Interios , Gastine and Wicht 2012 Icarus
    MHD EULAGContact:
    Charbonneau (Universite de Montreal)    		 Global MHD simulation of convection zone (Anelastic simulation).
    References:
    e.g. Cossette, Charbonneau, Smolarkiewicz 2013, ApJL
    AMaTeRAS
    (AMR Magnetohydrodynamics code
    with Technique of RSS for Astro-
    and Solar physics)    		 Contacts:
    Hotta (Chiba Univ.)
    contact
    M. Rempel (HAO)
    contact
    		 Simulation with reduced sound speed.
    References:
    e.g., Hotta et.al. 2012 A&A
    Pencil Code
    website

    Contacts:
    Petri Käpylä (Univ. of Helsinki)
    contact
    Jörn Warnecke (MPS)
    contact
    Axel Brandenburg (NORDITA)
    contact     		Compressible HD and MHD simulations in spherical wedges where polar regions are omitted. Also possible to add a coronal layer.
    Availability: Open source licensed under GPL3, freely expandable (http://pencil-code.googlecode.com/)
    Data available on demand, please contact Petri Käpylä
    References:
    e.g. Käpylä et al. 2011, Käpylä et al. 2012, Käpylä et al. 2013, Warnecke et al. 2013

    2. Numerical Simulations of linear waves/modes in complex media

    NamesLink/Contact personAvailability
    SPARC and Glass website

    Contact: S. Hanasoge
    contact
    E. Papini (MPS)
    contact     		SPARC : Linear HD, plane-parallel geometry
    Glass : Linear HD, 3D spherical geometry - full sphere
    Availability:
    SPARC codes can be downloaded from the website
    SLiM (Semi-spectral Linear MHD) codewebsite

    Contact: R.Cameron (MPS)
    contact
    H. Schunker (MPS)
    contact     		Simulation of wave propagation through an inhomogeneous, magnetised solar atmosphere
    Cameron et al. 2007 AN
    Availability:
    Older version is available on the web. For newer version contact Cameron.
    IAC MHD Mancha code website

    Contact: T. Felipe(NWRA)
    contact
    E. Khomenko(IAC)
    contact     		The current working version of the code is 2.5D/3D magnetohydrodynamical code with hyper diffusion algorithms and Cartesian grid written in Fortran 90 (2.5D means that all vector quantities are in three dimensions, while the derivatives are only done in two dimensions).
    Availability:
    Contact Felipe or Khomenko for current version data.
    Newer version will be available at the webapge around later 2014.
    SAC codeSheffield groupReference:
    Shelyag et al. 2008 A&A, Shelyag et al. 2009 A&A
    Pencil Codewebsite

    Contact:
    Axel Brandenburg (NORDITA)
    contact     		Codes for high-order finite-difference code for compressible hydrodynamic flows with magnetic fields.
    Availability:
    open, extendable code
    Artificial helioseismology data by Thomas Hartlepwebsite
    Contact:
    Thomas Hartlep (see website)    		 Numerical simulations of helioseismic oscillations in a 3D full sphere Sun. Several datasets with different setups are available.
    Availability:
    Datasets are downloadable from the website
    Artificial helioseismology data by K. Parchevsky Contact: K. Parchevsky 3D simulation of acoustic waves in the solar upper convection zone.
    Reference:
    e.g., Parchevsky & Kosovichev 2007 ApJ

    3. Box simulations of compressible magnetoconvection

    NamesLink/Contact personComments
    MURaMwebsite

    Contact: M. Rempel (HAO)
    contact
    R. Cameron (MPS)
    contact    		 3D MHD simulation including radiative transfer
    Reference: Voegler et al. 2005 A&A
    Availability:
    Will be open on their website Currently no documents for users yet.
    Some snapshots and shorter time series (1-2hr) are available at MPS. For this, contact R. Cameron.
    For sunspot data and longer (1day - ) data, contact M. Rempel.
    STAGGERwebsite

    Contact: Bob Stein (Michigan State Univ.)
    contact    		 3D MHD convection simulation.
    Reference:e.g., Stein et al. 2009 AIPC, Stein et al.2009 ASPC, Stein 2012 LRSP
    Availability:
    Some datacubes are available on the website.
    Selected datacubes (96Mmx96Mmx20Mm, ~5hr) of Quiet Sun (with weak magnetic field) are available at MPS. For this, contact: K. Nagashima (MPS)
    BifrostResearch Group in Oslo Stellar atmosphere simulation from the convection zone to the upper atmosphere (corona).
    Reference: Gudikson et al. 2011, A&A
    CO5BOLDwebsite 3D radiative hydrodynamics simulation
    Reference:Freytaget al. 2012 J, Nutto, Steiner, Roth 2012 A&A
    Pencil Code
    website

    Contact persons:
    Petri Käpylä (Univ. of Helsinki)
    contact
    Axel Brandenburg (NORDITA)
    contact     		Availability:
    Codes are open and extendable
    References:
    Käpylä et al. 2008, Käpylä et al. 2009

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