6) ANOMALOUSLY SPLIT MODE 3 S 2
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Transcript of 6) ANOMALOUSLY SPLIT MODE 3 S 2
6) ANOMALOUSLY SPLIT MODE 3S2
4) OBSERVATIONS 3) INTEREST of MODE OBSERVATIONS
A new catalog of eigenfrequencies from the 26th December 2004 Sumatra-Andaman mega-event and first perspectives
Julien Roch, Geneviève Roult and Eric Clévédé
Institut de Physique du Globe de Paris, 4 Place Jussieu, 75005 Paris, France. Contact: [email protected]
9) CONCLUSIONThe FDSN networks provide high quality records of the Sumatra mega-event and long-period spectra allowing a precise determination of eigenfrequencies for some modes and individual singlets. At present 17 modes have been precisely analyzed from both vertical and horizontal components (0S0, 1S0, 2S0, 3S0, 4S0, 0S2, 0S3, 0S4, 0S5, 2S1, 3S1, 11S1, 1S2, 3S2, 13S2, 2S3, 0T2).
Our results show sometimes interesting discrepancy with prediction and known features. We are completing our collection in order to determine a density profile model and to improve the resolution of both attenuation and density in the Earth, parameters not well presently constrained. They will contribute to a better knowledge of the internal structure of the Earth.
Some modes are very interesting due to their sensitivity to the outer and inner cores
UNM station. Spectrum of 10 days recording (Roult et al., 2008)
2) DATA
1) INTRODUCTIONThe high-quality records obtained for the Sumatran-Andaman event of 2004, December 26th from all FDSN stations, allows to determine precise eigenfrequencies of some singlets from the gravest modes and from some « anomalous » modes. These data will help to better constrain density models of the deep Earth and increase our knowledge on some parameters for the whole Earth.
inner core
outer core
vertical components (10days)
horizontal components (10days)
The symbol size is proportional to measurement quality
All the anoumalously split modes, as 3S2, are sensitive to the inner core. The five black thin lines indicate the PREM-re theoretical eigenfrequencies. Two singlets are particularly well resolved, the singlet m=-2 and the ‘supposed’ singlet m=0. Despite few measurements for the singlet m=+1, we calculate the splitting ratio (r=1.70) that can be compared to the previously estimated 1.58 splitting ratio [He and Tromp, 1996].
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0S2 mode, ECH (France, G)
3S2 mode, COLA (Alaska, IU)
0S0 mode, CAN (Australia, G)
-2 -1 0 +1 +2
1S0 mode, BBSR (Atl. Oc., IU)
3S1 mode, KMI (China, IU)
-1 0 +1
0S2
53.9’
2S1
0T2
0S3
35.6’
20.9’ dr=0.05mm
0S0
0S4
1S2
0T40T3
0S5
2S2
1S3
3S2
0S6
1S5
2S4
0S7 0S8 0S9 0S10
1S4 1S04S2
1S8
2S3
1S7
2S61S9
3S1
0S120S11
2S5
1S6
CMB
mantle
ICB
0S3 3S1 3S2
___ compressional --- shear ___ density
m = -2 -1 0 +1 +2
-2 -1 0 +1 +2
-2 -1 0 +1 +2
1S2 mode, ECH (France, G)
We got data more than 1 year after the Sumatra-Andaman event, via the NetDC procedure from 320 operational FDSN stations. We downloaded all data spanning the period 2004 December 25th to 2005 February 1st. Our goal was to obtain records of one month in continue, in order to improve the resolution. Unfortunately, lots of records have numerous gaps or glitches, it means that for some stations we got more than 30 files with gaps exceeding sometimes 5 minutes. We finally decided to restrict ambition to the 15 days continuous series, that it to say a selection of only 151 stations and 247 different recordings.
5) FUNDAMENTAL MODES
OS2
Our results exhibit no large discrepancies with the theoretical values (black lines) computed in the PREM-re (PREM model [Dziewonski and Anderson, 1981] with rotation and ellipticity) [Millot et al., 2003], The observed splitting ratio r (ratio of the observed splitting width to the splitting width predicted due to the effects of rotation and hydrostatic ellipticity) is indicated (top left).
We plot all observed eigenfrequencies versus the station latitude (red dots and vertical red lines corresponding to the individual singlet mean value)
8) RESULTS
7) SYNTHETICS SPECTRAUsing the HOPT method (Lognonné, 1991; Lognonné et Clévédé, 2002; Millot-Langet et al., 2003), we compute synthetics spectra with the PREM model taking into account both rotation and ellipticity and a 3D elastic model of the mantle (SAW12D). We also compute synthetics spectra using a complex source (Tsai et al. 2005), and the Harvard CMT source, and we compare the results.
The blue beachballs indicate the focal mechanism of the five Tsai et al. sources used to represent the fault rupture. The red one is the Harvard CMT solution.
Roult G., J.Roch and E. Clévédé, 2008, A new catalog of eigenfrequencies from the 26th December 2004 Sumatra-Andaman mega-event, PEPI, submitted
-2 -1 0 +1+2
All FDSN (GEOSCOPE, IRIS,...) stations used in this study. Too few were able to provide long time series without any problem (gaps, glitches…).
The data are best fitted for the Tsai et al. complex rupture (5 sources) than for the Harvard mechanism.