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• W2027772258 endingPage "L75" @default.
• W2027772258 startingPage "L72" @default.
• W2027772258 abstract "The magnetic field strength inside a model coronal loop is estimated using coronal seismology, to examine the reliability of magnetic field strengths derived from observed, transverse coronal loop oscillations. Three-dimensional numerical simulations of the interaction of an external pressure pulse with a coronal loop (modeled as a three-dimensional density enhancement inside a two-dimensional magnetic arcade) are analyzed and the observed properties of the excited transverse loop oscillations are used to derive the value of the local magnetic field strength, following the method of Nakariakov & Ofman. Due to the (unexpected) change in periodicity, the magnetic field derived from our observed oscillation is substantially different from the actual (input) magnetic field value (approximately 50%). Coronal seismology can derive useful information about the local magnetic field, but the combined effect of the loop curvature, the density ratio, and aspect ratio of the loop appears to be more important than previously expected." @default.
• W2027772258 created "2016-06-24" @default.
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• W2027772258 date "2009-06-17" @default.
• W2027772258 modified "2023-10-16" @default.
• W2027772258 title "PUTTING CORONAL SEISMOLOGY ESTIMATES OF THE MAGNETIC FIELD STRENGTH TO THE TEST" @default.
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• W2027772258 doi "https://doi.org/10.1088/0004-637x/699/2/l72" @default.
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