Journal: Solar Physics

  • Publication
    First Results on it P Modes from GOLF Experiment
    The GOLF experiment on the SOHO mission aims to study the internal structure of the Sun by measuring the spectrum of global oscillations in the frequency range...
  • Publication
    First View of the Solar Core from GOLF Acoustic Modes
    After 8 months of nearly continuous measurements the GOLF instrument, aboard SOHO, has detected acoustic mode frequencies of more than 100 modes, extending from...
  • Publication
    Global Oscillations at Low Frequency from the SOHO Mission (GOLF)
    The GOLF experiment on the SOHO mission aims to study the internal structure of the sun by measuring the spectrum of global oscillations in the frequency range...
  • Publication
    High-resolution Observations of Hα Spectra with a Subtractive Double Pass
    High-resolution imaging spectroscopy in solar physics has relied on Fabry-Pérot interferometers (FPIs) in recent years. FPI systems, however, become technically...
  • Publication
    In-Flight Performance of the Virgo Luminosity Oscillations Imager Aboard SOHO
    Not Available
  • Publication
    In-Flight Performance of the Virgo Solar Irradiance Instruments on SOHO
    The in-flight performance of the total and spectral irradiance instruments within VIRGO (Variability of solar IRradiance and Gravity Oscillations) on the ESA...
  • Publication
    Inference of Solar Magnetic Field Parameters from Data with Limited Wavelength Sampling
    We investigate the diagnostic potential of polarimetric measurements with filtergraph instruments. Numerical simulations are used to explore the possibility of...
  • Publication
    Influence of Low-Degree High-Order p-Mode Splittings on the Solar Rotation Profile
    The solar rotation profile is well constrained down to about 0.25 R &sun; thanks to the study of acoustic modes. Since the radius of the inner turning point of...
  • Publication
    Is the Solar Core Rotating Faster of Slower Than the Envelope?
    The Sun is not a rigid body and it is well known that its surface rotation is differential, the polar regions rotating substantially slower than the equator...