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Comment on ``Millennium scale sunspot number reconstruction: Evidence for an unusually active Sun since the 1940s'' - Reply. Physical Review Letters 62.
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Effects of non-grey radiative transfer on 3D simulations of solar magneto-convection. Astronomy and Astrophysics 63.
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421, pp. 741 - 754 (2004)
Approximations for non-grey radiative transfer in numerical simulations of the solar photosphere. Astronomy and Astrophysics 64.
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421, pp. L33 - L36 (2004)
Vertical oscillations of a coronal loop observed by TRACE. Astronomy and Astrophysics 65.
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427 (3), pp. 1031 - 1043 (2004)
Comparison between KPVT/SPM and SoHO/MDI magnetograms with an application to solar irradiance reconstructions. Astronomy and Astrophysics 66.
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Optimization code with weighting function for the reconstruction of coronal magnetic fields. Solar Physics 67.
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Similarities and differences between coronal holes and the quiet sun: are loop statistics the key? Solar Physics 68.
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Observations of the Sun at vacuum-ultraviolet wavelengths from space. Part I: Concepts and instrumentation. Space Science Reviews 69.
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On the widths of the Mg X lines near 60 nm in the corona. Astronomy and Astrophysics 70.
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The structure and dynamics of the Jovian energetic particle distribution. Advances in Space Research 71.
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On the network structures in solar equatorial coronal holes - Observations of SUMER and MDI on SOHO. Astronomy and Astrophysics Book Chapter (6)
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Simulation of solar magneto-convection. In: High Performance Computing in Science and Engineering: Transactions of the Second Joint HLRB and KONWIHR Result and Reviewing Workshop, pp. 431 - 442 (Eds. Wagner, S.; Hanke, W.; Bode, A.; Durst, F.). Springer, Berlin (2004)
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Waves and turbulence in the solar corona. In: The Sun and the Heliosphere as an Integrated System, pp. 283 - 317 (Eds. Poletto, G.; Suess, S. T.). Kluwer Academic Publishers, Dordrecht, The Netherlands (2004)
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The magnetic field from the solar interior to the heliosphere. In: The Sun and the Heliosphere as an Integrated System, pp. 373 - 395 (Eds. Poletto, G.; Suess, S. T.). Kluwer, Dordrecht (2004)
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Signature of current sheets as seen by TIP at VTT in the HeI multiplet at 1083.0 nm. In: Proc. SOHO 15 `Coronal Heating', pp. 593 - 596 (Eds. Walsh, R. W.; Ireland, J.; Danesy, D.; Fleck, B.). ESA Publ. Div., Noordwijk (2004)
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Probability analysis of coincident blinkers and explosive events. In: Proc. SOHO 15 - Coronal heating, pp. 465 - 470 (Eds. Walsh, R. W.; Ireland, J.; Danesy, D.; Fleck, B.). ESA Publ. Div., Noordwijk (2004)
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Magnetic coupling of photosphere and corona: MHD simulation for multi-wavelength observations. In: Multi-Wavelength Investigations of Solar Activity, pp. 353 - 356 (Eds. Stepanov, A. V.; Benevolenskaya, E. E.; Kosovichev, A. G.). Cambridge University Press, Cambridge, UK (2004)