Tipo de publicación: Sin árbitro

  • Publicación
    Solar p-mode frequencies
    Mathematical formulas derived from solar p-mode frequencies not only accurately reproduce observed frequencies, but extrapolate them to limits beyond current...
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    Solar P-Mode Frequencies from the IRIS Network
    Not Available
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    Solar Polarization
    Not Available
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    Solar Polarization Workshop 6
    Not Available
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    Solar Radar Astronomy with LOFAR
    A new approach to the study of the Sun's corona and its dynamical processes is possible with radar investigations in the frequency range of about 10-50 MHz. The...
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    Solar radius variations using LOI-T guiding pixels
    The LOI (Luminosity Oscillations Imager) is a low resolution solar photometer built at the SSD of ESA. It is one of the instruments in the VIRGO experiment on...
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    Solar research with stratospheric balloons
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    Solar research with stratospheric balloons
    Balloons, driven by hot air or some gas lighter than air, were the first artificial machines able to lift payloads (including humans) from the ground. After...
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    Solar Rotation Near the Surface: The Outer 1%
    We present an estimate of the solar rotation rate near the surface (i.e., the outer 1%) based on rotational splittings estimated for high degree modes ( ) from...