@ARTICLE{2004A&A...420..737K,
       author = {{Kolesnikov}, F. and {B{\"u}nte}, M. and {Schmitt}, D. and {Sch{\"u}ssler}, M.},
        title = "Kelvin-Helmholtz and shear instability of a helical flow around a magnetic flux tube",
      journal = {\aap},
         year = 2004,
       volume = {420},
        pages = {737-749},
          doi = {10.1051/0004-6361:20041040},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2004A&A...420..737K},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
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@ARTICLE{1994A&A...283..642B,
       author = {{B{\"{u}}nte}, M. and {Bogdan}, T.~J.},
        title = "Magneto-atmospheric waves subject to Newtonian cooling",
      journal = {\aap},
         year = 1994,
       volume = {283},
       number = {2},
        pages = {642-649},
       adsurl = {https://ui.adsabs.harvard.edu/abs/1994A&A...283..642B},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@INPROCEEDINGS{1994smf..conf..179B,
       author = {{B{\"u}nte}, M. and {Solanki}, S.~K.},
        title = "Surface waves: Origin of the Evershed phenomenon?",
    booktitle = {Solar Magnetic Fields},
         year = 1994,
       editor = {{Sch{\"u}ssler}, Manfred and {Schmidt}, Wolfgang},
        pages = {179},
       adsurl = {https://ui.adsabs.harvard.edu/abs/1994smf..conf..179B},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@INPROCEEDINGS{1994IAUS..154..459B,
       author = {{B{\"{u}}nte}, M. and {Steiner}, O. and {Solanki}, S.~K. and {Pizzo}, V.~J.},
        title = "Flux Tube Shredding Its Infrared Signature",
    booktitle = {Infrared Solar Physics},
         year = 1994,
       editor = {{Rabin}, D.~M. and {Jefferies}, John T. and {Lindsey}, C.},
       volume = {154},
        pages = {459},
       adsurl = {https://ui.adsabs.harvard.edu/abs/1994IAUS..154..459B},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{1993A&A...276..236B,
       author = {{B{\"{u}}nte}, M.},
        title = "On the interchange instability of solar magnetic flux tubes. Ill. The influence of the magnetic field geometry",
      journal = {\aap},
         year = 1993,
       volume = {276},
        pages = {236},
       adsurl = {https://ui.adsabs.harvard.edu/abs/1993A&A...276..236B},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{1993A&A...274..478B,
       author = {{B{\"{u}}nte}, M. and {Darconza}, G. and {Solanki}, S.~K.},
        title = "Surface waves as the origin of the Evershed phenomenon",
      journal = {\aap},
         year = 1993,
       volume = {274},
        pages = {478},
       adsurl = {https://ui.adsabs.harvard.edu/abs/1993A&A...274..478B},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{1993A&A...273..287B,
       author = {{B{\"{u}}nte}, M. and {Hasan}, S. and {Kalkofen}, W.},
        title = "On the interchange instability of solar magnetic flux tubes. II. The influence of energy transport effects",
      journal = {\aap},
         year = 1993,
       volume = {273},
        pages = {287},
       adsurl = {https://ui.adsabs.harvard.edu/abs/1993A&A...273..287B},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{1993A&A...271..167B,
       author = {{B{\"{u}}nte}, M. and {Saar}, S.~H.},
        title = "The interchange instability of stellar magnetic flux tubes",
      journal = {\aap},
         year = 1993,
       volume = {271},
        pages = {167},
       adsurl = {https://ui.adsabs.harvard.edu/abs/1993A&A...271..167B},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@INPROCEEDINGS{1991sopo.work..468B,
       author = {{B{\"u}nte}, M. and {Steiner}, O. and {Solanki}, S.~K.},
        title = "Center-to-limb variation of the Stokes V asymmetry in solar magnetic flux tubes.",
    booktitle = {Solar Polarimetry},
         year = 1991,
       editor = {{November}, L.~J.},
        pages = {468-478},
       adsurl = {https://ui.adsabs.harvard.edu/abs/1991sopo.work..468B},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


