JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 107, NO. B10, 2256, doi:10.1029/2001JB000804, 2002 Characteristics of Lg attenuation in the Tibetan Plateau Guangwei Fan and Thorne Lay1 Center for the Study of Imaging and Dynamics of the Earth, Institute of Geophysics and Planetary Physics, University of California, Santa Cruz, California, USA Received 23 July 2001; revised 5 March 2002; accepted 2 May 2002; published 25 October 2002. [1] Lg, a regional seismic wave comprised of multiple shear wave reverberations trapped in the crustal waveguide, is important for magnitude estimation and source discrimination for monitoring nuclear testing treaties. In stable continental regions, Lg propagates with a group velocity of about 3.5 km/s and can often be observed at distances up to 4000 km. To better understand the absence of high-frequency Lg arrivals for paths traversing the northern boundary of the Tibetan Plateau, we investigate spatial variations of broadband (0.15–5.0 Hz) energy in the Lg group velocity window (3.6–3.0 km/s) using regional waveforms recorded at the Chinese Digital Seismic Network station WMQ. Vertical component seismograms are analyzed for 90 events with magnitudes of 4.4 mb 6.4 that occurred between 1987 and 1999 in the Tibetan Plateau and around its margins. The Lg amplitude spectra for events located near the northern margin of the plateau have apparent corner frequencies of 1–2 Hz, nearly identical to those for comparable size events at similar distances outside the plateau. High-frequency (>1 Hz) Lg energy recorded at WMQ decreases rapidly as a function of source distance into the plateau. A path length of 300–400 km within the northern Plateau suffices to eliminate 2–5 Hz Lg energy. For events in southern Tibet with paths crossing the central portion of the Tibetan Plateau, almost total Lg extinction occurs, even for energy in the low-frequency band of 0.2–1 Hz. Corresponding apparent corner frequencies of the ‘‘Lg’’ amplitude spectra range between 0.2 and 0.4 Hz. The corner frequency shift is found to vary systematically with path length across the plateau. Linear regressions demonstrate that the shift in apparent corner frequency of Lg amplitude spectra is negatively correlated with features of the Tibetan Plateau, such as mean elevation along the paths or travel distance within the plateau above specified elevation thresholds. The systematic variations in the amplitude and frequency content of energy in the Lg window as a function of path length within the plateau indicate that strong crustal attenuation plays an important role in Lg extinction for paths traversing central and northern Tibet, superimposed on any structural blockage effects associated with abrupt thinning of the crust near the northern boundary of the plateau. Spectral ratios of many event pairs along great circle paths give estimates of frequency-dependent Lg attenuation for paths crossing western, central, and eastern sectors of Tibet. The region of strong Sn attenuation in northern central Tibet also has strong Lg attenuation with QLg for 1 Hz on the order of Qo = 80–90, while in southern central Tibet, Qo increases to about 316, and in eastern and western Tibet, Qo is on the order of 120–200 for paths traversing the entire plateau. The strong Lg attenuation in northern central Tibet is responsible for the so-called Lg blockage and may be associated with partial melting in the crustal low-velocity layer in northern Tibet. Our QLg values for Tibet are significantly lower than most earlier estimates, primarily as a result of not excluding blocked observations along with allowing for lateral variations within INDEX TERMS: 7203 Seismology: Body wave propagation; 7255 Seismology: Surface waves and Tibet. free oscillations; 7205 Seismology: Continental crust (1242); KEYWORDS: Lg, Tibetan Plateau, nuclear event discrimination, crustal attenuation, Lg blockage, crustal partial melting Citation: Fan, G., and T. Lay, Characteristics of Lg attenuation in the Tibetan Plateau, J. Geophys. Res., 107(B10), 2256, doi:10.1029/2001JB000804, 2002. 1 Also at Earth Sciences Department, Institute of Tectonics, University of California, Santa Cruz, California, USA. Copyright 2002 by the American Geophysical Union. 0148-0227/02/2001JB000804$09.00 ESE 1. Introduction [2] Lg is a regional seismic phase commonly observed in continental areas. It is variously described as a superposition of many higher mode surface waves or trapped postcritical S 14 - 1 ESE 14 - 2 FAN AND LAY: CHARACTERISTICS OF Lg ATTENUATION IN THE TIBETAN PLATEAU waves, with most of its energy being confined to the crustal waveguide [e.g., Xie and Lay, 1994]. When observed on vertical component seismograms, Lg can be primarily associated with Rayleigh wave overtone modes, although scattering may mix Love and Rayleigh energy. Lg is rather insensitive to earthquake radiation patterns, thus it has particular value for seismic magnitude estimation. Because Lg is dominated by shear wave energy, it tends to be more strongly excited by earthquakes than by explosions. Thus, various P/Lg amplitude measures have been developed for source identification applications, with good success for frequencies above 2 – 3 Hz [e.g., Walter et al., 1995; Taylor, 1996; Hartse et al., 1997]. Lg propagation is affected by laterally heterogeneous crustal thickness and velocity structure [e.g., Kennett, 1989; Bostock and Kennett, 1990; Zhang et al., 1994] and Lg does not propagate efficiently in thin oceanic crust [e.g., Press and Ewing, 1952; Zhang and Lay, 1995], but it is otherwise extensively observed. In Eurasia, Lg is the most stable phase observed at regional distances [Sereno et al., 1990; Baumgardt, 1990; Rapine et al., 1997], with efficient broadband Lg transmission over large distances in much of the continental crust. [3 ] Strong attenuation or blockage of Lg has been observed in some continental areas where significant changes in crustal thickness are located, such as the mountain belts in central Asia [Ruzaikin et al., 1977], the Tibetan Plateau [Båth, 1954; Ni and Barazangi, 1983; McNamara et al., 1996; Rapine et al., 1997], in the Bolivian Altiplano [Baumont et al., 1999] and near the Alpine mountains [Campillo et al., 1993]. It is believed that scattering of Lg energy from fractures within the shallow crust may be a major cause of strong Lg attenuation in tectonically active regions, while in regions such as Tibet partial melt in the crust may also play an important role. It is also possible that the lack of a continuous waveguide in areas with significant variations of crustal thickness and sedimentary basin thickness may result in disruption of Lg [Baumgardt, 1990]. Understanding the causes of inefficient Lg propagation in various settings is very important for event discrimination, particularly in the context of nuclear test monitoring efforts; anomalously low Lg amplitudes may cause earthquake signals to resemble those for explosions. [4] Of particular interest for this study are observations that Lg is extremely weak or totally extinguished for paths traversing the northern margins of the Tibetan Plateau. Ruzaikin et al. [1977] found that a path length of 200 km within the plateau is sufficient to attenuate 1 Hz Lg signals down to noise levels for observing stations located north of the plateau. Those authors suggested that either strong attenuation or scattering by a thinning crustal waveguide was responsible, but their narrow-band data did not resolve a progressive shift of Lg spectral content to lower frequencies with increasing path length in Tibet, as would be expected if attenuation is primarily responsible. They did note that very low QLg values of 20– 40 would be required to attenuate 1 Hz Lg energy by a factor of 100 over 100 –200 km path lengths, as their qualitative observations suggested. Qualitative analysis of Lg propagation efficiency relative to P wave coda for stations west and south of Tibet indicated that Lg signals are strongly attenuated within central and northern Tibet while the phase does propagate along the Himalayan mountain belt [Ni and Barazangi, 1983]. This inefficient Lg propagation was again attributed to either strong crustal attenuation within Tibet or to waveguide disruption on the southern margin. Rapine et al. [1997] found inefficient Lg propagation across most of Tibet, with no Lg from western Himalayan events reaching either station WMQ to the north of the Tarim Basin or station LSA within Tibet (LSA did record Lg on some paths from events in the eastern Himalayas and eastern Tibet, suggesting internal variations in propagation efficiency within the plateau). [5] McNamara et al. [1996] analyzed data recorded at 11 broadband stations in eastern central Tibet, finding that highfrequency Lg is generated by events within the plateau, and can propagate to distances of at least 600 km; however, the phase was not observed for paths traversing western or central Tibet or for events in the Himalayas. For eastern Tibet, where sufficient Lg signal-to-noise ratios were observed, a frequency-dependent QLg function given by QLg( f ) = (366 ± 37) f (0.45±0.06) was estimated for the passband (0.5 –16 Hz) [McNamara et al., 1996]. This is comparable to the estimate of QLg( f ) = (448 ± 82) f (0.426±0.157) estimated for 1 – 6 s Lg waves traversing Tibet by Shih et al. [1994]. This latter value is likely also dominated by eastern Tibet paths, as ‘‘blocked’’ observations were omitted from the calculation. QLg value at 1 Hz was also estimated to be about 340 for events north of LSA using spectral methods by assuming a constant QLg model [Reese et al., 1999]. These attenuation values are typical of tectonically active areas, and are not low enough to cause rapid extinction of 1 Hz Lg over just a few hundred kilometers, as observed for paths traversing the northern margin of Tibet. One could perhaps infer that waveguide disruption must cause extinction of Lg in the latter regions; however, this is not a secure interpretation because QLg may vary laterally within Tibet. Indeed one might expect this to be the case, for it is true of Sn attenuation, which is strongest in northern central Tibet. The possibility of stronger Lg attenuation in northern and central Tibet is suggested by the lack of high-frequency Lg detections for events to the west of the broadband stations in the data set of McNamara et al. [1996]. [6] Although the failure of Lg to propagate on oceanic paths has been relatively well explained by numerical modeling [Kennett, 1986; Cao and Muirhead, 1993; Zhang and Lay, 1995], the physical nature of Lg blockage for continental paths is still debated. For paths traversing the northern margin of Tibet the question is whether a step in crustal thickness on the plateau margins plays a significant role or whether other properties of the crust are important. It is probable that crustal attenuation plays some role as moderate necking of the crust alone is not likely to impede high-frequency Lg propagation to the extent observed [Regan and Harkrider, 1989; Gibson and Campillo, 1994]. We analyze broadband, digital seismic data to characterize general features of Lg wave propagation across the northern Tibetan Plateau margin and to explore the relative roles of Lg attenuation and crustal disruption. Assuming a frequency-dependent QLg model, we estimate the values of the Lg attenuation for different parts of Tibet to characterize attenuation heterogeneity in Tibet. 2. Data Analysis [7] Our main data are regional waveforms recorded at broadband station WMQ, the westernmost station of the FAN AND LAY: CHARACTERISTICS OF Lg ATTENUATION IN THE TIBETAN PLATEAU ESE 14 - 3 Figure 1. Topography in western China and its vicinity. The location of station WMQ is shown. The squares, circles, triangles, and inverted triangles indicate the epicenters of the events used in this study, keyed to other figures. Squares with origin dates indicate events for which spectra are shown. The events within Tibet are grouped into eastern (inverted triangles), central (circles) and western (triangles) groups. Chinese Digital Seismic Network. This station lies just north of the Tarim Basin, about 650 km from the northern boundary of the Tibetan Plateau (Figure 1). While threecomponent data were obtained, we restrict our analysis to the vertical component seismograms due to the attenuated nature of the Lg phases traversing Tibet, which leads to confusion with fundamental mode Love wave energy on the transverse components. We examine energy in the standard Lg group velocity window of 3.6 to 3.0 km/s, which precedes short and intermediate period fundamental mode Rayleigh wave energy. We analyze recordings for 90 earthquakes with magnitudes of 4.4 mb 6.4 that occurred between 1987 and 1999 in the Tibetan Plateau and around its margins. A few events with paths well removed from Tibet (Figure 1) were also analyzed. [8] The recorded seismograms show great variability in broadband waveforms, and our analysis is constrained to relative measures because we use only one station and cannot fully account for source effects. For events prior to 1998 the source parameters are taken from the International Seismological Center (ISC) bulletin. For more recent events the source parameters are from the USGS Preliminary Determination of Epicenters (PDE) catalog. Only events with catalog focal depths less than 50 km are included. While catalog source depths in this region are subject to tens of kilometers of uncertainty, this criterion probably ensures that all events analyzed are crustal events, given that the crustal thickness in the central Tibetan Plateau is about 65 to 75 km [e.g., Hirn et al., 1984; Molnar, 1988; McNamara et al., 1995; Rodgers and Schwartz, 1998; Zhao et al., 2001]. All selected events have signal-to-noise ratios greater than 2 for broadband measurements of the Pn signal and pre-Pn noise. A list of the events used is available from the authors upon request. [9] Figure 2 demonstrates the predominant feature of high-frequency Lg propagation across the northern Tibetan Plateau boundary first documented by Ruzaikin et al. [1977]. The records shown are for a roughly northwest to southeast profile of events, with the signals filtered in the bandpass 1.0 –5.0 Hz. The first three records are for events located near the 4000 m topographic contour along the northern boundary of the plateau. These show typical earthquake-like high-frequency signals, with predominant Lg energy that is much stronger than the Pn arrivals. The largest arrivals in the Lg window (brackets) tend to have group velocities near 3.5 km/s. The lower two records are from events 250– 400 km further to the southeast, and the maximum relative amplitude ratio of Lg to P energy is about a factor of ten lower than for the northwestern events, giving these signals explosion-like character. While P wave amplitudes tend to vary more than Lg due to focal mechanism effects, this relative behavior is observed for all waveforms. The distribution of events in Tibet (Figure 1) presents a challenge in that there is not a continuous distribution of events from the plateau margin to the interior; this makes it difficult to separate possible waveguide disruption effects from strong crustal attenuation effects as causes for the high-frequency Lg energy blockage. However; we can consider behavior of Lg at lower frequency on longer profiles to assess the role of attenuation in the plateau, as this should be manifested in a progressive shift of the frequency content of Lg with propagation length across the plateau as suggested by Molnar (in a personal opinion expressed by Ruzaikin et al. [1977]). 14 - 4 ESE FAN AND LAY: CHARACTERISTICS OF Lg ATTENUATION IN THE TIBETAN PLATEAU Dist=632 km BAZ=158.9 5000 specific energy, but a group velocity of 3.5 km/s is a reasonable value to use for the larger arrivals early in the Lg signal. [11] We lack detailed knowledge of the source process and radiation effects for our events, and the station coverage is not adequate to enable empirical separation of source and propagation effects. However, our broadband digital data indicate that propagation effects dominate in shaping the Lg window. We examine windowed and tapered velocity amplitude spectra with no source corrections, measuring the apparent corner frequency of the velocity amplitude 4.49 0 -5000 940907 -10000 30000 Dist=701 km BAZ=154.3 2.75 0 -30000 870225 80000 Dist=759 km BAZ=150.2 3.68 Dist=632 km (940907) 0 -80000 1000 900114 (1/3 x Amp.) Dist=1006 km BAZ=154.4 500 0.42 Dist=701 km (870225) 0 890513b -500 300 Dist=983 km (980113) Dist=1116 km BAZ=159.5 0.59 Dist=1116 km (881125) 0 881125 -300 0 100 200 TIME (s) 300 Dist=1339 km (900602) 400 Dist=1415 km (940723) Figure 2. Demonstration of the rapid decrease in Lg energy near the northern Tibetan Plateau boundary. Events are identified with numbers indicating year/month/day. WMQ records are shown for a short NW – SE profile of events, with bandpass filters isolating the 1.0– 5.0 Hz passband, for events near the northern boundary (top 3 records) and a few hundred kilometers into the plateau (lower 2 records). The Lg group velocity window (3.6 – 3.0 km/s) is indicated by the bracket below each seismogram. Small arrows represent the Pn arrivals after the onset of visible signal in each trace. There is about a factor of 10 decrease in the Lg/Pn amplitude ratio (shown by the numbers on upper right of each trace) common to all events several hundred kilometers south of the plateau boundary. Dist=1526 km (980825) Dist=1644 km (880125) Dist=1781 km (970131) Dist=1839 km (980926) 0 [10] Figure 3 shows a longer profile of records, retaining the full broadband energy with amplitudes normalized relative to the 20 s Rayleigh wave energy in each signal. The dramatic shift of frequency content in the Lg group velocity window over the first few hundred kilometers is again apparent, but now it is clear that there is also a progressive shift of frequency content and a decrease of relative amplitudes in the Lg window for lower frequencies as path length across the plateau increases. This suggests that while high-frequency Lg energy is eliminated over short path segments in the plateau, lower frequency energy survives much longer and can be used to constrain any progressive path effect. The rapid amplitude decrease with distance and sparse sampling make it difficult to track 200 400 TIME (s) 600 800 Figure 3. Broadband recordings at WMQ for events along a profile traversing the entire central portion of the Tibetan Plateau. The records have been amplitude-normalized relative to the 20 s Rayleigh wave energy in each signal (note the amplitude reduction for the first record) to help display the rapid decrease of high frequency energy in the Lg group velocity window (brackets). Small arrows represent the first P arrivals after the onset of visible signal in each trace. There is a steady shift of the spectral content and relative amplitude of energy in the Lg window as path length within the plateau increases. The two most distant recordings show increased P amplitudes due to upper mantle triplications. FAN AND LAY: CHARACTERISTICS OF Lg ATTENUATION IN THE TIBETAN PLATEAU 900114 Event 107 106 Amplitude 105 104 103 102 101 Lg Wave Pre-Pn Noise 100 10-1 10-2 a) 10-1 100 Frequency (Hz) 101 920730 Event 106 105 Amplitude 104 103 102 101 Lg Wave 100 Pre-Pn Noise 10-1 b) 10-2 10-1 100 Frequency (Hz) 101 Figure 4. Amplitude spectra for Lg signal and pre-Pn noise recorded at seismic station WMQ for: (a) an event located near the northern margin of the plateau, and (b) for an event located in southern Tibet. The event locations are indicated in Figure 1. The event magnitudes are comparable, so most of the tremendous variation in Lg spectral content is due to propagation effects. spectra for each event. The observed apparent corner frequency is defined as the frequency where the amplitude spectra start to fall-off. We call this corner frequency, which is not to be confused with the source radiation effect, and use its values below to infer relative attenuation of the Lg energy. [12] To explore whether the Lg group velocity significantly affects the spectral corner frequency estimate, we considered several group velocity windows (3.6 to 2.8, 3.8 to 2.8, 3.6 to 3.0 and 3.8 to 3.0 km/s). The corner frequency measurements are relatively insensitive to the value of the larger group velocity, but the choice of lower group velocity affects the low-frequency part of the amplitude spectra. This is because fundamental Rayleigh wave energy enters the window as the lower Lg group velocity decreases from 3.0 km/s to 2.8 km/s. For events in southern Tibet, the Lg wave defined by a group velocity window of 3.6 to 3.0 km/s is well isolated, albeit almost totally attenuated (Figure 3), so we hold this group velocity window fixed. [13] We compare the Lg amplitude spectra with pre-Pn noise as a guide to signal bandwidth. One can also consider the pre-Lg signal strength, but our purpose is not to define a threshold for defining the existence of an Lg phase, only to characterize the overall spectral evolution of the Lg window ESE 14 - 5 with distance. The noise spectra are computed from 10 –15 s time windows preceding the Pn arrival. Figure 4 shows some comparisons of the Lg and background noise spectra. Our data generally have good low-frequency signal-to-noise ratios, but the spectral character is strongly dependent on source location. Figure 4a shows the velocity spectra for a representative event located near the northern margin of the plateau. The signal-to-noise ratio is high across the entire frequency band, and the Lg amplitudes are much higher than noise amplitudes at frequencies up to 6 Hz, where the instrument limitations flatten the spectra. The corner frequency is not very well defined for this spectrum, but fitting of asymptotes to the 0.1 – 0.7 Hz band and the 1 – 4 Hz band gives a corner frequency near 0.8 to 1.0 Hz. Around 4 – 5 Hz the spectral roll-off steepens further. For events near the southern margin of the plateau, the WMQ spectra for Lg are above background noise for frequencies below 1 Hz, but there is no high-frequency Lg signal even relative to the background noise level (see Figure 4b). A comparison with spectra for the pre-Lg window (Sn coda window) indicates that all energy above 0.5– 1.0 Hz in this window may be scattered Sn. This limits the range used for QLg estimation. A corner frequency of around 0.18– 0.22 Hz can be defined. There is clearly a huge difference in spectral content that greatly exceeds any plausible effect of the source radiation for these events. Lacking detailed source corrections, we will seek systematic behavior in our large data population to effectively average out minor source effects. 3. Distance Dependence of Lg Spectra in Tibet [14] For most events located near the northern margin of the Tibetan Plateau, the WMQ Lg velocity spectra have a corner frequency of 1 – 2 Hz. The windowed and tapered Lg energy decays fairly slowly at frequencies from 2 – 5 Hz and more rapidly after 5 Hz, as shown in Figure 4a. Many associated paths traverse either the central or eastern regions of the Tarim Basin, and thus these Lg signals may still be anomalous relative to Lg on other paths in Eurasia. To assess this, we compare the amplitude spectra for an event on the Tibetan Plateau margin with an event located directly west from WMQ. The two events have the same magnitude, similar seismic moments, similar Harvard Centroid Moment Tensor depths and focal mechanisms, and similar propagation distances (Figure 5a). The waveforms and spectra are quite similar, with corner frequencies in the vicinity of 1 Hz and steepening of the high-frequency spectra near 5 Hz due to instrument and windowing effects. Comparisons with other distance- and magnitude-matched pairs indicate that there is nothing anomalous about the Lg signals from events on the northern Tibetan Plateau margin relative to events elsewhere in central Eurasia. This indicates that Lg propagation across the eastern Tarim Basin is similar to that elsewhere in the China platform, consistent with results from Lg attenuation tomography by Phillips et al. [2000]. It also appears that there is no abrupt effect on Lg associated with the rapid increase in topography and presumably rapid crustal thickening along the northern margin of the plateau, as similar waveforms and spectra are observed for events located beneath topography ranging from 2000 to 4000 m. This is consistent with prior observations. Numerical simulations of Lg wave propagation indicate that a stepwise 14 - 6 ESE FAN AND LAY: CHARACTERISTICS OF Lg ATTENUATION IN THE TIBETAN PLATEAU a. b. 931230 50000 10000 0 0 -50000 -5000 0 100 200 300 400 Time (sec) mb = 5.7 Mo = 1.87E+17 N m Dist. = 715 km -10000 0 200 400 600 Time (sec) 106 mb = 5.5 Mo = 8.27E+16 N m Dist. = 1685 km 106 105 105 104 Amplitude Amplitude 880103 5000 103 102 101 931230 870225 100 10-1 10-2 104 103 102 101 880103 880125 100 10-1 100 101 10-1 10-2 Frequency (Hz) 5000 870225 100000 10-1 100 101 Frequency (Hz) 880125 0 0 -5000 -100000 0 100 200 Time (sec) 300 400 mb = 5.7 Mo = 5.75E+17 N m Dist. = 701 km 0 200 400 Time (sec) 600 mb = 5.4 Mo = 8.86E+16 N m Dist. = 1645 km Figure 5. Comparisons of Lg amplitude spectra for events located on the margin or within the Tibetan Plateau with events outside the plateau that have similar path lengths, magnitudes and focal mechanisms: (a) The top seismogram is for event 931230 (year/month/day), an event located west of WMQ, and the lower seismogram is for event 870225 near the northern Plateau margin (see Figure 1). Note the similarity of the Lg spectra and waveforms. (b) The top seismogram is for event 880103 in central China while the lower seismogram is for event 880125 in southern Tibet (see Figure 1). Note the relative depletion of high frequency Lg energy for the path traversing the plateau. Lower hemisphere best double couples are shown from the Harvard Centroid Moment Tensor solutions for all events, along with corresponding seismic moments. decrease in crustal thickness does not cause Lg blockage [e.g., Gibson and Campillo, 1994], and this would be particularly true for events located very close to the step change. However, because there is a two hundred kilometer distance gap to the next concentration of seismic activity in the plateau, and those events lack high-frequency Lg signals, a possible role of blockage by crustal necking for the events further to the south remains open. [15] For events near the Himalayan mountains, Lg signals at WMQ traverse the entire Tibetan Plateau. Without exception, Lg signals at WMQ for long travel paths across the plateau are weak or entirely extinguished. For the Himalayan and southern Plateau events, the corresponding corner frequencies of velocity spectra range between 0.2 and 0.4 Hz, and the spectra are similar to Figure 4b. The question then arises as to how anomalous such spectra are, so we again compare with signals for comparable propagation distances outside the plateau. Figure 5b shows one such comparison, for events of similar magnitude, seismic moment, focal mechanism and propagation distance. The event in Central China is quite typical of Eurasian observations at this distance, with strong, high-frequency Lg energy arriving ahead of the fundamental mode Rayleigh wave, and a spectral corner frequency around 0.7 Hz. The seismogram for the event in southern Tibet is visibly depleted in high-frequency Lg, and the corner frequency is shifted to about 0.2 Hz, despite the presence of comparable high-frequency energy in direct P and the P coda and comparable fundamental mode amplitudes. Such comparisons confirm that the Tibetan paths are truly anomalous relative to standard Eurasian paths, and that the spectral character is robust enough that we can proceed to characterize the evolution of this spectral behavior across Tibet even though detailed source models are not available. [16] We observe that the Lg spectra evolve systematically between the extremes in Figures 5a and 5b as a function of path length across Tibet. The pattern is most evident for the longest paths through central Tibet, and somewhat more subdued for paths across western and eastern Tibet. We thus divide the events into three subgroups based on the back FAN AND LAY: CHARACTERISTICS OF Lg ATTENUATION IN THE TIBETAN PLATEAU Corner Frequency (Hz) 101 CC = -0.820 SD = 0.156 K = -0.0605 Lg 100 10-1 500 1000 a) 1500 2000 Distance (km) Corner Frequency (Hz) 101 CC = -0.938 SD = 0.0950 K = -34.383 Lg 100 10-1 1 b) 2 3 4 Mean Elevation (km) Figure 6. Apparent corner frequency of the Lg amplitude spectra for events in the Tibetan Plateau as a function of (a) path length from WMQ and (b) mean path elevation along the path to WMQ. Symbols in (a) are the same as those in Figure 1, and these indicate the shift to lower corner frequencies for paths in central Tibet; solid circles in (b) represent all events used. CC, linear correlation coefficients; SD, standard deviation of linear regression; K, slope of the regression line. The dotted lines indicate ±1 standard deviation about the regression lines. azimuth of each event (see Figure 1). While the corner frequency of the velocity spectra is a rather uncertain, subjective parameter, we find it useful for conveying the overall evolution of the spectra manifested in the raw data. Figure 6a shows the corner frequency estimates as a function of total path length to WMQ, with symbols differentiating the three spatial subgroups. While one would expect some trend due to attenuation, a much subtler trend would be found for events outside Tibet, effectively a shift from 1 – 2 Hz near 700 km to 0.7 –1 Hz near 2000 km, as demonstrated in Figure 5. While source size should affect corner frequency, this is also expected to be a small effect because most of our data span only one unit of magnitude. We actually find no correlation between the observed corner frequencies and event magnitude, suggesting that the source effect is swamped by propagation factors. We also could not detect any systematic variation with source focal mechanism for the events with Harvard CMT solutions, although such dependence may be rather complex. Lg radiation patterns are often treated as isotropic for gross measure- ESE 14 - 7 ments such as ours [e.g., Shih et al., 1994], and we will make this assumption below. [17] Overall, the data in Figure 6a display a systematic decrease in corner frequency with path length, with a baseline shift between central Tibet and eastern or western regions of the plateau. In detail, the data exhibit some clustering that reflects distributions in the seismicity, but if one focuses on the circles, which are for paths through central Tibet, it is clear that the primary factor appears to be propagation distance from the Tibetan Plateau margin. It has been observed that a sharp change in crustal thickness across the northern margin of the Tibetan Plateau results in anomalous double-pulse teleseismic P waves at one station near the margin [Zhu and Helmberger, 1998]. Because Lg propagation at regional distances is more complicated than for teleseismic P waves, it is unclear whether there is any abrupt affect on Lg. Nevertheless, it is reasonable to infer that if crustal necking at the northern margin is responsible for the observed Lg blockage, one would expect far less of a uniform trend between central and southern Tibet events than observed. The logarithmic corner frequency values decay rather linearly with distance. Effectively, these spectra fulfill Molnar’s prediction (as individually summarized by Ruzaikin et al. [1977]) that strong frequency shifts with distance would indicate a progressive attenuation effect. This is, however, a much stronger effect than would be expected for the moderate attenuation values previously found for eastern Tibet [McNamara et al., 1996]. [18] The distribution of seismicity and the geographic pattern of the Tibetan Plateau relative to WMQ (Figure 1) are such that propagation distance alone does not isolate the contributions from the plateau portions of the paths very well. We thus consider the behavior of the Lg amplitude spectra relative to various measures that reflect the plateau path contribution more directly using a parametric analysis method [e.g., Fan and Lay, 1988]. We mainly considered topographic features [Gesch et al., 1999] and parameters from the crustal waveguide structure [Fielding et al., 1992]. Regression analysis shows that the Lg corner frequency measurements have strong, negative correlations with several physical parameters of the Tibetan Plateau. The highest correlation coefficient (0.94) we found is for mean elevation along each path, which reflects the relative portion of the paths within Tibet (see Figure 6b). This correlation appears to suppress any east to west variations within the plateau. If travel distance along the plateau above a certain elevation threshold, such as 4000 m, is used rather than the entire path length to WMQ, the value of correlation coefficient varies from 0.82 (Figure 6a) to 0.92, again suppressing variations from east to west. Strong correlations are also found using mean crustal thickness and mean topographic roughness (variance) of each path (0.90 and 0.85, respectively); these parameters covary strongly with mean elevation. The mean thickness of the sediment layer on each path displays only a weak, positive correlation (0.35) with Lg corner frequency. The available sedimentary thickness information for Tibet is rather low resolution, so it is premature to discount some control on Lg energy by sedimentary basin scattering. The slopes of the higher frequency portion of the Lg amplitude spectra for each event were also computed, but these measures do not show any simple relationship with other physical parameters. This ESE 14 - 8 FAN AND LAY: CHARACTERISTICS OF Lg ATTENUATION IN THE TIBETAN PLATEAU Figure 7. A map showing interpolated estimates of apparent corner frequency for the Lg amplitude spectra for events in the Tibetan Plateau as observed at WMQ. Interpolation of the observations is done using a standard kriging algorithm. Small circles represent the event locations used in this study; thick solid lines are 3000-meter topographic contours. See color version of this figure at back of this issue. may reflect an interaction of frequency-dependent attenuation and source radiation controlling the slope. [19] The two-dimensional spatial pattern of the corner frequency measures made at station WMQ was further examined using an ordinary kriging algorithm to assess whether the single parameter regressions were missing any behavior. The interpolated pattern basically follows the integrated path sampling of plateau topography, surrounded by a base level in other regions of China, and no subtle spatial pattern emerges (see Figure 7). We found similar results when kriging RMS measures of Pg/Lg in various passbands. Thus, physical properties of the crustal waveguide in the Tibetan Plateau are responsible for the systematic pattern in the low-frequency Lg observations. Attenuation strong enough to account for the variation in spectra over long paths transiting central Tibet certainly requires more pronounced QLg values than previously reported. The next step in our analysis is to demonstrate whether this attenuation is uniform or needs to have particularly low values in the northernmost region in order to account for the rapid loss of high-frequency energy. 4. Determination of Lg Attenuation [20] Our observations of Lg spectral content shifting to lower frequency with increased path length in Tibet demonstrate a strong, progressive Lg attenuation in the crust beneath the plateau. Using a simple two-event method, we estimate Lg attenuation coefficient g( f ) for the paths crossing several sectors of Tibet. Some constraints are placed on regional heterogeneity of Lg attenuation. [21] The displacement spectral amplitude of the Lg wave arriving from a source at a distance d can be expressed in the form Að f ; d Þ ¼ Sð f ÞRð f ; qÞGðd Þ ð f ; qÞI ð f ÞSS ð f ; Þ; ð1Þ where f denotes the frequency, q the station azimuth, S( f ) is the source excitation function, R( f, q) is the source radiation pattern, G(d ) is the Lg geometrical spreading function, I( f ) is the instrument response, SS( f, ) is the station site response which can vary with the backazimuth, , ( f, q) is anelastic attenuation function which can be written by ð f ; qÞ ¼ egd ; ð2Þ where g is the attenuation coefficient , which is related to the quality factor Q and the group velocity U as g ¼ ð pf Þ=ðQU Þ: ð3Þ This parameter will account for both intrinsic attenuation and scattering attenuation losses. We assume a constant group velocity of 3.5 km/s, as this is generally consistent with the larger arrivals in the early part of the Lg wave train as seen in Figures 2 and 3, along with corresponding to Rayleigh overtone energy apparent in time-variable filtered plots of some of the signals. Certainly some error is incurred by assuming a single, somewhat uncertain group velocity for all frequencies, but the path geometry precludes a detailed analysis of individual modes as FAN AND LAY: CHARACTERISTICS OF Lg ATTENUATION IN THE TIBETAN PLATEAU necessary to do better. Given the interference effects of the multimode contributions to Lg, it is unlikely that a more robust group velocity behavior can be determined for our strongly attenuated data, given the present data distribution. [22] Restricting our attention to two events that lie within a few degrees of the great circle path connecting the receiver and the two epicenters, we obtain the ratio of Lg wave spectral amplitude for event 2 (the distant event) to that for event 1 (the nearer event) as Að f ; d2 Þ=Að f ; d1 Þ ¼ ½S2 ð f Þ=S1 ð f Þ½Gðd2 Þ=Gðd1 Þexp½g; ð4Þ Where the indices 1 and 2 represent event 1 and event 2, respectively, and is the distance between the two events. Note that the source radiation pattern R( f, q) does not appear in (4) because we adopt the common assumption that Lg source radiation is azimuthally independent to first order [Sereno et al., 1990; Shih et al., 1994]. This is the most difficult assumption to validate, and we rely on stacking of multiple ratios to overcome any bias due to neglect of azimuthal radiation effects. The site amplification term cancels out for small differences in event backazimuth. For the geometrical spreading function G(d ), we adopted G(d ) = d0.5, as appropriate for Lg waves analyzed in the frequency domain, (versus G(d) = d0.83 in the time domain) [Ewing et al., 1957; Campillo et al., 1984; Hasegawa, 1985; Chun et al., 1987; Shin and Herrmann, 1987]. The precise exponent to use for a laterally heterogenous structure is not clear, however, the study by Xie [2002] and our own calculations indicate that the choice of different reasonable geometrical spreading parameters does not lead to significant changes in QLg estimates. [23] To solve for the attenuation coefficient, we need to estimate the effects of the source excitation term S( f ), which can be represented by the w2 model as S ð f Þ ¼ S0 =ð1 þ f 2 =f c2 Þ; ð5Þ where S0 is a constant for a given event, and fc is the corner frequency. The radiation corner frequency fc is related to the stress drop, s, the shear wave velocity at the source, ub, and the seismic moment of the event, M0 [Brune, 1970]. If the difference in fc for the two events is small, then, as a first order approximation, (5) can be simply reduced to S( f ) ffi S0. One can assume constant stress drop and scale corner frequency with moment, but this is rather arbitrary given observed scatter in measured stress drops. Since our spectral ratios are extremely bandwidth limited by strong attenuation, we ignore small, high-frequency corrections and restrict our analysis to frequencies below 0.5– 1.0 Hz. Thus, we can rewrite (4) as Að f ; d2 Þ=Að f ; d1 Þ ¼ ½S02 =S01 ½d2 =d1 0:5 exp½g; ð6Þ and solve for the attenuation coefficient g(f ). Our simplified source correction is approximately equivalent to shifting the spectral ratio to a zero baseline at its low – ESE 14 - 9 frequency limit. We found that use of the seismic moments from the Harvard CMT solutions provided spectral ratios with small scatter for different event pairs with about the same magnitudes. Because not all of the events studied have Harvard CMT solutions available, we first constructed a reference spectral ratio curve by averaging all spectral ratios after source corrections. Other spectral ratios lacking moment information were then shifted relative to the reference spectral ratio by correlating over the frequency band of 0.2– 0.5 Hz. Finally, a stacked average is calculated from all spectral ratios for all event pairs to provide a representative Lg attenuation, g(f ), along a profile. [24] We constructed four profiles approximately in the north-south direction. Figure 8 shows the locations of selected events used for estimating Lg attenuation. The first three profile are positioned in the western, central, and eastern parts of the Tibetan Plateau, respectively, with events located near the southern and northern margins and the associated paths crossing the entire plateau (see Figure 8). The fourth profile covers a relatively small area in the central part of northern Tibet, where strong Lg attenuation was observed. In order to approximate great circle paths, only events with backazimuths confined to a range of 30 degrees are used in calculating g(f ). The number of events used for each profile is 4 3, 6 6, 4 7, and 5 6, respectively, where the first number represents the number of events in the north and the second is the number of events in the south. The events that have Harvard CMT solutions available were used in calculating the reference Lg attenuation curves, which are the average of many spectral ratios after source corrections for selected event pairs. The construction of a moment-corrected reference Lg attenuation curve is demonstrated in Figure 9. The source corrections do not eliminate scatter, but do appear to give a well-defined mean curve. Any additional ratios for which absolute amplitude information is lacking are correlated with the mean, shifted to that level and averaged in, mainly to smooth and stabilize the curve. In constructing reference attenuation curves, 15 event pairs were used for profile III, and 8 event pairs for profiles II and IV. For profile I, the reference curve was calculated using only three event pairs, and is thus less reliable. The spectral ratios are calculated out only to 1 Hz, given the low signal-to-noise ratio at higher frequencies. [25] The Lg attenuation coefficients g(f) for each profile show clear frequency dependence across the band of 0.1– 1.0 Hz (see Figure 10). Scatter in the 0.2– 0.5 Hz band was minimized by our processing. The largest scatter is observed for profile IV. In general, the Lg attenuation g(f) increases with frequency up to about 1 Hz for profiles I, II, and III and up to about 2 Hz for profile IV, then it gradually drops off. This drop off may be caused in part by lack of high-frequency source corrections, but mainly is due to high-frequency Sn coda appearing in the Lg window at large distances. The rate of increase in Lg attenuation g(f ) is not a constant function of frequency and differs for each profile. The highest attenuation and the best linearity for LOG[g(f )] of Lg are observed in profile IV, where rapid attenuation is observed across a short distance range. ESE 14 - 10 FAN AND LAY: CHARACTERISTICS OF Lg ATTENUATION IN THE TIBETAN PLATEAU Figure 8. A map showing locations of four profiles used for the Lg attenuation study. The event epicenters in each profile are shown by different symbols with triangles for profile I, circles for profile II and crosses for profile III. An expanded map on the top shows event locations (squares) for profile IV. Those squares with origin dates indicate events for which waveforms are shown in Figure 2. [26] Assuming a power law frequency-dependent model, Lg attenuation can be written in terms of quality factor QLg as QLg ð f Þ ¼ Q0 f h ; ð7Þ where Q0 is the value of QLg at 1 Hz, and h is the power law frequency dependence. Based on equations (3) and (7), we fit a QLg(f ) model to observed g(f ) to estimate the value of Lg attenuation in various areas of the Tibetan Plateau. Our data lack sufficient bandwidth and spatial sampling to pursue a separation of intrinsic and scattering attenuation effects. [27] The logarithmic Lg attenuation coefficients g(f ) are fit to a QLg(f ) model by least squaress linear regression in two frequency bands, 0.2– 0.5 Hz and 0.2– 1.0 Hz, for each profile. Figures 11a –11d show our results. The numerical values of the best fit model parameters Q0 and h are listed in Table 1. Previous research on Lg attenuation in Asia indicates that h is very sensitive to lateral hetero- geneity in the crust, thus reliable h estimates are difficult to obtain [Shih et al., 1994], particularly with band-limited data. [28] We found that Q0 values differ for each profile. There is little difference in Q0 for profile IV between the two best fit models because the logarithmic spectra are very linear. However, there are variations in the Q0 estimates for the other profiles between the 0.2 – 0.5 Hz and 0.2 – 1.0 Hz bands. Profiles II and III show a reduced slope in logarithmic g(f ) commencing at about 0.5 Hz. Thus, broader band estimates give higher Q0 values. We believe that this is likely due to contamination at higher frequencies (above 0.5 Hz) by increased contribution of high-frequency Sn coda rather than true Lg signals. The Q0 value of Lg for the Tibetan Plateau as a whole is in a range of about 120– 150 for the 0.2 – 0.5 Hz band, and in a range of 160 –230 for the 0.2– 1.0 Hz band based on the results for profiles I, II and III. Our observations indicate that a region in northern central Tibet close to the plateau margin is characterized by very FAN AND LAY: CHARACTERISTICS OF Lg ATTENUATION IN THE TIBETAN PLATEAU Lg Attenuation Coef. 0.015 0.010 0.005 0.000 -0.005 No Source Correction -0.010 10-1 a) 100 Frequency (Hz) Lg Attenuation Coef. 0.015 0.010 0.005 0.000 -0.005 After Source Correction -0.010 10-1 b) 100 Frequency (Hz) Figure 9. The construction of a reference Lg attenuation curve by averaging spectral ratios of 15 event pairs after simplified source corrections. Dashed lines are (a) observed spectral ratios of 15 event pairs, and (b) the same spectral ratios after simplified source corrections. Thick solid line in (b) represents the reference Lg attenuation curve, which is the average of all event pairs after simplified source corrections. strong Lg attenuation, with a Q0 value of 85– 90. This is consistent with observed high-frequency amplitude decay by a factor of ten or more in that region (see Figure 2). 5. Discussion [29] The Lg attenuation estimates obtained in section 4 are much lower than those discussed in the introduction, most of which are for eastern Tibet. One concern is that there is still some bias due to traversing the northern margin of Tibet despite our observation of progressive evolution of the Lg spectra. We thus consider Lg observations at station LSA, which is located within Tibet, for 31 events throughout the plateau, none of which have paths traversing the northern margin of the plateau. Figure 12 is a plot of observed apparent corner frequency versus path length from LSA, showing great similarity to the WMQ observations in eastern and western Tibet, with only the central part having a stronger pattern. We infer that paths to LSA sample Q0 attenuation values of 122 – 150 as in profiles I, II and III. Recently, Xie [2002] has reanalyzed the Lg spectra data used by McNamara et al. [1996], ESE 14 - 11 obtaining a QLg model with Q0 = (126 ± 9) and h = (0.37 ± 0.02), which is very consistent with our estimates in profiles II and III, where the data overlap (however, note that our estimates are for paths across the entire plateau). Xie’s estimate is for the 0.2 – 3.6 Hz band, with the extension to higher frequency being viable due to the short path lengths involved. This extrapolates smoothly up from our 0.2– 0.5 Hz band prior to the decrease in slope of LOG[g(f)]. Phillips et al. [2000] obtain tomographic models of Q0 with values of 200 in Tibet south of the Qaidam and Tarim basins. Their results give Q0 = 500 for the Tarim Basin, compatible with our observation of efficient propagation there. Their coverage of western Tibet is very limited due to constraining the data to 0.75– 1.5 Hz, which is strongly attenuated over longer paths in Tibet. [30] We resolve a region in northernmost Tibet with much lower QLg than previously reported by any study of Tibet. Figure 13 summarizes our Q0 estimates, illustrating the localized region with Q0 values of 85– 90. Profile II gives overall Q0 values of 141 for the 0.2 –0.5 Hz band, which requires that Q0 increase in southern central Tibet. Phillips et al. [2000] indicate such an increase in Q0 from north to south, with higher Q0 values of 450 – 500 south and east of Lhasa. We estimated QLg for a fifth profile using four southern events in profile IV as reference events relative to three events near the southern margin of the plateau. Fitting data in the 0.2– 0.5 Hz band gives an estimated Q0 value of 316 for the region from 35N to the southern margin of Tibet. This is very compatible with recent Lg analysis sampling to the west of LSA in the 0.5– 1.0 Hz band, which gives values of Q0 = 300– 350, somewhat reduced from the earlier results of Phillips et al. [2000] after elimination of events with uncertain mb values (S. Phillips, personal communication, 2002). Because the reference events in profile V are already attenuated significantly, we cannot extend our frequency band to higher frequency, but the consistency is encouraging. Our value for southern central Tibet is also consistent with the results of McNamara et al. [1996] and Reese et al. [1999], but our values are not as low as in the analysis by Xie [2002]. If the region of very low Q0 in northern Tibet extends further west and east than can be resolved by our data, there may also be north-to-south gradients in Q0 in western and eastern Tibet. Phillips et al. [2000] do not detect strong trends from north to south in these regions, but detailed work is needed. [31] Our low Q0 values of 85– 146 are comparable to Lg attenuation values found in other tectonically active areas, such as California [Herrmann, 1980; Nuttli, 1986] and Iran [Nuttli, 1980]. In the central Andes, where the crustal thickening is comparable to that in Tibet, an average Qs of 100 has been reported for the Bolivian Altiplano [Baumont et al., 1999]. The latter study interpreted the frequency-dependent attenuation of Lg as mainly being caused by strong crustal scattering, although a significant contribution from small amounts of partial melting in the crust was suggested. The similarity of Lg attenuation values in the Altiplano and in Tibet may suggest a common effect of thickened, deformed crust within major continental plateaus behind active mountain belts. The strong attenuation of Lg waves in Tibet and the ESE 14 - 12 FAN AND LAY: CHARACTERISTICS OF Lg ATTENUATION IN THE TIBETAN PLATEAU Profile II Lg Attenuation Coef. Lg Attenuation Coef. Profile I 0.010 0.005 0.000 -0.005 -0.010 10-1 0.010 0.005 0.000 -0.005 -0.010 100 10-1 Frequency (Hz) a Profile IV Lg Attenuation Coef. Lg Attenuation Coef. Profile III 0.010 0.005 0.000 -0.005 -0.010 10-1 100 Frequency (Hz) b 0.015 0.010 0.005 0.000 -0.005 100 10-1 Frequency (Hz) c 100 Frequency (Hz) d Figure 10. Lg attenuation coefficient g(f ) as a function of frequency for each profile. The dashed lines are calculated from the spectral ratio of each event-pair after simplified source correction, the solid line represents a stacked average for all Lg attenuation coefficient g(f ) observations in each profile. 10-2 Profile I scale crustal waveguide variations do not dominate the attenuation effect, it is certainly possible that scattering from small scale heterogeneity within the crust plays a role, similar to the Alpine environment [e.g., Campillo et Lg Attenuation Coef. Lg Attenuation Coef. very sparse station coverage preclude an attempt to apportion Lg attenuation estimates into intrinsic anelasticity versus small-scale scattering attenuation, as attempted in the Altiplano. While we have demonstrated that large 10-3 10-2 Profile II 10-3 100 100 Frequency (Hz) a b Profile III Profile IV Lg Attenuation Coef. Lg Attenuation Coef. Frequency (Hz) 10-3 10-2 100 Frequency (Hz) c 100 Frequency (Hz) d Figure 11. Lg attenuation coefficient g(f ) and the best fit QLg models (straight lines) for each profile. Crosses are g(f ) values used for the data fitting. Solid and dashed lines represent the best fit QLg models in frequency bands of 0.2 – 0.5 Hz, and 0.2– 1.0 Hz, respectively. FAN AND LAY: CHARACTERISTICS OF Lg ATTENUATION IN THE TIBETAN PLATEAU ESE 14 - 13 Table 1. Values of Lg Attenuation in Different Parts of Tibet Profile I Profile II Profile III Qo h 146 ± 20 0.67 ± 0.12 141 ± 17 0.15 ± 0.11 0.2 – 0.5 Hz 122 ± 20 0.19 ± 0.15 Qo h 160 ± 5 0.75 ± 0.04 224 ± 10 0.56 ± 0.06 0.2 – 1.0 Hz 195 ± 14 0.24 ± 0.08 al., 1993]. As improved resolution of Tibetan crustal complexity is achieved, it may become viable to assess the scattering contribution, but for this study it is lumped into the overall effective Lg attenuation. [32] The region of northern central Tibet where we find very strong effective attenuation is the most volcanically active area of Tibet [e.g., Molnar, 1988; Turner et al., 1993, 1996; Arnaud et al., 1992]. In general, mechanisms Profile IV Profile V 90 ± 20 0.15 ± 0.10 316 ± 31 0.40 ± 0.09 85 ± 2 0.10 ± 0.04 – – of intrinsic shear wave attenuation are very sensitive to temperature conditions, and the very low Qo of 85– 90 may be associated with partial melting of the crust in northern Tibet, for which there is some independent evidence. Owens and Zandt [1997] presented evidence for a lower crustal low-velocity zone likely to involve partial melt in northern Tibet. This region has inefficient Sn propagation [Ni and Barazangi, 1983; McNamara et Figure 12. Top figure is a topography map in western China and its vicinity. The location of station LSA is shown. The squares with crosses indicate the epicenters of the 31 events used in this study. Bottom figure shows apparent corner frequency of observed amplitude spectra versus distance from station LSA. The solid and dotted lines represent the regression line observed from stations LSA and WMQ, respectively. CC, linear correlation coefficients. ESE 14 - 14 FAN AND LAY: CHARACTERISTICS OF Lg ATTENUATION IN THE TIBETAN PLATEAU Figure 13. A summary map of Qo values estimated for different parts of Tibet. Thick solid lines are 3000-meter topographic contours, thin solid lines represent three subregions, where QLg values are estimated. The central corridor has very low Qo in the north and higher Qo in the south, with overall Qo values of 141– 224. The thick dashed line represents the region with inefficient Sn propagation based on the work of McNamara et al. [1995]; thin dashed lines are political borders. al., 1995], low Pn velocity [McNamara et al., 1997], and high Poisson’s ratios of 0.34 –0.35 over a 30 km thickness [Owens and Zandt, 1997]. Rodgers and Schwartz [1998] find very low Qs values of 44 – 89 in the Qiangtang Terrane, along with high Poisson’s ratio, which they attribute to partial melting of the crust. Our profile IV, which provides the lowest Qo values, samples the northern half of the Qiangtang Terrane. Figure 14 shows a north-south profile through Tibet adapted from Owens and Zandt [1997], indicating the coincidence of the proposed partial melt zone in the deep crust of northern Tibet and the region of low QLg. Further analysis is required to constrain the spatial extent of the very low QLg region, particularly its southward extent, but it is clear that Tibet cannot be viewed as a region with uniform Lg attenuation, nor as a region with Lg attenuation values only in the n ya ya th la Te ima H as h ay ig l H ima H er ys ss la Le ima H S [34] The Tibetan Plateau appears to have very strong attenuation of Lg phases for paths within and traversing the northern boundary of the plateau. This is demonstrated by the broadband spectral behavior of Lg, which undergoes a systematic shift of apparent corner frequency from 2 to 0.2 Hz as a function of path length. The apparent corner frequency shift is consistent with progressive energy losses proportional to path length within the plateau, and is particularly well correlated with physical properties of the plateau. Spectral ratios for various path geometries across Tibet indicate that Lg attenuation values at 1 Hz are on the order of Qo = 80– 90 in the northern central region of Tibet, near 316 in southern central Tibet and on the order of 122 – 195 for whole plateau averages in eastern and western Tibet. This implies that so-called blockage of Lg energy for paths in Tibet is mainly caused by very strong attenuation in the crust. The very low QLg values in northern Tibet may be a result of partial melt in the low-velocity layer in the lower crust. Qiangtang terrane Moho n ya ic re th Te ean phe Oc thos Li 200 240 km 200 Qaidam basin N 40 Indian Continental Lithosphere 100 Songpan-Ganz terrane Very low Lg Q Indian Crust 120 160 0 6. Conclusions MBT 40 80 Lhasa terrane Tsangpo Suture range of Qo = 340 – 450 as previously reported. There is some evidence for partial melt and crustal low-velocity zones existing north of the Tsangpo suture in southern Tibet [Nelson et al., 1996; Kind et al., 1996; Cotte et al., 1999]. This low-velocity zone may also relate to a localized low QLg region, however, it is not resolved by our data set due to lack of spatial resolution in southern Tibet. [33] Further work is also needed to constrain the depth distribution of attenuation in the crust, as QLg involves complex sampling of the crustal waveguide. With relatively low overall crustal velocities likely to exist in northern Tibet [e.g., Rodgers and Schwartz, 1998; Owens and Zandt, 1997], Lg waves may provide overall sampling of the thick crust, averaging the entire attenuation structure. Shallow crustal attenuation needs to be constrained by fundamental mode attenuation in order to establish the Qs structure of the upper and lower crust [e.g., Mitchell and Xie, 1994]. 300 400 500 Partially Molten Lower Crust 80 Inefficient Sn Asian Low Pn Velocity Continental Lithosphere 200 240 km 600 km Figure 14. A schematic north – south profile through Tibet adapted from Owens and Zandt [1997], indicating the coincidence of the partial melt zone in the deep crust of northern Tibet and the region of low QLg. FAN AND LAY: CHARACTERISTICS OF Lg ATTENUATION IN THE TIBETAN PLATEAU [35] Acknowledgments. We thank D. Baumgardt for sharing his unpublished work on Lg blockage in Tibet. Comments from S. 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(thorne@es.ucsc.edu) FAN AND LAY: CHARACTERISTICS OF Lg ATTENUATION IN THE TIBETAN PLATEAU Figure 7. A map showing interpolated estimates of apparent corner frequency for the Lg amplitude spectra for events in the Tibetan Plateau as observed at WMQ. Interpolation of the observations is done using a standard kriging algorithm. Small circles represent the event locations used in this study; thick solid lines are 3000-meter topographic contours. ESE 14 - 8