Tipo de publicación: Sin árbitro

  • Publicación
    Progress Report: Probabilistic and Statistical Bases of Surface Brightness Fluctuations
    The surface brightness fluctuations (SBF) method is a statistical method applied on image pixels in different bands. This contribution aims to distinguish...
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    Progress Toward an IRIS++ Database Open to the Helioseismological Community
    The IRIS network is now fourteen years old, and has continuously been taking data since 1989. The data analysis, which produced some noticeable scientifical...
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    Project Cassini - A potential collaborative ESA/NASA Saturn Orbiter and Titan Probe mission
    Project Cassini is concerned with a potential collaborative mission to Saturn and Titan. The project has been the subject of a joint ESA/NASA Technical...
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    Project overview and update on WEAVE: the next generation wide-field spectroscopy facility for the William Herschel Telescope
    We present an overview of and status report on the WEAVE next-generation spectroscopy facility for the William Herschel Telescope (WHT). WEAVE principally...
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    Projected Rotational Velocities in Galactic OB Stars of Different OB Associations
    Not Available
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    Prominence Seismology
    Given the difficulty in directly determining prominence physical parameters from observations, prominence seismology stands as an alternative method to probe...
  • Publicación
    Prominence seismology using ground- and space-based observations
    Ground- and space-based observations have confirmed the presence of oscillatory motions in prominences and they have been interpreted in terms of...
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    Prompt Comparison of Data for Optical Transients of Gamma-Ray Bursts
    The prompt information given by the GRB Coordinates Network (GCN) differs very much for different GRBs. We compare the optical magnitudes quoted in GCNs for...
  • Publicación
    Propagating Waves Transverse to the Magnetic Field in a Solar Prominence
    We have observed a quiescent prominence with the Hinode Solar Optical Telescope (SOT, in Ca II and H-alpha lines), Sacramento Peak Observatory (in H-alpha, H...