TY - JOUR
T1 - Detection of three periodicities in a single oscillating coronal loop
AU - Van Doorsselaere, T.
AU - Birtill, D. C C
AU - Evans, G. R.
PY - 2009/12/4
Y1 - 2009/12/4
N2 - Context: TRACE 171 A° observations of transverse loop oscillations on May 13, 2001 have been studied by De Moortel & Brady (2007). They found hints of 3 periodicities present in this event.Aims: The aim of this article is to improve the analysis, and measure the periodicities more accurately in order to do coronal seismology.Methods: We create multiple (x,t)-slices across the loop, and determine the oscillatory parameters within those slices. We then use statistical methods to reduce the errors on the measured oscillations parameters.Results: We find two populations with a clearly distinct period. The population at the loop top has a period of 895 ± 2 s, while the population in the loop leg has a period of 452 ± 1 s. The fact that the ratio of these two periods is roughly 2 and the geometry of the problem suggests that two harmonics are observed. In the residues, we confirm the presence of a 3rd harmonic with period 309 ± 15 s using two separate data analysis techniques. The three periods are then used to do a seismological estimate of the loop expansion and the density scale height.
AB - Context: TRACE 171 A° observations of transverse loop oscillations on May 13, 2001 have been studied by De Moortel & Brady (2007). They found hints of 3 periodicities present in this event.Aims: The aim of this article is to improve the analysis, and measure the periodicities more accurately in order to do coronal seismology.Methods: We create multiple (x,t)-slices across the loop, and determine the oscillatory parameters within those slices. We then use statistical methods to reduce the errors on the measured oscillations parameters.Results: We find two populations with a clearly distinct period. The population at the loop top has a period of 895 ± 2 s, while the population in the loop leg has a period of 452 ± 1 s. The fact that the ratio of these two periods is roughly 2 and the geometry of the problem suggests that two harmonics are observed. In the residues, we confirm the presence of a 3rd harmonic with period 309 ± 15 s using two separate data analysis techniques. The three periods are then used to do a seismological estimate of the loop expansion and the density scale height.
KW - Magnetohydrodynamics (MHD)
KW - Sun: Corona
KW - Sun: oscillations
UR - http://www.scopus.com/inward/record.url?scp=72849139848&partnerID=8YFLogxK
U2 - 10.1051/0004-6361/200912753
DO - 10.1051/0004-6361/200912753
M3 - Article
AN - SCOPUS:72849139848
SN - 0004-6361
VL - 508
SP - 1485
EP - 1491
JO - Astronomy & Astrophysics
JF - Astronomy & Astrophysics
IS - 3
ER -