Coronal loop seismology using multiple transverse loop oscillation harmonics

Astronomy and Astrophysics – Astrophysics

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Sun: Corona, Sun: Magnetic Fields, Sun: Oscillations, Sun: Uv Radiation

Scientific paper

Context: TRACE observations (23/11/1998 06:35:57-06:48:43 UT) in the 171 Å bandpass of an active region are studied. Coronal loop oscillations are observed after a violent disruption of the equilibrium. Aims: The oscillation properties are studied to give seismological estimates of physical quantities, such as the density scale height. Methods: A loop segment is traced during the oscillation, and the resulting time series is analysed for periodicities. Results: In the loop segment displacement, two periods are found: 435.6 ± 4.5~s and 242.7 ± 6.4~s, consistent with the periods of the fundamental and 2nd harmonic fast kink oscillation. The small uncertainties allow us to estimate the density scale height in the loop to be 109~Mm, which is about double the estimated hydrostatical value of 50~Mm. Because a loop segment is traced, the amplitude dependence along the loop is found for each of these oscillations. The obtained spatial information is used as a seismological tool to give details about the geometry of the observed loop.

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