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Correlation heights of the sources of solar ultraviolet emission lines in a quiet-sun region. Astrophysical Journal 62.
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Solar wind origin in coronal funnels. Science 63.
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Electron density along a coronal loop observed with CDS/SOHO. Astronomy and Astrophysics 64.
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110, S. A10102 (2005)
Solar activity, cosmic rays and Earth's temperature: A millenium-scale comparison. Journal Geophysical Research 65.
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Quasiadiabatic description of nonlinear particle dynamics in typical magnetotail configurations. Nonlinear Processes in Geophysics 66.
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76, S. 842 - 849 (2005)
On the effect of photospheric magnetic fields on solar surface brightness: Results of radiative MHD simulations. Memorie della Societa Astronomica Italiana 67.
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Simulations of magneto-convection in the solar photosphere: Equations, methods and results of the MURaM code. Astronomy and Astrophysics 68.
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Jovian plasma sheet morphology: particle and field observations by the Galileo spacecraft. Planetary and Space Science 69.
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Initiation of hot coronal loop oscillations: Spectral features. Astronomy and Astrophysics 70.
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Can surface magnetic fields reproduce solar irradiance variations in cycles 22 and 23? Astronomy and Astrophysics 71.
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How to use magnetic field information for coronal loop identification. Solar Physics 72.
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Comparing magnetic field extrapolations with measurements of magnetic loops. Astronomy and Astrophysics 73.
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432, S. L1 - L4 (2005)
Links between magnetic fields and plasma flows in a coronal hole. Astronomy and Astrophysics 74.
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435, S. 733 - 741 (2005)
The widths of vacuum-ultraviolet spectral lines in the equatorial solar corona observed with CDS and SUMER. Astronomy and Astrophysics 75.
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On the nature of the unidentified solar emission near 117 nm. Astronomy and Astrophysics 76.
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Time series study of EUV spicules observed by SUMER/SOHO. Astronomy and Astrophysics 77.
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A comparative study of the contrast of solar magnetic elements in CN and CH. Astronomy and Astrophysics 78.
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The Second Solar Spectrum - A high spectral resolution polarimetric survey of scattering polarization near the solar limb in graphical representation. Vol. III: 3160 Ã… to 3915 Ã…. vdf, Zürich (2005), 188 S.
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Plasma acceleration due to transition region reconnection. In: Particle acceleration in astrophysical plasmas: Geospace and beyond, S. 161 - 170 (Hg. Horwitz, J. L.; Perez, J. D.; Preece, R. D.; Queenby, J.). American Geophysical Union (2005)