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The Sun

In this subdiscipline: 440 papers
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Popular papers

  1. This paper reviews recent advances and current debates in modeling the solar cycle as a hydromagnetic dynamo process. Emphasis is placed on (relatively) simple dynamo models that are nonetheless detailed enough to be comparable to solar cycle…
  2. The Sun's outer atmosphere, or corona, is heated to millions of degrees, considerably hotter than its surface or photosphere. Explanations for this enigma typically invoke the deposition in the corona of nonthermal energy generated by…
  3. We use the Michelson Doppler Imager and TRACE observations of photospheric magnetic and velocity fields in NOAA 10759 to build a three-dimensional coronal magnetic field model. The most dramatic feature of this active region is the 34 rotation of…
  4. We present the first Solar Dynamics Observatory Atmospheric Imaging Assembly (AIA) observations of a global coronal EUV disturbance (so-called "EIT wave") revealed in unprecedented detail. The disturbance observed on 2010 April 8 exhibits two…
  5. We review the current status of local helioseismology, covering both theoretical and observational results. After a brief introduction to solar oscillations and wave propagation through inhomogeneous media, we describe the main techniques of local…
  6. We developed numerical codes designed for automated analysis of SDO/AIA im- age datasets in the six coronal filters, including: i) coalignment test between different wave- lengths with measurements of the altitude of the EUV-absorbing chromosphere,…
  7. Relying purely on solar photospheric magnetic field measurements that\ncover most of solar cycle 23 (1996-2005), we calculate the total\nrelative magnetic helicity injected into the solar atmosphere, and\neventually shed into the heliosphere, over…

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