Publications

2019

  • F. Zaussinger, “GeoFlow I and GeoFlow II: A Review,” in Book of abstracts, school ISTROF 2019, Instabilities and turbulence in strato-rotational flows, cottbus, 2019.
    [BibTeX] [Download PDF]
    @inproceedings{Zaussinger_2019d,
    Author = {F. Zaussinger},
    Booktitle = {Book of abstracts, School {ISTROF} 2019, {I}nstabilities and Turbulence in Strato-Rotational Flows, Cottbus},
    Date-Added = {2019-07-03 10:43:31 +0200},
    Date-Modified = {2019-07-08 13:55:16 +0200},
    Keywords = {zaussinger},
    Organization = {BTU Cottbus-Senftenberg},
    Title = {{GeoFlow I and GeoFlow II: A Review}},
    Url = {https://www-docs.b-tu.de/fg-aerodynamik-stroemungslehre/public/PDF/Veranstaltungen/Aktuelles/ISTROF2019/AbstractBook.pdf},
    Year = {2019},
    Bdsk-Url-1 = {https://www-docs.b-tu.de/fg-aerodynamik-stroemungslehre/public/PDF/Veranstaltungen/Aktuelles/ISTROF2019/AbstractBook.pdf}}

  • F. Zaussinger and F. Kupka, “Layer formation in double-diffusive convection over resting and moving heated plates,” Theoretical and computational fluid dynamics, 2019. doi:10.1007/s00162-019-00499-7
    [BibTeX]
    @article{Zaussinger_2019c,
    Author = {Zaussinger, F. and Kupka, F.},
    Date-Added = {2019-05-29 09:06:27 +0200},
    Date-Modified = {2019-07-08 14:03:05 +0200},
    Doi = {10.1007/s00162-019-00499-7},
    Journal = {Theoretical and Computational Fluid Dynamics},
    Keywords = {SC,zaussinger},
    Title = {{Layer formation in double-diffusive convection over resting and moving heated plates}},
    Year = 2019,
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    Bdsk-Url-1 = {https://doi.org/10.1007/s00162-019-00499-7}}

  • F. Zaussinger, P. Canfield, A. Froitzheim, V. Travnikov, P. Haun, M. Meier, A. Meyer, P. Heintzmann, T. Driebe, and C. Egbers, “Atmoflow – investigation of atmospheric-like fluid flows under microgravity conditions,” Microgravity science and technology, 2019. doi:10.1007/s12217-019-09717-7
    [BibTeX] [Abstract] [Download PDF]

    The main objective of the AtmoFlow experiment is the investigation of convective flows in the spherical gap geometry. Gaining fundamental knowledge on the origin and behavior of flow phenomena such as global cells and planetary waves is interesting not only from a meteorological perspective. Understanding the interaction between atmospheric circulation and a planet’s climate, be it Earth, Mars, Jupiter, or a distant exoplanet, contributes to various fields of research such as astrophysics, geophysics, fluid physics, and climatology. AtmoFlow aims to observe flows in a thin spherical gap that are subjected to a central force-field. The Earth’s own gravitational field interferes with a simulated central force-field with the given parameters of the model which makes microgravity conditions of g<10−3g0{\$}{$\backslash$}mathrm {\{}g{\}}<10\^{}{\{}-3{\}} {$\backslash$}mathrm {\{}g{\}}{_}{\{}0{\}}{\$}(e.g. on the ISS) necessary. Without losing its overall view on the complex physics, circulation in planetary atmospheres can be reduced to a simple model of a central gravitational field, the incoming and outgoing energy (e.g. radiation) and rotational effects. This strongly simplified assumption makes it possible to break some generic cases down to test models which can be investigated by laboratory experiments and numerical simulations. Varying rotational rates and temperature boundary conditions represent different types of planets. This is a very basic approach, but various open questions regarding local pattern formation or global planetary cells can be investigated with that setup. A concept has been defined for developing a payload that could be installed and utilized on-board the International Space Station (ISS). This concept is based on the microgravity experiment GeoFlow, which has been conducted successfully between 2008 and 2016 on the ISS. This paper addresses the scientific goals, the experimental setup, the concept for implementation of the AtmoFlow experiment on the ISS and first numerical results.

    @article{Zaussinger_2019b,
    Abstract = {The main objective of the AtmoFlow experiment is the investigation of convective flows in the spherical gap geometry. Gaining fundamental knowledge on the origin and behavior of flow phenomena such as global cells and planetary waves is interesting not only from a meteorological perspective. Understanding the interaction between atmospheric circulation and a planet's climate, be it Earth, Mars, Jupiter, or a distant exoplanet, contributes to various fields of research such as astrophysics, geophysics, fluid physics, and climatology. AtmoFlow aims to observe flows in a thin spherical gap that are subjected to a central force-field. The Earth's own gravitational field interferes with a simulated central force-field with the given parameters of the model which makes microgravity conditions of g<10−3g0{\$}{$\backslash$}mathrm {\{}g{\}}<10\^{}{\{}-3{\}} {$\backslash$}mathrm {\{}g{\}}{\_}{\{}0{\}}{\$}(e.g. on the ISS) necessary. Without losing its overall view on the complex physics, circulation in planetary atmospheres can be reduced to a simple model of a central gravitational field, the incoming and outgoing energy (e.g. radiation) and rotational effects. This strongly simplified assumption makes it possible to break some generic cases down to test models which can be investigated by laboratory experiments and numerical simulations. Varying rotational rates and temperature boundary conditions represent different types of planets. This is a very basic approach, but various open questions regarding local pattern formation or global planetary cells can be investigated with that setup. A concept has been defined for developing a payload that could be installed and utilized on-board the International Space Station (ISS). This concept is based on the microgravity experiment GeoFlow, which has been conducted successfully between 2008 and 2016 on the ISS. This paper addresses the scientific goals, the experimental setup, the concept for implementation of the AtmoFlow experiment on the ISS and first numerical results.},
    Author = {Zaussinger, F. and Canfield, P. and Froitzheim, A. and Travnikov, V. and Haun, P. and Meier, M. and Meyer, A. and Heintzmann, P. and Driebe, T. and Egbers, Ch.},
    Date-Added = {2019-06-27 10:49:23 +0200},
    Date-Modified = {2019-06-27 10:49:59 +0200},
    Doi = {10.1007/s12217-019-09717-7},
    Isbn = {1875-0494},
    Journal = {Microgravity Science and Technology},
    Title = {AtmoFlow - Investigation of Atmospheric-Like Fluid Flows Under Microgravity Conditions},
    Url = {https://doi.org/10.1007/s12217-019-09717-7},
    Year = {2019},
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  • F. Zaussinger, C. Egbers, P. Canfield, P. Haun, V. Travnikov, A. Froitzheim, A. Meyer, and M. Meier, "AtmoFlow - Investigation of atmospheric-like fluid flows under micro-gravity conditions," in EGU general assembly conference abstracts, 2019, p. 8441.
    [BibTeX] [Download PDF]
    @inproceedings{Zaussinger_2019a,
    Author = {Zaussinger, Florian and Egbers, Christoph and Canfield, Peter and Haun, Peter and Travnikov, Vadim and Froitzheim, Andreas and Meyer, Antoine and Meier, Martin},
    Booktitle = {{EGU} General Assembly Conference Abstracts},
    Date-Modified = {2019-07-03 10:36:16 +0200},
    Keywords = {ATMOFLOW,zaussinger},
    Month = April,
    Pages = {8441},
    Series = {{EGU} General Assembly Conference Abstracts},
    Title = {{AtmoFlow - Investigation of atmospheric-like fluid flows under micro-gravity conditions}},
    Url = {https://meetingorganizer.copernicus.org/EGU2019/EGU2019-8441.pdf},
    Volume = 21,
    Year = 2019,
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2018

  • F. Zaussinger, "A dynamic beam model for the motility of listeria monocytogenes," Acta mechanica, p. 1–18, 2018. doi:10.1007/s00707-018-2277-1
    [BibTeX] [Abstract] [Download PDF]

    A non-conservative Lagrangian is used to derive a dynamic beam equation in a moving reference frame to describe the motility of Listeria monocytogenes. Bending, stretching, and frictional forces are incorporated to describe the kinematics of the moving actin filament network. Adapted boundary conditions are able to simulate the influence of the bacterium on the tail as well as the polymerization process. A semi-implicit numerical operator splitting method has been developed to solve the nonlinear equations in the plane. The model has been validated on existing force-velocity relationships and measurements for realistic physical model parameters. In particular, the fictional losses due to substrate-tail adhesion have been analyzed by a linear and a nonlinear approach. Numerical simulations are performed for varying polymerization speeds, friction, and bending parameters. Complex trajectories of the actin tail are found by adjusting the bending properties of the attaching actin filament cluster. The results reveal that the present model is able to predict and reproduce actin-based motions observed in experiments.

    @article{Zaussinger_2018c,
    Abstract = {A non-conservative Lagrangian is used to derive a dynamic beam equation in a moving reference frame to describe the motility of Listeria monocytogenes. Bending, stretching, and frictional forces are incorporated to describe the kinematics of the moving actin filament network. Adapted boundary conditions are able to simulate the influence of the bacterium on the tail as well as the polymerization process. A semi-implicit numerical operator splitting method has been developed to solve the nonlinear equations in the plane. The model has been validated on existing force-velocity relationships and measurements for realistic physical model parameters. In particular, the fictional losses due to substrate-tail adhesion have been analyzed by a linear and a nonlinear approach. Numerical simulations are performed for varying polymerization speeds, friction, and bending parameters. Complex trajectories of the actin tail are found by adjusting the bending properties of the attaching actin filament cluster. The results reveal that the present model is able to predict and reproduce actin-based motions observed in experiments.},
    Author = {Zaussinger, Florian},
    Date-Added = {2018-10-26 08:29:07 +0200},
    Date-Modified = {2019-03-14 19:53:43 +0100},
    Doi = {10.1007/s00707-018-2277-1},
    Issn = {0001-5970},
    Journal = {Acta Mechanica},
    Keywords = {Listeria,zaussinger},
    Month = {10},
    Pages = {1--18},
    Title = {A dynamic beam model for the motility of Listeria monocytogenes},
    Url = {http:https://doi.org/10.1007/s00707-018-2277-1},
    Year = {2018},
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    Bdsk-Url-1 = {http:https://doi.org/10.1007/s00707-018-2277-1},
    Bdsk-Url-2 = {https://doi.org/10.1007/s00707-018-2277-1}}

  • F. Zaussinger, P. Canfield, T. Driebe, C. Egbers, P. Heintzmann, V. Travnikov, A. Froitzheim, P. Haun, and M. Meier, "AtmoFlow - Simulating atmospheric flows on the International Space Station. Part II: Experiments and numerical simulations," in 69th IAC conference proceedings, 2018.
    [BibTeX] [Download PDF]
    @inproceedings{Zaussinger_2018f,
    Author = {Zaussinger, Florian and Canfield, Peter and Driebe, Thomas and Egbers, Christoph and Heintzmann, Pascal and Travnikov, Vadim and Froitzheim, Andreas and Haun, Peter and Meier, Martin},
    Booktitle = {69th {IAC} conference proceedings},
    Date-Added = {2018-10-25 20:32:20 +0200},
    Date-Modified = {2019-07-03 10:21:47 +0200},
    Keywords = {ATMOFLOW,zaussinger},
    Month = {September},
    Organization = {International Astronautical Federation},
    Title = {{A}tmo{F}low - {S}imulating atmospheric flows on the {I}nternational {S}pace {S}tation. {P}art {II}: {E}xperiments and numerical simulations},
    Url = {http://iafastro.directory/iac/archive/browse/IAC-18/A2/7/42847/},
    Volume = {18.A2.7.18-69},
    Year = {2018},
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  • F. Zaussinger, P. Haun, I. Mutabazi, and C. Egbers, "Dielectrically driven convection in spherical gap geometry," in Scientific programm EFMC12, http://info.tuwien.ac.at/efmc12/EFMC12_program_v3.2.pdf, 2018, p. 46.
    [BibTeX]
    @inproceedings{Zaussinger_2018h,
    Address = {http://info.tuwien.ac.at/efmc12/EFMC12_program_v3.2.pdf},
    Author = {Zaussinger, F. and Haun, P. and Mutabazi, I. and Egbers, Ch.},
    Booktitle = {{Scientific programm EFMC12}},
    Date-Added = {2019-06-07 11:30:22 +0200},
    Date-Modified = {2019-07-08 13:57:51 +0200},
    Month = {September},
    Pages = {46},
    Series = {Scientific programm EFMC},
    Title = {Dielectrically driven convection in spherical gap geometry},
    Volume = {1},
    Year = {2018}}

  • P. Canfield, F. Zaussinger, C. Egbers, and P. Heintzmann, "AtmoFlow - Simulating atmospheric flows on the International Space Station. Part I: Experiment and ISS-implementation concept," in 69th IAC conference proceedings, 2018.
    [BibTeX] [Download PDF]
    @inproceedings{Canfield_2018a,
    Author = {Canfield, Peter and Zaussinger, Florian and Egbers, Christoph and Heintzmann, Pascal},
    Booktitle = {69th {IAC} conference proceedings},
    Date-Added = {2018-10-25 20:03:23 +0200},
    Date-Modified = {2019-07-03 10:22:06 +0200},
    Keywords = {ATMOFLOW,zaussinger},
    Month = {September},
    Organization = {International Astronautical Federation},
    Title = {{A}tmo{F}low - {S}imulating atmospheric flows on the {I}nternational {S}pace {S}tation. {P}art {I}: {E}xperiment and {ISS}-implementation concept},
    Url = {http://iafastro.directory/iac/archive/browse/IAC-18/A2/6/44307/},
    Volume = {18.A2.6.15-69},
    Year = {2018},
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  • F. Zaussinger, P. Haun, M. Neben, T. Seelig, V. Travnikov, C. Egbers, H. Yoshikawa, and I. Mutabazi, "Dielectrically driven convection in spherical gap geometry," Phys. rev. fluids, vol. 3, p. 93501, 2018. doi:10.1103/PhysRevFluids.3.093501
    [BibTeX] [Download PDF]
    @article{Zaussinger_2018b,
    Author = {Zaussinger, F. and Haun, P. and Neben, M. and Seelig, T. and Travnikov, V. and Egbers, C. and Yoshikawa, H. and Mutabazi, I.},
    Date-Added = {2018-09-12 08:50:50 +0200},
    Date-Modified = {2019-03-15 09:29:23 +0100},
    Doi = {10.1103/PhysRevFluids.3.093501},
    Issue = {9},
    Journal = {Phys. Rev. Fluids},
    Keywords = {dielectric heating,zaussinger},
    Month = {Sep},
    Numpages = {17},
    Pages = {093501},
    Publisher = {American Physical Society},
    Title = {Dielectrically driven convection in spherical gap geometry},
    Url = {https://link.aps.org/doi/10.1103/PhysRevFluids.3.093501},
    Volume = {3},
    Year = {2018},
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  • F. Kupka, F. Zaussinger, and M. H. Montgomery, "Mixing and overshooting in surface convection zones of DA white dwarfs: First results from ANTARES," Monthly Notices of the Royal Astronomical Society, vol. 474, iss. 4, pp. 4660-4671, 2018. doi:10.1093/mnras/stx3119
    [BibTeX]
    @article{Kupka_2017,
    Author = {Kupka, F. and Zaussinger, F. and Montgomery, M. H.},
    Date-Added = {2018-01-24 10:48:20 +0000},
    Date-Modified = {2019-03-15 09:41:46 +0100},
    Doi = {10.1093/mnras/stx3119},
    Journal = {Monthly {N}otices of the {R}oyal {A}stronomical {S}ociety},
    Keywords = {ANTARES,zaussinger},
    Number = {4},
    Pages = {4660-4671},
    Title = {Mixing and overshooting in surface convection zones of {DA} white dwarfs: {F}irst results from {ANTARES}},
    Volume = {474},
    Year = {2018},
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    Bdsk-Url-1 = {https://dx.doi.org/10.1093/mnras/stx3119}}

  • B. Uhlig, C. Kirner, A. Preuss, J. Graf, M. Neben, and F. Zaussinger, "Kolbenring-Öltransport II : Öltransport durch die Kolbenringe," , Frankfurt am Main 2018.
    [BibTeX] [Abstract]

    Ziele des Vorhabens sind die Verbesserung der Messtechnik für tribologische Untersuchungen in der Kolbengruppe aus dem Vorläufervorhaben Kolbenring-Öltransport I und die Untersuchung von verschiedenen Betriebsbedingungen und Komponenten hinsichtlich ihres Einflusses auf den Ölhaushalt. Der Fokus liegt auf der verbesserten Auflösung der Schmierfilmdickenmessung und der Ringsto√ülagen. Mit der erweiterten Kapillar- und Lichtleiterkonfiguration werden neue Öltransportvorgänge entlang des Kolbenringpakets mittels Tracerinjektion und simultaner LiF-Messung beobachtet. Das methodische Vorgehen bei der optischen Analyse des Kapillarfüllungsgrades wird an einem Labor-Druckprüfstand weiterentwickelt. Des Weiteren werden komplexe Simulationsmodelle erstellt, mit denen die Kolbensekundär-bewegung, die Kolbenringbewegung, die Gasströmung im Ringpaket und der Öltransport im Ringpaket geklärt werden können. Die Kolbensekundärbewegungsrechnung basiert auf einer FEM-Diskretisierung die aus CAD-Modellen sämtlicher Bauteile abgeleitet ist. Die dreidimensionale Berechnung der Kolbenringbewegung erfolgt unter Berücksichtigung dynamisch wirkender Kräfte aus der Bewegung, der Ringreibung, dem Gasdruck und den Zwischenring- drücken. Die Elastizität der Ringe wird berücksichtigt, so dass Biegung, Torsion und damit auch das Twisten abgebildet werden können. Nut- und Ringgeometrie sowie thermisch bedingte Verzüge flie√üen ebenfalls in die Berechnung mit ein. Als Ergebnisgrö√üen stehen neben den Ringbewegungen und -lagen auch die Gasströmungen und -drücke, Schmierfilmhöhen und Verlustleistungen zur Verfügung.

    @techreport{Uhlig_2018,
    Abstract = {Ziele des Vorhabens sind die Verbesserung der Messtechnik f{\"u}r tribologische Untersuchungen in der Kolbengruppe aus dem Vorl{\"a}ufervorhaben Kolbenring-{\"O}ltransport I und die Untersuchung von verschiedenen Betriebsbedingungen und Komponenten hinsichtlich ihres Einflusses auf den {\"O}lhaushalt. Der Fokus liegt auf der verbesserten Aufl{\"o}sung der Schmierfilmdickenmessung und der Ringsto√{\"u}lagen. Mit der erweiterten Kapillar- und Lichtleiterkonfiguration werden neue {\"O}ltransportvorg{\"a}nge entlang des Kolbenringpakets mittels Tracerinjektion und simultaner LiF-Messung beobachtet. Das methodische Vorgehen bei der optischen Analyse des Kapillarf{\"u}llungsgrades wird an einem Labor-Druckpr{\"u}fstand weiterentwickelt. Des Weiteren werden komplexe Simulationsmodelle erstellt, mit denen die Kolbensekund{\"a}r-bewegung, die Kolbenringbewegung, die Gasstr{\"o}mung im Ringpaket und der {\"O}ltransport im Ringpaket gekl{\"a}rt werden k{\"o}nnen. Die Kolbensekund{\"a}rbewegungsrechnung basiert auf einer FEM-Diskretisierung die aus CAD-Modellen s{\"a}mtlicher Bauteile abgeleitet ist. Die dreidimensionale Berechnung der Kolbenringbewegung erfolgt unter Ber{\"u}cksichtigung dynamisch wirkender Kr{\"a}fte aus der Bewegung, der Ringreibung, dem Gasdruck und den Zwischenring- dr{\"u}cken. Die Elastizit{\"a}t der Ringe wird ber{\"u}cksichtigt, so dass Biegung, Torsion und damit auch das Twisten abgebildet werden k{\"o}nnen. Nut- und Ringgeometrie sowie thermisch bedingte Verz{\"u}ge flie√{\"u}en ebenfalls in die Berechnung mit ein. Als Ergebnisgr{\"o}√{\"u}en stehen neben den Ringbewegungen und -lagen auch die Gasstr{\"o}mungen und -dr{\"u}cke, Schmierfilmh{\"o}hen und Verlustleistungen zur Verf{\"u}gung.},
    Address = {Frankfurt am Main},
    Author = {Uhlig, Benedict and Kirner, Claus and Preuss, Ann-Christin and Graf, Johann and Neben, Matthias and Zaussinger, Florian},
    Date-Added = {2018-07-31 17:12:15 +0200},
    Date-Modified = {2019-03-14 19:56:14 +0100},
    Keywords = {Kolbenring,zaussinger},
    Language = {de},
    Pages = {70},
    Publisher = {FVV, Forschungsvereinigung Verbrennungskraftmaschinen},
    Title = {{Kolbenring-{\"O}ltransport II : {\"O}ltransport durch die Kolbenringe}},
    Year = {2018},
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  • C. Egbers, F. Zaussinger, P. Haun, P. Canfield, V. Travnikov, and A. Froitzheim, "Convection in the spherical gap under micro-gravity conditions: From Earth's mantle to atmospheric flows.," in 20th Int. Couette-Taylor Workshop, 2018.
    [BibTeX] [Download PDF]
    @inproceedings{Zaussinger_2018e,
    Author = {Egbers, Christoph and Zaussinger, Florian and Haun, Peter and Canfield, Peter and Travnikov, Vadim and Froitzheim, Andreas},
    Booktitle = {{20th Int. Couette-Taylor Workshop}},
    Date-Added = {2018-08-21 08:13:04 +0200},
    Date-Modified = {2019-07-03 10:30:38 +0200},
    Keywords = {GEOFLOW,zaussinger},
    Organization = {{Aix Marseille universite}},
    Title = {{Convection in the spherical gap under micro-gravity conditions: From Earth's mantle to atmospheric flows.}},
    Url = {https://ictw20.sciencesconf.org/data/pages/Final_Program_IV.pdf},
    Year = {2018},
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  • F. Zaussinger, C. Egbers, P. Canfield, P. Haun, V. Travnikov, and A. Froitzheim, "AtmoFlow - Experimental investigation of atmospheric flows under microgravity conditions," in EGU general assembly conference abstracts, 2018, p. 6273.
    [BibTeX] [Download PDF]
    @inproceedings{Zaussinger_2018d,
    Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
    Author = {Zaussinger, Florian and Egbers, Christoph and Canfield, Peter and Haun, Peter and Travnikov, Vadim and Froitzheim, Andreas},
    Booktitle = {{EGU} General Assembly Conference Abstracts},
    Date-Added = {2019-01-09 15:34:07 +0100},
    Date-Modified = {2019-07-03 10:36:03 +0200},
    Keywords = {ATMOFLOW,zaussinger},
    Month = feb,
    Pages = {6273},
    Series = {{EGU} General Assembly Conference Abstracts},
    Title = {{AtmoFlow - Experimental investigation of atmospheric flows under microgravity conditions}},
    Url = {https://meetingorganizer.copernicus.org/EGU2018/EGU2018-6273.pdf},
    Volume = 20,
    Year = 2018,
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  • F. Zaussinger, F. Kupka, M. Montgomery, and C. Egbers, Numerical simulation of DA white dwarf surface convectionIOP Publishing, 2018. doi:doi:10.1088/1742-6596/1031/1/012013
    [BibTeX] [Download PDF]
    @proceedings{Zaussinger_2018a,
    Author = {F. Zaussinger and F. Kupka and M. Montgomery and Ch. Egbers},
    Date-Added = {2018-07-16 07:49:02 +0000},
    Date-Modified = {2019-03-29 10:02:37 +0100},
    Doi = {doi:10.1088/1742-6596/1031/1/012013},
    Journal = {Journal of {P}hysics: {C}onference Series},
    Keywords = {ANTARES, WD, convection,zaussinger, DFG_DH},
    Number = {1},
    Pages = {012013},
    Publisher = {IOP Publishing},
    Title = {Numerical simulation of {DA} white dwarf surface convection},
    Url = {http://stacks.iop.org/1742-6596/1031/i=1/a=012013},
    Volume = {1031},
    Year = {2018},
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2017

  • V. Travnikov, F. Zaussinger, P. Beltrame, and C. Egbers, "Influence of the temperature-dependent viscosity on convective flow in the radial force field," Physical Review E, vol. 96, iss. 2, 2017.
    [BibTeX]
    @article{Travnikov_2017,
    Author = {Travnikov, V. and Zaussinger, F. and Beltrame, P. and Egbers, C.},
    Date-Added = {2017-08-30 08:03:20 +0000},
    Date-Modified = {2019-03-15 09:42:51 +0100},
    Issn = {2470-0053},
    Journal = {Physical {R}eview {E}},
    Keywords = {GEOFLOW,zaussinger},
    Month = {Aug},
    Number = {2},
    Publisher = {American Physical Society (APS)},
    Title = {Influence of the temperature-dependent viscosity on convective flow in the radial force field},
    Volume = {96},
    Year = {2017},
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  • F. Zaussinger, C. Egbers, A. Krebs, and V. Travnikov, "New results of the spherical convection experiment Geoflow IIc," in EGU general assembly conference abstracts, 2017, p. 7801.
    [BibTeX] [Download PDF]
    @inproceedings{Zaussinger_2017c,
    Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
    Adsurl = {http://adsabs.harvard.edu/abs/2017EGUGA..19.7801Z},
    Author = {Zaussinger, Florian and Egbers, Christoph and Krebs, Andreas and Travnikov, Vadim},
    Booktitle = {{EGU} General Assembly Conference Abstracts},
    Date-Added = {2018-07-31 15:55:53 +0200},
    Date-Modified = {2019-07-03 10:28:06 +0200},
    Keywords = {GEOFLOW,zaussinger},
    Month = apr,
    Pages = {7801},
    Series = {EGU General Assembly Conference Abstracts},
    Title = {{New results of the spherical convection experiment {G}eoflow {IIc}}},
    Url = {https://meetingorganizer.copernicus.org/EGU2017/EGU2017-7801.pdf},
    Volume = 19,
    Year = 2017,
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  • F. Zaussinger, C. Egbers, and A. Krebs, "The GeoFlow experiments on the ISS: Thermal convection under microgravity conditions," in Joint Conference ISPS-7 and ELGRA-25 October, 2-6 2017, Juan-les-Pins, France, Abstract book, 2017, p. S. 30.
    [BibTeX] [Download PDF]
    @inproceedings{Zaussinger_2017e,
    Author = {Zaussinger, Florian and Egbers, Christoph and Krebs, Andreas},
    Booktitle = {{Joint Conference ISPS-7 and ELGRA-25 October, 2-6 2017, Juan-les-Pins, France, Abstract book}},
    Date-Added = {2018-07-31 17:14:34 +0200},
    Date-Modified = {2019-07-03 10:40:40 +0200},
    Keywords = {GEOFLOW,zaussinger},
    Language = {en},
    Pages = {S. 30},
    Series = {Joint Conference ISPS-7 and ELGRA-25 October, 2-6 2017, Juan-les-Pins, France, Abstract book},
    Title = {{The GeoFlow experiments on the ISS: Thermal convection under microgravity conditions}},
    Url = {http://www.elgra.org/wp-content/uploads/2017/03/ISPS-7_ELGRA_25_2017_17A02-Abstract-book-final.pdf},
    Year = {2017},
    Bdsk-Url-1 = {http://www.elgra.org/wp-content/uploads/2017/03/ISPS-7_ELGRA_25_2017_17A02-Abstract-book-final.pdf}}

  • F. Zaussinger, A. Krebs, V. Travnikov, and C. Egbers, "Recognition and tracking of convective flow patterns using Wollaston shearing interferometry," Advances in Space Research, vol. 60, iss. 6, pp. 1327-1344, 2017. doi:https://doi.org/10.1016/j.asr.2017.06.028
    [BibTeX] [Download PDF]
    @article{Zaussinger_2017b,
    Author = {F. Zaussinger and A. Krebs and V. Travnikov and Ch. Egbers},
    Date-Added = {2017-10-06 10:20:07 +0000},
    Date-Modified = {2019-03-14 19:53:32 +0100},
    Doi = {https://doi.org/10.1016/j.asr.2017.06.028},
    Issn = {0273-1177},
    Journal = {Advances in {S}pace {R}esearch},
    Keywords = {GEOFLOW,zaussinger},
    Number = {6},
    Pages = {1327 - 1344},
    Title = {Recognition and tracking of convective flow patterns using {W}ollaston shearing interferometry},
    Url = {http://www.sciencedirect.com/science/article/pii/S0273117717304544},
    Volume = {60},
    Year = {2017},
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  • F. Zaussinger, F. Kupka, C. Egbers, M. Neben, S. Hücker, C. Bahr, and M. Schmitt, Semi-convective layer formation, 2017. doi:doi :10.1088/1742-6596/837/1/012012
    [BibTeX] [Abstract] [Download PDF]

    Semi-convective mixing, as an example of double-diffusive convection, is of general importance in multi-component fluid mixing processes. In astrophysics it occurs when the mean molecular weight gradient caused by a mixture of light material on top of heavier one counteracts the convective instability caused by a temperature gradient. Direct numerical simulations of double-diffusive fluid flows in a realistic stellar or planetary parameter space are currently non-feasible. Hence, a model describing incompressible semi-convection was developed, which allows to investigate semi-convective layer formation. A detailed parameter study with varying Rayleigh number and stability parameter has been performed for the giant planet case. We conclude that semi-convective layering may not play that important role as suggested in earlier works for the planetary case.

    @proceedings{Zaussinger_2017a,
    Abstract = {Semi-convective mixing, as an example of double-diffusive convection, is of general importance in multi-component fluid mixing processes. In astrophysics it occurs when the mean molecular weight gradient caused by a mixture of light material on top of heavier one counteracts the convective instability caused by a temperature gradient. Direct numerical simulations of double-diffusive fluid flows in a realistic stellar or planetary parameter space are currently non-feasible. Hence, a model describing incompressible semi-convection was developed, which allows to investigate semi-convective layer formation. A detailed parameter study with varying Rayleigh number and stability parameter has been performed for the giant planet case. We conclude that semi-convective layering may not play that important role as suggested in earlier works for the planetary case.},
    Author = {F. Zaussinger and F. Kupka and Ch. Egbers and M. Neben and S. H{\"u}cker and C. Bahr and M. Schmitt},
    Date-Added = {2017-06-14 18:14:27 +0000},
    Date-Modified = {2019-05-15 17:00:45 +0200},
    Doi = {doi :10.1088/1742-6596/837/1/012012},
    Journal = {Journal of {P}hysics: {C}onference Series},
    Keywords = {SC,DFG_DH},
    Number = {1},
    Pages = {012012},
    Title = {Semi-convective layer formation},
    Url = {http://stacks.iop.org/1742-6596/837/i=1/a=012012},
    Volume = {837},
    Year = {2017},
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2016

  • U. Harlander, I. Kirschner, C. Maas, and F. Zaussinger, "On the generation of internal wave modes by surface waves," in EGU general assembly conference abstracts, 2016, p. EPSC2016-14128.
    [BibTeX] [Download PDF]
    @inproceedings{Harlander_2016,
    Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
    Adsurl = {http://adsabs.harvard.edu/abs/2016EGUGA..1814128H},
    Author = {Harlander, Uwe and Kirschner, Ian and Maas, Christian and Zaussinger, Florian},
    Booktitle = {{EGU} General Assembly Conference Abstracts},
    Date-Added = {2018-07-31 15:56:41 +0200},
    Date-Modified = {2019-07-03 10:27:05 +0200},
    Eid = {EPSC2016-14128},
    Keywords = {Waves,zaussinger},
    Month = apr,
    Pages = {EPSC2016-14128},
    Series = {EGU General Assembly Conference Abstracts},
    Title = {{On the generation of internal wave modes by surface waves}},
    Url = {https://meetingorganizer.copernicus.org/EGU2016/EGU2016-14128.pdf},
    Volume = 18,
    Year = 2016,
    Bdsk-Url-1 = {https://meetingorganizer.copernicus.org/EGU2016/EGU2016-14128.pdf}}

  • M. M. B. F. A. K. Florian Zaussinger Christoph Egbers, Durchführung und Auswertung des Kugelspaltexperiments GeoFlow auf der Internationalen Raumstation (ISS) : Schlussbericht 50WM0822, {TIB Lebnitz-Infomrationszentrum Technik und Naturwissenschaften Universitätsbibliothek}, 2016. doi:10.2314/GBV:872395197
    [BibTeX]
    @book{Zaussinger_2016,
    Author = {Florian Zaussinger, Christoph Egbers, Martin Meier, Birgit Futterer, Andreas Krebs},
    Date-Added = {2018-08-20 18:14:53 +0200},
    Date-Modified = {2019-04-30 09:41:22 +0200},
    Doi = {10.2314/GBV:872395197},
    Keywords = {GEOFLOW,zaussinger},
    Publisher = {{TIB Lebnitz-Infomrationszentrum Technik und Naturwissenschaften Universit{\"a}tsbibliothek}},
    Series = {BKL: 38.70 Geophysik: Allgemeines / 50.93 Weltraumforschung},
    Title = {{Durchf{\"u}hrung und Auswertung des Kugelspaltexperiments GeoFlow auf der Internationalen Raumstation (ISS) : Schlussbericht 50WM0822}},
    Year = {2016},
    Bdsk-File-1 = {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},
    Bdsk-Url-1 = {https://doi.org/10.2314/GBV:872395197}}

  • C. Egbers and F. Zaussinger, "Simulation of geophysical fluid flows in spherical shells: the geoflow experiments on ISS," in Book of abstracts, school ISTROF 2016, Instabilities and turbulence in strato-rotational flows, july 11-13th, 2016, Le Havre, 2016.
    [BibTeX] [Download PDF]
    @inproceedings{Egbers_2016,
    Author = {Egbers, Christoph and Zaussinger, Florian},
    Booktitle = {Book of abstracts, School {ISTROF} 2016, {I}nstabilities and Turbulence in Strato-Rotational Flows, July 11-13th, 2016, {Le Havre}},
    Date-Added = {2018-07-31 17:11:12 +0200},
    Date-Modified = {2019-07-03 10:26:02 +0200},
    Keywords = {GEOFLOW,zaussinger},
    Language = {en},
    Series = {Book of abstracts, School ISTROF 2016, Instabilities and Turbulence in Strato-Rotational Flows, July 11-13th, 2016, Le Havre},
    Title = {Simulation of geophysical fluid flows in spherical shells: The Geoflow experiments on {ISS}},
    Url = {https://sites.google.com/site/schoolistrof/program},
    Year = {2016},
    Bdsk-Url-1 = {https://sites.google.com/site/schoolistrof/program}}

2015

  • F. Zaussinger, F. Kupka, S. Hücker, and C. Egbers, "Double-diffusive layer formation," in EGU general assembly conference abstracts, 2015, p. 3705.
    [BibTeX] [Download PDF]
    @inproceedings{Zaussinger_2015b,
    Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
    Adsurl = {http://adsabs.harvard.edu/abs/2015EGUGA..17.3705Z},
    Author = {Zaussinger, Florian and Kupka, Friedrich and H{\"u}cker, Sebastian and Egbers, Christoph},
    Booktitle = {{EGU} General Assembly Conference Abstracts},
    Date-Added = {2018-07-31 15:57:44 +0200},
    Date-Modified = {2019-07-03 10:33:49 +0200},
    Eid = {3705},
    Keywords = {SC,zaussinger},
    Month = apr,
    Pages = {3705},
    Series = {EGU General Assembly Conference Abstracts},
    Title = {{Double-diffusive layer formation}},
    Url = {https://meetingorganizer.copernicus.org/EGU2015/EGU2015-3705-1.pdf},
    Volume = 17,
    Year = 2015,
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  • F. Zaussinger, C. Egbers, A. Krebs, F. Schwarzbach, and C. Kunze, "Time-dependent convective flows with high viscosity contrasts under micro gravity conditions.," in EGU general assembly conference abstracts general assembly conference abstracts, 2015, p. 5833.
    [BibTeX] [Download PDF]
    @inproceedings{Zaussinger_2015,
    Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
    Adsurl = {http://adsabs.harvard.edu/abs/2015EGUGA..17.5833Z},
    Author = {Zaussinger, Florian and Egbers, Christoph and Krebs, Andreas and Schwarzbach, Felix and Kunze, Christian},
    Booktitle = {{EGU} General Assembly Conference Abstracts General Assembly Conference Abstracts},
    Date-Added = {2018-07-31 15:57:15 +0200},
    Date-Modified = {2019-07-03 10:31:56 +0200},
    Eid = {5833},
    Keywords = {GEOFLOW,zaussinger},
    Month = apr,
    Pages = {5833},
    Series = {EGU General Assembly Conference Abstracts},
    Title = {{Time-dependent convective flows with high viscosity contrasts under micro gravity conditions.}},
    Url = {https://meetingorganizer.copernicus.org/EGU2015/EGU2015-5833.pdf},
    Volume = 17,
    Year = 2015,
    Bdsk-Url-1 = {https://meetingorganizer.copernicus.org/EGU2015/EGU2015-5833.pdf}}

  • F. Zaussinger, A. Christl, P. Gorenz, M. Neben, and C. Egbers, "An applied couette-taylor system as a simplified bearing model," in Book of abstracts, ICTW 19, 19th International Couette-Taylor Workshop, June 24-26, 2015 Cottbus, Germany, Cottbus, 2015, p. 170 – 171.
    [BibTeX] [Download PDF]
    @inproceedings{Zaussinger_2015d,
    Address = {Cottbus},
    Author = {Zaussinger, Florian and Christl, Andreas and Gorenz, Paul and Neben, Matthias and Egbers, Christoph},
    Booktitle = {{Book of abstracts, ICTW 19, 19th International Couette-Taylor Workshop, June 24-26, 2015 Cottbus, Germany}},
    Date-Added = {2018-07-31 17:14:05 +0200},
    Date-Modified = {2019-07-03 10:38:48 +0200},
    Keywords = {Gleitlager,zaussinger},
    Language = {en},
    Pages = {170 -- 171},
    Publisher = {BTU},
    Series = {Book of abstracts, ICTW 19, 19th International Couette-Taylor Workshop, June 24-26, 2015 Cottbus, Germany},
    Title = {An applied Couette-Taylor system as a simplified bearing model},
    Url = {https://www.b-tu.de/fg-aerodynamik-stroemungslehre/aktuelles/tagungen/ictw-2015},
    Year = {2015},
    Bdsk-Url-1 = {https://www.b-tu.de/fg-aerodynamik-stroemungslehre/aktuelles/tagungen/ictw-2015}}

  • F. Zaussinger, A. Krebs, D. Breuer, A. Plesa, and C. Egbers, "Convection in the spherical gap with high viscosity contrasts," in ICTW 19, Book of Abstracts, 19th International Couette-Taylor Workshop, June 24 - 26, 2015 Cottbus, Germany, Cottbus, 2015, p. 88 – 89.
    [BibTeX] [Download PDF]
    @inproceedings{Zaussinger_2015c,
    Address = {Cottbus},
    Author = {Zaussinger, Florian and Krebs, Andreas and Breuer, Doris and Plesa, Ana-Catalina and Egbers, Christoph},
    Booktitle = {{ICTW 19, Book of Abstracts, 19th International Couette-Taylor Workshop, June 24 - 26, 2015 Cottbus, Germany}},
    Date-Added = {2018-07-31 17:13:34 +0200},
    Date-Modified = {2019-07-03 10:38:32 +0200},
    Keywords = {GEOFLOW,zaussinger},
    Language = {en},
    Pages = {88 -- 89},
    Series = {ICTW 19, Book of Abstracts, 19th International Couette-Taylor Workshop, June 24 - 26, 2015 Cottbus, Germany},
    Title = {Convection in the spherical gap with high viscosity contrasts},
    Url = {https://www.b-tu.de/fg-aerodynamik-stroemungslehre/aktuelles/tagungen/ictw-2015},
    Year = {2015},
    Bdsk-Url-1 = {https://www.b-tu.de/fg-aerodynamik-stroemungslehre/aktuelles/tagungen/ictw-2015}}

  • F. Kupka, M. Losch, F. Zaussinger, and T. Zweigle, "Semi-convection in the ocean and in stars: a multi-scale analysis," Meteorologische Zeitschrift, vol. 24, iss. 3, pp. 343-358, 2015. doi:10.1127/metz/2015/0643
    [BibTeX]
    @article{Kupka_2015,
    Author = {Kupka, F. and Losch, M. and Zaussinger, F. and Zweigle, T.},
    Date-Added = {2017-02-23 15:15:40 +0000},
    Date-Modified = {2019-03-15 09:42:22 +0100},
    Doi = {10.1127/metz/2015/0643},
    Journal = {Meteorologische {Z}eitschrift},
    Keywords = {SC,zaussinger},
    Number = {3},
    Pages = {343-358},
    Title = {Semi-convection in the ocean and in stars: A multi-scale analysis},
    Volume = {24},
    Year = {2015},
    Bdsk-File-1 = {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}}

  • H. Grimm-Strele, F. Kupka, B. Löw-Baselli, E. Mundprecht, F. Zaussinger, and P. Schiansky, "Realistic simulations of stellar surface convection with ANTARES: I. Boundary conditions and model relaxation," New Astronomy, vol. 34, pp. 278-293, 2015. doi:http://dx.doi.org/10.1016/j.newast.2013.11.005
    [BibTeX] [Abstract] [Download PDF]

    Abstract We have implemented open boundary conditions into the \{ANTARES\} code to increase the realism of our simulations of stellar surface convection. Even though we greatly benefit from the high accuracy of our fifth order numerical scheme (WENO5) the broader stencils needed for the numerical scheme complicate the implementation of boundary conditions. We show that the effective temperature of a numerical simulation cannot be changed by corrections at the lower boundary since the thermal stratification does only change on the Kelvin–Helmholtz time scale. Except for very shallow models this time scale cannot be covered by multidimensional simulations due to the enormous computational requirements. We demonstrate to what extent numerical simulations of stellar surface convection are sensitive to the initial conditions and the boundary conditions. An ill-conceived choice of parameters for the boundary conditions can have a severe impact. Numerical simulations of stellar surface convection will only be (physically) meaningful and realistic if the initial model, the extent and position of the simulation box and the parameters from the boundary conditions are chosen adequately.

    @article{Grimm_2015,
    Abstract = {Abstract We have implemented open boundary conditions into the \{ANTARES\} code to increase the realism of our simulations of stellar surface convection. Even though we greatly benefit from the high accuracy of our fifth order numerical scheme (WENO5) the broader stencils needed for the numerical scheme complicate the implementation of boundary conditions. We show that the effective temperature of a numerical simulation cannot be changed by corrections at the lower boundary since the thermal stratification does only change on the Kelvin--Helmholtz time scale. Except for very shallow models this time scale cannot be covered by multidimensional simulations due to the enormous computational requirements. We demonstrate to what extent numerical simulations of stellar surface convection are sensitive to the initial conditions and the boundary conditions. An ill-conceived choice of parameters for the boundary conditions can have a severe impact. Numerical simulations of stellar surface convection will only be (physically) meaningful and realistic if the initial model, the extent and position of the simulation box and the parameters from the boundary conditions are chosen adequately. },
    Author = {H. Grimm-Strele and F. Kupka and B. L{\"o}w-Baselli and E. Mundprecht and F. Zaussinger and P. Schiansky},
    Date-Added = {2017-01-18 17:30:45 +0000},
    Date-Modified = {2019-05-21 10:41:30 +0200},
    Doi = {http://dx.doi.org/10.1016/j.newast.2013.11.005},
    Issn = {1384-1076},
    Journal = {New {A}stronomy},
    Keywords = {ANTARES, DFG_DH, zaussinger},
    Pages = {278 - 293},
    Title = {Realistic simulations of stellar surface convection with {ANTARES}: {I}. {B}oundary conditions and model relaxation},
    Url = {http://www.sciencedirect.com/science/article/pii/S1384107613001383},
    Volume = {34},
    Year = {2015},
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2014

  • C. Egbers, B. Futterer, F. Zaussinger, and U. Harlander, "Simulation of large scale motions and small scale structures in planetary atmospheres and oceans: from laboratory to space experiments on ISS," in EGU general assembly conference abstracts, 2014, p. 16940.
    [BibTeX] [Download PDF]
    @inproceedings{Egbers_2014,
    Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
    Author = {Egbers, Christoph and Futterer, Birgit and Zaussinger, Florian and Harlander, Uwe},
    Booktitle = {{EGU} General Assembly Conference Abstracts},
    Date-Added = {2018-07-31 15:53:38 +0200},
    Date-Modified = {2019-07-03 10:24:00 +0200},
    Eid = {16940},
    Keywords = {GEOFLOW,zaussinger},
    Month = may,
    Pages = {16940},
    Series = {EGU General Assembly Conference Abstracts},
    Title = {Simulation of large scale motions and small scale structures in planetary atmospheres and oceans: From laboratory to space experiments on {ISS}},
    Url = {https://meetingorganizer.copernicus.org/EGU2014/EGU2014-16940.pdf},
    Volume = 16,
    Year = 2014,
    Bdsk-Url-1 = {https://meetingorganizer.copernicus.org/EGU2014/EGU2014-16940.pdf}}

2013

  • B. Futterer, A. Krebs, A. -C. Plesa, F. Zaussinger, R. Hollerbach, D. Breuer, and C. Egbers, "Sheet-like and plume-like thermal flow in a spherical convection experiment performed under microgravity," Journal of Fluid Mechanics, vol. 735, p. 647–683, 2013. doi:10.1017/jfm.2013.507
    [BibTeX] [Download PDF]
    @article{Futterer_2013,
    Abstractnote = {AbstractWe introduce, in spherical geometry, experiments on electro-hydrodynamic driven Rayleigh--B{\'e}nard convection that have been performed for both temperature-independent (``GeoFlow I'') and temperature-dependent fluid viscosity properties (``GeoFlow II'') with a measured viscosity contrast up to 1.5. To set up a self-gravitating force field, we use a high-voltage potential between the inner and outer boundaries and a dielectric insulating liquid; the experiments were performed under microgravity conditions on the International Space Station. We further run numerical simulations in three-dimensional spherical geometry to reproduce the results obtained in the ``GeoFlow'' experiments. We use Wollaston prism shearing interferometry for flow visualization -- an optical method producing fringe pattern images. The flow patterns differ between our two experiments. In ``GeoFlow I'', we see a sheet-like thermal flow. In this case convection patterns have been successfully reproduced by three-dimensional numerical simulations using two different and independently developed codes. In contrast, in ``GeoFlow II'', we obtain plume-like structures. Interestingly, numerical simulations do not yield this type of solution for the low viscosity contrast realized in the experiment. However, using a viscosity contrast of two orders of magnitude or higher, we can reproduce the patterns obtained in the ``GeoFlow II'' experiment, from which we conclude that nonlinear effects shift the effective viscosity ratio.},
    Author = {Futterer, B. and Krebs, A. and Plesa, A.-C. and Zaussinger, F. and Hollerbach, R. and Breuer, D. and Egbers, C.},
    Date-Added = {2017-01-12 14:56:54 +0000},
    Date-Modified = {2019-03-14 19:52:55 +0100},
    Doi = {10.1017/jfm.2013.507},
    Journal = {Journal of {F}luid {M}echanics},
    Keywords = {GEOFLOW,zaussinger},
    Month = {Nov},
    Pages = {647--683},
    Place = {Cambridge, UK},
    Publisher = {Cambridge University Press},
    Title = {Sheet-like and plume-like thermal flow in a spherical convection experiment performed under microgravity},
    Url = {https://www.cambridge.org/core/article/div-class-title-sheet-like-and-plume-like-thermal-flow-in-a-spherical-convection-experiment-performed-under-microgravity-div/32CFFF7061E5F96C8153453826DCFF55},
    Volume = {735},
    Year = {2013},
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  • B. Futterer, F. Zaussinger, A. Plesa, A. Krebs, C. Egbers, and D. Breuer, "Sheet-like and plume-like thermal flow in a spherical convection experiment with high viscosity contrast.," in EGU General Assembly Conference Abstracts, 2013, p. EGU2013-4830.
    [BibTeX]
    @inproceedings{Futterer_2013b,
    Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
    Adsurl = {http://adsabs.harvard.edu/abs/2013EGUGA..15.4830F},
    Author = {Futterer, Birgit and Zaussinger, Florian and Plesa, Ana-Catalina and Krebs, Andreas and Egbers, Christoph and Breuer, Doris},
    Booktitle = {{EGU General Assembly Conference Abstracts}},
    Date-Added = {2018-07-31 15:54:49 +0200},
    Date-Modified = {2019-03-14 19:58:06 +0100},
    Eid = {EGU2013-4830},
    Keywords = {GEOFLOW,zaussinger},
    Month = apr,
    Pages = {EGU2013-4830},
    Series = {EGU General Assembly Conference Abstracts},
    Title = {{Sheet-like and plume-like thermal flow in a spherical convection experiment with high viscosity contrast.}},
    Volume = 15,
    Year = 2013}

  • F. Zaussinger, F. Kupka, and H. Muthsam, "Studying stellar rotation and convection," , Lecture Notes in Physics Eds. M. Goupil et al., Ed., , 2013, vol. 865, pp. 219-237. doi:doi :10.1007/978-3-642-33380-4
    [BibTeX]
    @inbook{Zaussinger_2013b,
    Author = {Zaussinger, F. and Kupka, F. and Muthsam, H.},
    Chapter = {11, Semi-convection},
    Date-Added = {2017-02-23 15:19:33 +0000},
    Date-Modified = {2019-05-15 17:00:30 +0200},
    Doi = {doi :10.1007/978-3-642-33380-4},
    Editor = {Lecture Notes in Physics, Eds. M. Goupil et al.,},
    Keywords = {SC,DFG_DH},
    Pages = {219-237},
    Series = {Lecture Notes in Physics},
    Title = {Studying Stellar Rotation and Convection},
    Volume = {865},
    Year = {2013},
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  • F. Zaussinger and H. C. Spruit, "Semiconvection: numerical simulations," Astronomy and Astrophysics, vol. 554, p. A119, 2013. doi:10.1051/0004-6361/201220573
    [BibTeX] [Download PDF]
    @article{Zaussinger_2013a,
    Author = {Zaussinger, F. and Spruit, H. C.},
    Date-Added = {2017-01-18 17:32:54 +0000},
    Date-Modified = {2019-03-14 19:53:26 +0100},
    Doi = {10.1051/0004-6361/201220573},
    Journal = {Astronomy and {A}strophysics},
    Keywords = {SC,zaussinger},
    Pages = {A119},
    Title = {Semiconvection: numerical simulations},
    Url = {http://dx.doi.org/10.1051/0004-6361/201220573},
    Volume = 554,
    Year = 2013,
    Bdsk-File-1 = {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},
    Bdsk-Url-1 = {http://dx.doi.org/10.1051/0004-6361/201220573}}

  • D. {Breuer}, B. {Futterer}, A. {Plesa}, A. {Krebs}, F. {Zaussinger}, and C. {Egbers}, "Sheet-like and plume-like thermal flow in a spherical convection experiment performed under microgravity." 2013, p. NG23A-1481.
    [BibTeX]
    @inproceedings{Breuer_2013,
    Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
    Adsurl = {http://adsabs.harvard.edu/abs/2013AGUFMNG23A1481B},
    Author = {{Breuer}, D. and {Futterer}, B. and {Plesa}, A. and {Krebs}, A. and {Zaussinger}, F. and {Egbers}, C.},
    Date-Added = {2018-07-31 15:58:44 +0200},
    Date-Modified = {2019-03-14 19:50:47 +0100},
    Eid = {NG23A-1481},
    Journal = {{AGU} Fall Meeting Abstracts},
    Keywords = {zaussinger,GEOFLOW},
    Month = dec,
    Pages = {NG23A-1481},
    Title = {{Sheet-like and plume-like thermal flow in a spherical convection experiment performed under microgravity}},
    Year = 2013}

2012

  • F. Zaussinger, B. Futterer, and C. Egbers, Non-linear effects in a spherical convection experiments with temperature dependent fluid properties: Microgravity experiment and numerical simulations, 2012.
    [BibTeX]
    @proceedings{Zaussinger_2012,
    Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
    Adsurl = {http://adsabs.harvard.edu/abs/2012AGUFMNG51D1795Z},
    Author = {Zaussinger, F. and Futterer, B. and Egbers, Ch.},
    Date-Added = {2018-07-31 16:00:16 +0200},
    Date-Modified = {2019-03-14 19:55:38 +0100},
    Eid = {NG51D-1795},
    Journal = {{AGU} Fall Meeting Abstracts},
    Keywords = {GEOFLOW,zaussinger},
    Month = dec,
    Pages = {NG51D-1795},
    Title = {{Non-linear effects in a spherical convection experiments with temperature dependent fluid properties: Microgravity experiment and numerical simulations}},
    Year = 2012,
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  • F. Zaussinger, A. Plesa, C. Egbers, and D. Breuer, "Mantle Convection in a Spherical Shell: Comparison of Numerical Simulations with the GeoFlow Experiment on the ISS," in EGU general assembly conference abstracts, 2012, p. 9939.
    [BibTeX]
    @inproceedings{Zaussinger_2012b,
    Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
    Adsurl = {http://adsabs.harvard.edu/abs/2012EGUGA..14.9939Z},
    Author = {Zaussinger, Florian and Plesa, Ana-Catalina and Egbers, Christoph and Breuer, Doris},
    Booktitle = {{EGU} General Assembly Conference Abstracts},
    Date-Added = {2018-07-31 16:00:54 +0200},
    Date-Modified = {2019-03-14 19:57:17 +0100},
    Editor = {{Abbasi}, A. and {Giesen}, N.},
    Keywords = {GEOFLOW,zaussinger},
    Month = apr,
    Pages = {9939},
    Series = {EGU General Assembly Conference Abstracts},
    Title = {{Mantle Convection in a Spherical Shell: Comparison of Numerical Simulations with the GeoFlow Experiment on the ISS}},
    Volume = 14,
    Year = 2012}

  • B. Futterer, F. Zaussinger, and C. Egbers, "Geophysical Fluid Dynamics in Space: spherical convection with low viscosity contrasts," in EGU general assembly conference abstracts, 2012, p. 7782.
    [BibTeX]
    @inproceedings{Futterer_2012b,
    Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
    Adsurl = {http://adsabs.harvard.edu/abs/2012EGUGA..14.7782F},
    Author = {Futterer, Birgit and Zaussinger, Florian and Egbers, Christoph},
    Booktitle = {{EGU} General Assembly Conference Abstracts},
    Date-Added = {2018-07-31 16:01:31 +0200},
    Date-Modified = {2019-03-14 19:58:12 +0100},
    Editor = {{Abbasi}, A. and {Giesen}, N.},
    Keywords = {GEOFLOW,zaussinger},
    Month = apr,
    Pages = {7782},
    Series = {EGU General Assembly Conference Abstracts},
    Title = {{Geophysical Fluid Dynamics in Space: spherical convection with low viscosity contrasts}},
    Volume = 14,
    Year = 2012}

2011

  • F. Zaussinger, "Semiconvection," in EGU general assembly conference abstracts, 2011, p. 2590.
    [BibTeX]
    @inproceedings{Zaussinger_2011c,
    Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
    Author = {Zaussinger, Florian},
    Booktitle = {{EGU} General Assembly Conference Abstracts},
    Date-Modified = {2019-03-14 19:57:23 +0100},
    Keywords = {SC,zaussinger},
    Pages = {2590},
    Series = {EGU General Assembly Conference Abstracts},
    Title = {{Semiconvection}},
    Volume = 13,
    Year = 2011,
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  • B. Futterer, F. Zaussinger, C. Egbers, and N. Scurtu, "Variation of viscosity contrast for convection experiments in spherical shells as part of geophysical flow simulation experiment GeoFlow II," in EGU general assembly conference abstracts, 2011, p. 5562.
    [BibTeX]
    @inproceedings{Zaussinger_2011b,
    Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
    Author = {Futterer, Birgit and Zaussinger, Florian and Egbers, Christoph and Scurtu, Nicoleta},
    Booktitle = {{EGU} General Assembly Conference Abstracts},
    Date-Modified = {2019-03-14 19:57:29 +0100},
    Keywords = {GEOFLOW,zaussinger},
    Pages = {5562},
    Series = {EGU General Assembly Conference Abstracts},
    Title = {Variation of viscosity contrast for convection experiments in spherical shells as part of geophysical flow simulation experiment {GeoFlow II}},
    Volume = 13,
    Year = 2011}

  • F. Zaussinger, "Numerical simulation of double-diffusive convection," PhD Thesis, 2011.
    [BibTeX] [Download PDF]
    @phdthesis{Zaussinger_2011,
    Author = {Zaussinger, F.},
    Date-Added = {2017-03-07 19:36:14 +0000},
    Date-Modified = {2019-04-03 13:47:18 +0200},
    Keywords = {SC, DFG_DH},
    School = {{Univ. Vienna}},
    Title = {Numerical simulation of double-diffusive convection},
    Url = {https://othes.univie.ac.at/13172/},
    Year = {2011},
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  • N. Happenhofer, O. Koch, F. Kupka, and F. Zaussinger, Total variation diminishing implicit Runge-Kutta methods for dissipative advection-diffusion problems in astrophysicsPAMM · Proc. Appl. Math. Mech., 2011. doi:10.1002/pamm.201110377
    [BibTeX] [Abstract] [Download PDF]

    Abstract We investigate the properties of dissipative full discretizations for the equations of motion associated with models of flow and radiative transport inside stars. We derive dissipative space discretizations and demonstrate that together with specially adapted total-variation-diminishing (TVD) or strongly stable Runge-Kutta time discretizations with adaptive step-size control this yields reliable and efficient integrators for the underlying high-dimensional nonlinear evolution equations. For the most general problem class, fully implicit SDIRK methods are demonstrated to be competitive when compared to popular explicit Runge-Kutta schemes as the additional effort for the solution of the associated nonlinear equations is compensated by the larger step-sizes admissible for strong stability and dissipativity. For the parameter regime associated with semiconvection we can use partitioned IMEX Runge-Kutta schemes, where the solution of the implicit part can be reduced to the solution of an elliptic problem. This yields a significant gain in performance as compared to either fully implicit or explicit time integrators. ({\copyright} 2011 Wiley-VCH Verlag GmbH & Co. KGaA, Weinheim)

    @proceedings{Happenhofer_2011,
    Abstract = {Abstract We investigate the properties of dissipative full discretizations for the equations of motion associated with models of flow and radiative transport inside stars. We derive dissipative space discretizations and demonstrate that together with specially adapted total-variation-diminishing (TVD) or strongly stable Runge-Kutta time discretizations with adaptive step-size control this yields reliable and efficient integrators for the underlying high-dimensional nonlinear evolution equations. For the most general problem class, fully implicit SDIRK methods are demonstrated to be competitive when compared to popular explicit Runge-Kutta schemes as the additional effort for the solution of the associated nonlinear equations is compensated by the larger step-sizes admissible for strong stability and dissipativity. For the parameter regime associated with semiconvection we can use partitioned IMEX Runge-Kutta schemes, where the solution of the implicit part can be reduced to the solution of an elliptic problem. This yields a significant gain in performance as compared to either fully implicit or explicit time integrators. ({\copyright} 2011 Wiley-VCH Verlag GmbH \& Co. KGaA, Weinheim)},
    Author = {Happenhofer, Natalie and Koch, Othmar and Kupka, Friedrich and Zaussinger, Florian},
    Date-Added = {2018-07-31 14:34:04 +0200},
    Date-Modified = {2019-03-14 19:55:31 +0100},
    Doi = {10.1002/pamm.201110377},
    Eprint = {https://onlinelibrary.wiley.com/doi/pdf/10.1002/pamm.201110377},
    Journal = {PAMM},
    Keywords = {ANTARES,zaussinger},
    Number = {11},
    Pages = {777-778},
    Publisher = {PAMM · Proc. Appl. Math. Mech.},
    Title = {Total Variation Diminishing Implicit {R}unge-{K}utta Methods for Dissipative Advection-Diffusion Problems in Astrophysics},
    Url = {https://onlinelibrary.wiley.com/doi/abs/10.1002/pamm.201110377},
    Volume = {11},
    Year = {2011},
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  • B. Futterer, F. Zaussinger, C. Egbers, and N. Scurtu, "Variation of viscosity contrast for convection experiments in spherical shells as part of geophysical flow simulation experiment GeoFlow II," in EGU general assembly conference abstracts, 2011, p. 5562.
    [BibTeX]
    @inproceedings{Futterer_2011,
    Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
    Author = {Futterer, Birgit and Zaussinger, Florian and Egbers, Christoph and Scurtu, Nicoleta},
    Booktitle = {{EGU} General Assembly Conference Abstracts},
    Date-Added = {2018-07-31 17:03:39 +0200},
    Date-Modified = {2019-03-14 19:58:17 +0100},
    Keywords = {GEOFLOW,zaussinger},
    Pages = {5562},
    Series = {EGU General Assembly Conference Abstracts},
    Title = {Variation of viscosity contrast for convection experiments in spherical shells as part of geophysical flow simulation experiment {GeoFlow II}},
    Volume = 13,
    Year = 2011,
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2010

  • F. Zaussinger, "Numerical simulation of double-diffusive convection.," in EGU general assembly conference abstracts, 2010, p. 4874.
    [BibTeX]
    @inproceedings{Zaussinger_2010,
    Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
    Adsurl = {http://adsabs.harvard.edu/abs/2010EGUGA..12.4874Z},
    Author = {Zaussinger, Florian},
    Booktitle = {{EGU} General Assembly Conference Abstracts},
    Date-Added = {2018-07-31 16:03:02 +0200},
    Date-Modified = {2019-03-14 19:57:35 +0100},
    Keywords = {SC,zaussinger},
    Month = may,
    Pages = {4874},
    Series = {EGU General Assembly Conference Abstracts},
    Title = {{Numerical simulation of double-diffusive convection.}},
    Volume = 12,
    Year = 2010}

  • H. ~J. Muthsam, F. Kupka, E. Mundprecht, F. Zaussinger, H. Grimm-Strele, and N. Happenhofer, "Simulations of stellar convection, pulsation and semiconvection," in Astrophysical Dynamics: From Stars to Galaxies, 2010. doi:doi:10.1017/S1743921311017595
    [BibTeX]
    @inproceedings{Muthsam_2010b,
    Author = {Muthsam, H.~J. and Kupka, F. and Mundprecht, E. and Zaussinger, F. and Grimm-Strele, H. and Happenhofer, N.},
    Booktitle = {{Astrophysical Dynamics: From Stars to Galaxies}},
    Date-Added = {2017-05-09 04:49:17 +0000},
    Date-Modified = {2019-03-14 19:57:42 +0100},
    Doi = {doi:10.1017/S1743921311017595},
    Journal = {IAU Symposium 271},
    Keywords = {ANTARES,zaussinger},
    Title = {Simulations of stellar convection, pulsation and semiconvection},
    Year = {2010},
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  • O. Koch, F. Kupka, B. Löw-Baselli, A. Mayrhofer, and F. Zaussinger, "SDIRK methods for the ANTARES code," ASC, 32, 2010.
    [BibTeX] [Download PDF]
    @techreport{Koch_2010,
    Author = {Koch, Othmar and Kupka, Friedrich and L{\"o}w-Baselli, Bernhard and Mayrhofer, A and Zaussinger, F},
    Date-Added = {2018-07-31 14:38:10 +0200},
    Date-Modified = {2019-03-14 19:56:08 +0100},
    Institution = {ASC},
    Keywords = {ANTARES,zaussinger},
    Number = {32},
    Title = {{SDIRK} Methods for the {ANTARES} Code},
    Url = {http://www.asc.tuwien.ac.at/preprint/2010/asc32x2010.pdf},
    Year = {2010},
    Bdsk-File-1 = {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}}

2009

  • F. Kupka, H. Muthsam, F. Zaussinger, H. Grimm-Strele, N. Happenhofer, B. Löw-Baselli, E. Mundprecht, and C. Obertscheider, "Solar surface flow simulations at ultra-high resolution," in High Performance Computing in Science and Engineering, 2009. doi:10.1007/978-3-642-13872-0
    [BibTeX]
    @inproceedings{Kupka_2009b,
    Author = {Kupka, Friedrich and Muthsam, Herbert and Zaussinger, Florian and Grimm-Strele, Hannes and Happenhofer, Natalie and L{\"o}w-Baselli, Bernhard and Mundprecht, Eva and Obertscheider, Christoph},
    Booktitle = {{H}igh {P}erformance {C}omputing in {S}cience and {E}ngineering},
    Date-Added = {2018-07-31 15:29:19 +0200},
    Date-Modified = {2019-04-01 12:52:25 +0200},
    Doi = {10.1007/978-3-642-13872-0},
    Editor = {Wagner, S., Steinmetz, M., Bode, A., Mueller, M.M.},
    Keywords = {ANTARES, stellar convection,zaussinger,DFG_DH},
    Series = {Transactions of the Fourth Joint {HLRB} and {KONWIHR} Review and Results Workshop, {D}ec. 8-9, 2009, {L}eibniz {S}upercomputing {C}entre, {G}arching/{M}unich, {G}ermany},
    Title = {Solar surface flow simulations at ultra-high resolution},
    Year = {2009},
    Bdsk-Url-1 = {https://doi.org/10.1007/978-3-642-13872-0}}

  • N. Happenhofer, H. Grimm-Strele, O. Koch, F. Kupka, H. Muthsam, and F. Zaussinger, "Simulation of low mach number flows." 2009, p. 31.
    [BibTeX]
    @inproceedings{Happenhofer_2009,
    Author = {Happenhofer, Natalie and Grimm-Strele, Hannes and Koch, Othmar and Kupka, Friedrich and Muthsam, Herbert and Zaussinger, Florian},
    Date-Added = {2018-07-31 15:50:11 +0200},
    Date-Modified = {2019-03-14 19:58:00 +0100},
    Keywords = {ANTARES,zaussinger},
    Pages = {31},
    Series = {5TH EUROPEAN POSTGRADUATE FLUID DYNAMICS CONFERENCE},
    Title = {Simulation of Low Mach Number Flows},
    Year = {2009},
    Bdsk-File-1 = {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}}