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496 (2), S. 469 - 473 (2009)
The planet-hosting subdwarf B star V 391 Pegasi is a hybrid pulsator. Astronomy and Astrophysics 442.
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496 (2), S. 469 - 473 (2009)
The planet-hosting subdwarf B star V 391 Pegasi is a hybrid pulsator. Astronomy and Astrophysics 443.
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504, S. 1041 - 1055 (2009)
Modelling of solar mesogranulation. Astronomy and Astrophysics 444.
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506, S. 875 - 884 (2009)
Large-scale horizontal flows in the solar photosphere V: Possible evidence for the disconnection of bipolar sunspot groups from their magnetic roots. Astronomy and Astrophysics 445.
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25, 075002 (2008)
1+1+2 Electromagnetic perturbations on non-vacuum LRS class II space-times: Decoupling scalar and 2-vector harmonic amplitudes. Class. Quantum Grav. 446.
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25, 075004 (2008)
1+1+2 Gravitational perturbations on LRS class II space-times: Decoupling gravito-electromagnetic tensor harmonic amplitudes. Class. Quantum Grav. 447.
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25, 235004 (2008)
1+1+2 gravitational perturbations on LRS class II spacetimes: II. Decoupling gravito-electromagnetic 2-vector and scalar harmonic amplitudes. Class. Quantum Grav. 448.
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German Data Center for the Solar Dynamics Observatory: A model for the PLATO mission? Communications in Asteroseismology 449.
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25, 075003 (2008)
1+1+2 Electromagnetic perturbations on general LRS space-times: Regge-Wheeler and Bardeen-Press equations. Class. Quantum Grav. 450.
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251, S. 291 - 308 (2008)
Helioseismology of sunspots: Confronting observations with three-dimensional MHD simulations of wave propagation. Solar Physics 451.
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251, S. 1 - 2 (2008)
Preface. Solar Physics 452.
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251, S. 241 - 250 (2008)
Observation and modeling of the solar-cycle variation of the meridional flow. Solar Physics 453.
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118, 011004 (2008)
Special session. J. Phys.: Conf. Ser. 454.
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118, 011003 (2008)
Abstract book. J. Phys.: Conf. Ser. 455.
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118, 011002 (2008)
Interactive conference picture. J. Phys.: Conf. Ser. 456.
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118, 011001 (2008)
Foreword. J. Phys.: Conf. Ser. 457.
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f-mode interactions with thin flux tubes: the scattering matrix. Astrophysical Journal 458.
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Structure and evolution of supergranulation from local helioseismology. Solar Physics 459.
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High-resolution mapping of flows in the solar interior: Fully consistent OLA inversion of helioseismic travel times. Solar Physics 460.
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118, 012033 (2008)
The forward and inverse problems in time-distance helioseismology. J. Phys.: Conf. Ser.