Tipo de publicación: Sin árbitro

  • Publicación
    Comparison of Magnetoconvection Simulations with the Approximation of Thin Flux Tubes
    The structure and dynamics of small vertical photospheric magnetic flux concentrations has been often treated in the framework of an approximation based upon a...
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    Comparison of NIR and Hα emission from the HII regions of M100
    We measure the flux values in the 4 Spitzer-IRAC bands, of a sample of 78 isolated luminous HII regions in the grand design galaxy M100. We estimate the near-IR...
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    Comparison Of Observations And Advanced Numerical Simulations Of Type II Spicules
    We have performed realistic 3D radiation MHD simulations of the solar atmosphere. These simulations show jet-like features that are similar to the type II...
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    Comparison of On-Off and Wobble mode observations for MAGIC
    Not Available
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    Comparison of parameters of low l solar p-modes at maximum and minimum activity
    Velocity measurements of disk integrated sunlight obtained by GOLF experiment aboard SOHO are used to find the parameters of solar p-modes (l
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    Comparison of Reconstruction and Control algorithms on the ESO end-to-end simulator OCTOPUS
    Extremely Large Telescopes are very challenging concerning their Adaptive Optics requirements. Their diameters, the specifications demanded by the science for...
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    Comparison of Solar Oscillation Data Obtained from a Study of the NA and K Fraunhoffer Absorption Lines
    Two independent resonant scattering spectrometers, one using a sodium and the other a potassium vapour cell, were operated simultaneously at the same site. Due...
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    Comparison of the aerosol index from satellites and the atmospheric extinction coefficient above the Canarian Observatories
    Satellite data measuring aerosols over the Canary Islands need to be correctly interpreted in accordance with the spatial resolution and spectroscopic channels...
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    Comparison of the Calibrated MDI and GOLF Signals. IV. p-Mode Energy Budget
    The energy calculation of the p-modes requires accurate estimates of both amplitudes and linewidths. These parameters can be derived from a suitable model used...