Source Parameters

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    ORIGINAL ARTICLE

    Source parameters and scaling relations for small

    earthquakes in Kumaon Himalaya, IndiaK. Sivaram & Dinesh Kumar & S. S. Teotia &

    S. S. Rai & K. S. Prakasam

    Received: 19 December 2011 / Accepted: 10 October 2012 / Published online: 28 October 2012# Springer Science+Business Media Dordrecht 2012

    Abstract We investigate the scaling relationships

    among earthquake source parameters using more than

    300 good quality broad band seismograms from 30

    small earthquakes in the Kumaon Himalaya from the

    spectral analysis of P and S waves. The average ratio

    of P/S wave corner frequency is found to be 1.13,

    which is suggestive of shift in the corner frequency.

    The estimated seismic moment range from 1.61013

    5.81015 Nm, while the stress drop varies from 0.6 to

    16 bars with 80 % of the events below 10 bars. An

    analysis of stress drop and apparent stress drop indi-cates the partial stress drop mechanism in the region.

    The source radii are between 0.17 and 0.88 km. The

    total seismic energy varies from 1.79108 to 7.30

    1011 J. We also observe the variation in seismic energy

    for a given seismic moment. The scaling relation be-

    tween the seismic moment and stress drop suggests the

    breakdown of constant stress drop scaling for the

    range of seismic moments obtained here for the re-

    gion. This shows the anomalous behavior of small

    earthquakes in the region. The study indicates that

    the stress drop is the dominant scaling factor for themoments studied here.

    Keywords Source parameters . Kumaon Himalaya.

    Small earthquakes . Scaling relations

    1 Introduction

    The Kumaon Himalaya region of the Himalayas is one

    of the youngest orogenic belts of the world, which has

    resulted by continuous tectonic collision of Indian

    plate with Eurasian plate since early Eocene. The

    arcuate Himalayan formation extends from the north-east to the northwest over a distance of about

    2,500 km. The study region, in the state of Uttarak-

    hand, India, falls in the central seismic gap between

    rupture zones of 1905 and 1934 great earthquakes

    (Khattri and Tyagi 1983; Khattri 1987). In addition,

    Bilham et al. (1997, 2001) suggest significant seismic

    potential for the Himalayan region between the west-

    ern Nepal and Western Himalaya. For the proper eval-

    uation of the seismic hazard potential in a region,

    determination of earthquake source parameters such

    as the seismic moment, stress drop, radiated seismicenergy, corner frequency, and rupture dimension pro-

    vides the basic building blocks. The ambient stress

    conditions and ranges of stress drop may vary for

    different regions. Therefore, the regional scaling rela-

    tions, instead of available global relations, are appro-

    priate to estimate the values of stress drop and fault

    dimensions. The developed scaling relations provide

    the information whether the stress drop is constant or

    not for the given range of seismic moments. A number

    J Seismol (2013) 17:579592

    DOI 10.1007/s10950-012-9339-y

    K. Sivaram (*) : S. S. Rai : K. S. PrakasamCSIR-National Geophysical Research Institute,

    Hyderabad, India

    e-mail: [email protected]

    D. Kumar: S. S. TeotiaDepartment of Geophysics, Kurukshetra University,

    Kurukshetra, India

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    of studies have been done to investigate the region-

    specific scaling of earthquakes, especially at lower

    magnitudes. (e.g., Abercrombie 1995; Prejean and

    Ellsworth 2001). In the Himalayan regions, Sharma

    and Wason (1994) have investigated the scaling rela-

    tions using 18 low magnitude, local events recorded

    by five vertical-component and two three-componentstations for Lower Himalayan regions. Using the 2

    source model, Sriram et al. (2005) have provided

    insights of earthquakes in some parts of Himachal

    Himalaya, whereas Kumar et al. (2006) have provided

    source parameter estimation for the 1999 chamoli

    earthquakes and nine of its aftershocks in Uttarakhand

    Himalaya using band-limited accelerograms. Kumar et

    al. (2008) suggested the self similar nature of Himala-

    yan earthquake sources with seismic moments in the

    range 1.4 10161.71019Nm. Their analysis is based

    on the 80 band-limited accelerograms of 12 earth-quakes in the Himalayan region.

    The study by Dysart et al. 1988 found different

    scaling relations for the small and large earthquakes

    in the same region. The purpose of this study is to

    determine the source parameters and investigate the

    possible sel f-similarity of small earthquakes for

    Kumaon Himalaya region using spectral analysis of

    the digital broadband waveforms of 30 earthquakes

    recorded over a seismograph network operated by

    the CSIR-National Geophysical Research Institute,

    from April 2005 to June 2008. The 2

    scaling model(Aki 1967; Brune 1970, 1971; Houston and Kanamori

    1986; Boore 1986) has been used for this purpose in

    the present study. In the following sections, we first

    describe the geological framework and seismotecton-

    ics of the study region, followed by dataset preparation

    and methodology of spectral analysis, the source

    par amete rs and scaling rel ati ons, and final ly the

    conclusions.

    2 Geological framework and seismotectonicsof the study region

    The Kumaon Himalayan region (latitude, 29 N

    31 N; longitude, 78 E81 E) forms a part of the

    Himalayas, which has resulted from a long geolog-

    ical evolution, after the closure of the Tethys Ocean

    and the underthrusting of the Indian with the Eur-

    asian continental plate. Figure 1 shows the surface

    trace of major tectonic features of the region that

    includes the Southern Tibetan Detachment (STD),

    the Main Central Thrust (MCT), the Main Bound-

    ary Thrust (MBT), and the Main Frontal Thrust

    ( M FT ) . T h e L ow e r H i ma l ay a i s s tr u ct u ra ll y

    bounded by MBT and MCT, consists mainly of

    Precambrian clastic sediments. The greater Hima-

    laya is bounded by MCT and STD and comprisesof early Cambrian metasedimentary rocks. Over the

    past 200 years, nearly half of the Himalayan belt

    has ruptured in at least six great earthquakes that

    occurred in 1803, 1833, 1897, 1905, 1934, and

    1950. Various seismo-tectonic models have been

    proposed for explaining the evolution and seismic-

    ity of the Himalayas (Seeber and Armbuster 1981;

    Ni and Barazangi 1984; Molnar and Chen, 1982;

    Yin and Harrison 2000). It is a well-accepted fact

    that most of the earthquakes recorded here tend to

    be shallow and restricted to a seismogenic zonewithin the upper ~25 km of the crust. Whereas

    the study region is experiencing low to moderate

    seismicity, a few recent moderate earthquakes being

    the Uttarkashi (M6.6, 1991), Chamoli (M6.3, 1999)

    earthquakes, the adjoining Himalayan regions have

    experienced bigger earthquakes (Kashmir, M7.6,

    2005, and Wenchuan, M8.0, 2008). Due to the

    varying ambient stress conditions and absence of a

    large magnitude seismic event in the region for a

    long time, the seismic risk potential is enhanced

    across Kumaon Himalaya region.

    3 Data set

    The study is based on the broad band seismograms

    recorded during April 2005June 2008 at a broadband

    seismograph network operated in Kumaon Himalaya re-

    gion by the CSIR- National Geophysical Research Insti-

    tute, under a project grant by Department of Science and

    Technology, New Delhi, India (Ashish et al 2009;

    Mahesh et al. 2013). Figure 1 shows the seismic networkof the study stations along with the major tectonic features

    and the epicenters of the earthquakes. Table 1 shows the

    details of the earthquakes considered in this study. The

    seismograph stations were equipped with Guralp CMG-

    3T triaxial broadband seismometer [with a flat velocity

    response in the frequency range of 0.0083 Hz (120 s

    period) to 50 Hz] coupled to 24-bit Reftek RT-130/1

    digital data acquisition system and synchronized by glob-

    al positioning system (GPS). The stations used in the

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    study were located on rock profiles and observed to have

    minimum noise interference. The data have been

    recorded at a sampling rate of 50 samples/s, and all the

    stations were synchronized to operate in a continuous

    mode. The earthquakes with focal depth

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    spreading, 0 is long period spectral level, Q is

    quality factor, fc is corner frequency, and R is

    source receiver distance. GS(R)0R1 for RRy

    and GS(R)0(RRy)0.5

    for R>Ry. Ry may be takenas twice the thickness of crust (Herrmann and

    Kijko 1983). In this study Ry has been taken as

    100 km corresponding to a crustal thickness of

    50 km (Singh et al. 2002; Rai et al. 2009) for

    the Himalaya. Our frequency analysis lies in the

    wider frequency band 0.220 Hz, as the maximum

    cut-off frequency for the seismometer is 50 Hz.

    We recognize here that we are neglecting the high

    frequency decay parameter in Eq. (1), for which,

    the spectra have been fitted in the frequency band

    of 0.210 Hz. Another reason for this choice, as

    discussed below, is that the constant Q model has

    been preferred in the present analysis.The term exp (ft/Q) represents the attenua-

    tion of seismic waves (Dainty 1981; Fletcher

    1995). A constant Q model, considered as path

    averaged Q, has been adopted for the relatively

    narrow frequency band of 0.210 Hz. The model

    has been found to be satisfactory in many studies

    (e.g., Kjartansson 1979; Masuda and Suzuki 1982;

    Archuleta 1982; Archuleta and Hartzell 1981;

    Anderson and Hough (1984); De Natale et al.

    Table 1 The earthquakes and

    the number of recording stations

    used in the present study

    Event number Latitude

    ( N)

    Longitude

    ( E)

    Depth

    (km)

    mb

    (USGS)

    Number of recording

    stations used for analysis

    1 31.56 79.57 12.6 3.5 9

    2 30.44 79.25 13.4 4.6 8

    3 30.38 79.31 20.0 3.8 9

    4 30.53 81.40 11.0 3.9 75 30.3 80.95 4.6 4.9 13

    6 30.32 80.96 4.6 3.8 14

    7 30.45 79.23 19.3 5.3 12

    8 30.47 79.23 14.4 3.7 13

    9 30.36 80.13 11.6 4.9 16

    10 30.41 80.15 17.6 4.5 16

    11 30.37 80.10 13.8 3.6 17

    12 31.74 77.20 4.5 3.9 18

    13 29.44 76.54 25.3 4.3 17

    14 32.31 77.78 18.5 4.2 18

    15 31.49 78.50 17.9 4.0 19

    16 31.48 78.46 6.0 3.5 19

    17 31.52 78.43 3.2 3.5 15

    18 30.02 80.52 20.5 3.8 19

    19 27.77 76.39 14.0 3.8 19

    20 31.13 80.21 14.6 3.9 21

    21 31.84 78.87 3.3 4.7 20

    22 31.24 77.80 9.5 4.1 17

    23 29.59 81.27 7.6 4.6 19

    24 30.93 78.28 4.4 3.9 20

    25 32.1 76.93 1.4 4.3 19

    26 30.33 80.31 3.6 3.9 12

    27 30.83 78.41 8.4 5.1 9

    28 30.94 78.26 3.1 3.8 10

    29 28.76 77.37 8.0 4.7 21

    30 31.38 77.35 8.9 3.4 18

    582 J Seismol (2013) 17:579592

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    1987; M en ke e t a l. 1995; Abercrombie 1995;

    Prejean and Ellsworth 2001; Kumar et al. 2006;

    Tomic et al. 2009). Anderson and Hough (1984)

    h av e s ho wn t ha t t he m od el o f a f re qu en cy -

    independent Q for the shallow crust is consistent

    with a 2 Brune source model. The fitting of the

    Brunes model to the observed spectra, as dis-

    cussed below, shows adequacy of constant Q

    model in the frequency range of 0.210 Hz for

    the region.

    Three parameters0, Q, and fcare required to

    define the source spectrum described by Eq. (1). The

    simultaneous estimation of these three parameters may

    lead to biasness because of tradeoff between Q and fcas well as between 0 and Q. Therefore, the corner

    frequency has been estimated separately, in the wider

    frequency band, and other two parameters0 and Q

    have been determined using the grid search method.

    Many methods have been proposed to estimate the

    critical parameter fc (Brune 1970; Andrews 1986;

    Snoke 1987; Margaris and Boore 1998; Shi et al.

    1998). The Snokes method (Snoke 1987) requires

    two parameters: long period spectral level 0 and the

    energy flux J (integral of square of the ground

    velocity). The value of 0 may be estimated either

    from the known seismic moment of the earthquake

    or by the visual inspection of the displacement

    spectrum. The Andrewss approach (Andrews

    1986) requires two spectral parametersJ a n d K (integral of square of ground displacement)to

    determine the corner frequency. Garca et al.

    (2004) have found that both approaches provide

    similar values. In order to avoid the possible error

    due to visual inspection of 0, the corner frequen-

    cy in the present study has been determined using

    Andrews (1986) approach. This approach helps

    significantly minimizing the error associated with

    the visual estimation of corner frequency, fc, given

    by:

    fc

    ffiffiffiffiffiffiffiffiffiffiffiffiS

    V2

    SD2

    r2p

    2

    where SV2 and SD2 are evaluated using the follow-

    ing integrals:

    SV2

    Z10

    V2fdf 3

    And

    SD2

    Z10

    D2fdf 4

    where V(f) and D(f) are the velocity and displacement

    spectra, respectively, and V0(f) and D0(f) are the cor-rected velocity and displacement spectra, respectively,

    as described below. The corner frequency has been

    estimated using the wider frequency band (0.220 Hz)

    of the spectra.

    A two-step search procedure for determining the

    optimum values of the parameters 0 and Q has been

    applied while adopting the corner frequency obtained

    as noted above (Kumar et al. 2006). In the first step,

    the values of the parameters 0 and Q are allowed to

    vary over the search space. Ten trial values per decade

    were chosen for0 and Q was allowed to vary from100 to 2,000. In the next step, a search was conducted

    for 0 around the value obtained in the previous

    search while keeping the value of Q obtained in the

    first step. The updated value of0 thus obtained was

    used for further analysis. A least square error function,

    Eis defined between the fitted Brune spectra, D(f) and

    the observed spectra, D0(f):

    E 1

    n

    XlogDf logD0f

    2 5

    where n is the number of spectral values of the dis-placement spectra.

    The values of fc and 0 obtained from the best-

    fitted Brune spectra are used to estimate the source

    parameters at the recording stations. The seismic mo-

    ment (M0), source radius (r), stress drop (), and

    moment magnitude (Mw) of an earthquake at the re-

    cording stations have been obtained using the expres-

    sions (Keilis-Borok 1960; Haskell 1964; Brune 1970,

    1971; Hanks and Kanamori 1979):

    M0p s=

    4pv3

    FPRf

    p s=0 6

    rp s= Kv

    2pfp s=

    c

    7

    p s= 7

    16

    Mp s=0

    r3p s=

    8

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    Mp s=w log10 M

    p s=0

    1:5

    10:7 9

    where Mp s=0 ,

    p s=0 , rp/s,f

    p s=c ,

    p/s, and Mp s=w are seismic

    moment, long period spectral level, source radius, cor-

    ner frequency, stress drop, and moment magnitude ofthe P or S waves, respectively; is the average density

    (02.67 g/cm3); Pis partition of energy (01/2); Kis the

    constant (2.34 for S waves and 1.92 for P waves); vis the

    shear wave velocity (03.46 km/s) or P wave velocity

    (06.07 km/s), Fis the free surface effect (02) and R

    is the average radiation pattern (00.52 for P waves and

    00.63 for shear waves). The radiated seismic energy has

    been estimated from moment rate spectra using the fol-

    lowing relation (Vassiliou and Kanamori 1982):

    ER AZ1

    0

    2pfMp0 f

    2df BZ

    1

    0

    2pfMs0f 2

    df

    10

    where A0(155)1 and B0(10

    5)1. The P and S

    wave radiated seismic energy have been estimated from

    the first and second term of above equation.

    Table 2 Earthquake source parameters obtained from the analysis of P waves

    Event

    number

    fc(P)

    (Hz)

    SD Mo

    (P) (Nm)

    SD r(P)

    (m)

    SD (P) (bars)

    SD Mw SD Qp SD Ep (J) SD

    1 1.998 0.094 1.47E+14 0.257 1118.60 0.094 0.461 0.349 3.399 0.022 1225.08 0.054 3.45E+07 0.313

    2 3.083 0.115 7.19E+14 0.319 821.34 0.122 5.675 0.653 3.856 0.025 1144.45 0.110 3.01E+09 0.487

    3 3.097 0.122 4.50E+14 0.201 721.50 0.122 5.243 0.434 3.724 0.016 1096.90 0.092 1.20E+09 0.319

    4 2.549 0.118 1.39E+14 0.227 876.70 0.118 0.903 0.423 3.379 0.029 1190.87 0.059 6.38E+07 0.325

    5 1.493 0.161 3.41E + 14 0 .279 154.90 0.161 0 .559 0.983 3.617 0.060 927.81 0.160 7.71E + 07 0.631

    6 2.021 0.099 4.84E + 14 0 .196 958.20 0.099 2 .408 0.451 3.745 0.015 601.52 0.117 3.86E + 08 0.324

    7 2.682 0.097 4.90E+15 0.122 731.60 0.097 54.785 0.327 4.416 0.008 779.61 0.156 9.23E+10 0.226

    8 3.511 0.140 2.87E + 14 0 .245 599.10 0.140 5 .839 0.382 3.592 0.020 706.81 0.091 7.09E + 08 0.313

    9 2.407 0.105 2.46E+15 0.128 1010.00 0.109 10.430 0.424 4.216 0.009 997.99 0.236 1.68E+10 0.276

    10 2.781 0.092 1.07E+15 0.294 826.20 0.092 8.282 0.519 3.972 0.021 808.57 0.183 4.89E+09 0.407

    11 3.112 0.112 2.23E+14 0.342 749.20 0.112 2.322 0.571 3.515 0.030 1112.42 0.152 2.99E+08 0.45612 4.582 0.084 4.72E+13 0.326 560.60 0.084 1.173 0.299 3.067 0.030 1274.54 0.045 4.27E+07 0.313

    13 2.601 0.106 1.06E+14 0.107 804.00 0.106 0.891 0.360 3.306 0.009 1337.52 0.030 3.92E+07 0.234

    14 2.542 0.112 4.42E+13 0.157 755.70 0.112 0.465 0.234 3.052 0.015 1254.30 0.046 6389871 0.195

    15 2.566 0.169 5.92E+13 0.266 840.30 0.169 0.437 0.870 3.114 0.061 1015.14 0.108 1.18E+07 0.568

    16 2.838 0.153 1.35E+14 0.434 807.60 0.153 1.123 0.733 3.366 0.040 1232.08 0.056 8.32E+07 0.583

    17 2.732 0.148 1.17E+14 0.139 904.90 0.126 0.692 0.491 3.335 0.012 1122.69 0.129 5.57E+07 0.315

    18 2.722 0.130 5.47E+13 0.404 913.10 0.130 0.314 0.238 3.106 0.037 1043.08 0.130 1.20E+07 0.324

    19 2.094 0.164 1.41E+14 0.241 853.80 0.164 0.389 0.293 3.386 0.020 1210.83 0.060 3.62E+07 0.267

    20 3.249 0.506 1.49E+14 0.242 850.40 0.155 1.061 0.505 3.403 0.021 1039.07 0.101 1.52E+08 0.373

    21 2.254 0.149 1.03E+14 0.184 1092.40 0.149 0.344 0.593 3.295 0.016 1056.81 0.182 2.40E+07 0.389

    22 3.367 0.091 2.11E+14 0.308 636.70 0.091 3.580 0.518 3.502 0.026 1269.15 0.065 3.39E+08 0.413

    23 2.956 0.158 1.17E+14 0.385 624.90 0.158 2.089 0.390 3.323 0.040 1379.40 0.014 6.98E+07 0.387

    24 3.922 0.199 8.88E+13 0.263 550.10 0.199 2.334 0.763 3.252 0.023 680.19 0.368 9.48E+07 0.513

    25 3.607 0.302 1.39E+13 0.164 912.10 0.302 0.449 0.776 2.717 0.017 1127.88 0.072 672677.4 0.470

    26 2.593 0.180 3.49E+13 0.311 658.60 0.182 0.535 0.468 2.978 0.034 1109.56 0.118 1.29E+07 0.390

    27 3.761 0.156 7.69E+15 0.251 998.90 0.156 33.740 0.357 4.540 0.027 1210.83 0.060 8.42E+10 0.304

    28 1.927 0.154 1.83E + 14 0 .45 761.60 0.152 1 .812 0.340 3.454 0.039 994.34 0.051 9.85E + 07 0.395

    29 2.454 0.136 1.83E+14 0.249 829.00 0.136 1.403 0.351 3.461 0.021 1298.46 0.024 5.65E+07 0.300

    30 2.042 0.191 5.04E+13 0.231 752.00 0.191 0.519 0.377 3.089 0.022 1155.42 0.043 6844693 0.305

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    The average values () and standard deviations SD

    (log ) of seismic moment, source radius, stress drop,

    and seismic energy have been obtained using the fol-

    lowing expressions (Archuleta et al. 1982):

    by anti log1

    Ns XNs

    i1

    logyi 11

    SD logby 1Ns 1

    XNsi1

    logyi logby 2" #1

    2

    12

    where Ns is number of stations used for analysis. The

    average values have been obtained using P and S

    waves separately for each of the 30 events used in

    the analysis.

    5 Results and discussion

    Table 1 shows the details of the earthquakes consid-

    ered in this study. The average values of parameters

    estimated from the analysis of P and S waves are given

    in Tables 2 and 3 respectively. Figure 2 shows the

    Table 3 Earthquake source parameters obtained from the analysis of S waves

    Event

    number

    fc(S)

    (Hz)

    SD Mo

    (Nm)

    SD r(S)

    (m)

    SD (S)(bars)

    SD Mw SD Qs SD Es (J) SD

    1 1.826 0.112 1.09E+14 0.130 610.2 0.113 1.369 0.238 3.190 0.012 1319.844 0.028 1.44E+08 0.239

    2 2.437 0.091 6.27E+14 0.458 467.7 0.091 22.929 0.463 3.766 0.036 1023.130 0.232 1.95E+10 0.598

    3 2.461 0.115 3.75E+14 0.190 476.1 0.115 12.162 0.322 3.606 0.015 1235.850 0.040 6.28E+09 0.333

    4 2.637 0.032 8.99E+13 0.132 450.6 0.032 1.943 0.138 3.028 0.013 1400.000 0.000 1.42E+08 0.176

    5 1.508 0.149 2.98E+14 0.327 202.6 1.416 3.785 0.585 3.557 0.026 1101.510 0.089 1.05E+09 0.593

    6 2.125 0.158 3.21E+14 0.081 531.7 0.158 4.566 0.510 3.420 0.007 1156.600 0.100 1.11E+09 0.384

    7 2.23 0.155 4.20E+15 0.419 534.0 0.155 100.686 0.705 4.312 0.029 1276.060 0.039 6.38E+11 0.731

    8 2.881 0.085 2.53E+14 0.139 362.7 0.085 20.177 0.191 3.517 0.012 1228.910 0.066 5.42E+09 0.215

    9 2.166 0.085 1.65E+15 0.282 552.3 0.123 21.856 0.486 3.903 0.021 757.540 0.170 3.37E+10 0.499

    10 2.626 0.109 5.75E+14 0.236 461.0 0.109 3.699 0.378 3.232 0.021 1086.820 0.076 5.82E+08 0.399

    11 2.913 0.221 1.67E+14 0.334 482.5 0.221 4.294 0.595 3.312 0.029 1022.080 0.138 1.41E+09 0.60412 3.149 0.109 6.32E+13 0.174 384.1 0.109 6.11 0.269 3.221 0.016 1274.540 0.045 9.16E+08 0.288

    13 2.107 0.077 1.86E+14 0.329 543.0 0.064 7.286 0.426 3.569 0.026 1252.560 0.053 3.11E+09 0.491

    14 1.755 0.069 1.08E+14 0.320 836.0 0.069 1.293 0.718 3.443 0.027 1109.560 0.119 7.55E+08 0.675

    15 2.347 0.090 8.23E+13 0.135 537.3 0.090 2.975 0.329 3.304 0.012 983.800 0.088 6.73E+08 0.302

    16 2.56 0.134 1.21E+14 0.192 535.4 0.134 3.047 0.376 3.307 0.017 1133.600 0.106 8.98E+08 0.369

    17 2.409 0.142 9.05E+13 0.369 560.0 0.142 1.592 0.297 3.153 0.033 845.150 0.174 2.67E+08 0.433

    18 2.423 0.135 4.80E+13 0.122 658.8 0.135 0.632 0.384 3.033 0.012 1065.420 0.082 1.13E+08 0.329

    19 2.087 0.106 1.05E+14 0.118 314.0 0.106 1.307 0.272 3.182 0.011 1144.720 0.080 2.03E+08 0.254

    20 2.91 0.145 1.11E+14 0.199 566.6 0.145 1.769 0.621 3.199 0.018 1232.080 0.056 6.24E+08 0.533

    21 1.963 0.130 1.01E+14 0.287 678.5 0.130 1.332 0.504 3.271 0.026 1062.170 0.089 3.48E+08 0.515

    22 3.079 0.113 1.96E+14 0.152 388.8 0.113 13.447 0.326 3.460 0.013 1377.990 0.026 4.46E+09 0.311

    23 2.56 0.114 2.00E+14 0.059 413.8 0.114 17.463 0.392 3.591 0.005 1134.430 0.141 6.28E+09 0.293

    24 3.255 0.178 8.23E+13 0.164 433.9 0.178 4.056 0.487 3.190 0.013 1147.560 0.097 9.26E+08 0.423

    25 2.435 0.203 1.57E+13 0.464 619.6 0.203 4.954 0.289 2.774 0.047 1244.980 0.045 2.08E+07 0.489

    26 3.046 0.160 5.72E+13 0.217 487.0 0.160 3.011 0.376 3.221 0.019 1013.720 0.076 8.37E+08 0.386

    27 2.066 0.123 5.78E+15 0.325 526.7 0.123 115.893 0.132 4.345 0.022 1053.540 0.101 6.19E+11 0.297

    28 2.43 0.123 1.28E + 14 0.511 657.8 0.125 1.11 0.269 3.186 0.041 972.800 0.060 3.53E + 08 0.507

    29 1.853 0.125 2.78E+14 0.280 540.3 0.068 11.194 0.364 3.667 0.022 849.930 0.128 4.15E+09 0.418

    30 2.848 0.163 5.07E+13 0.351 340.0 0.163 3.493 0.517 3.088 0.034 1210.830 0.060 2.82E+08 0.564

    J Seismol (2013) 17:579592 585

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    fitting of Brune displacement spectra obtained

    from estimated parameters to the observed spectra

    as an example. The agreement between the Brune

    spectra and the observed spectra, in general, is

    good for the frequencies up to about 10 Hz, be-

    yond which the observed spectra show a more

    rapid fall off. This represents the characteristic fall

    off of source spectrum (Hanks 1981). The ob-

    served spectra are higher as compared to the

    Brune spectra in narrow frequency bands at some

    stations. These are possibly caused by the site

    amplifications. Overall, the agreement between

    the observed and estimated spectra indicates that

    the estimated parameters are well constrained.

    0.0001

    0.001

    0.01

    0.1

    1

    10

    100

    1000

    AMPLIT

    UDE

    SPECTRA

    0.001

    0.01

    0.1

    1

    10

    100

    1000

    0.0001

    0.001

    0.01

    0.1

    1

    10

    100

    1000

    AMPLITUDES

    PECTRA

    0

    0.0001

    0.001

    0.01

    0.1

    1

    10

    100

    1000

    ALI BNK

    GTHHLG

    FREQUENCY (Hz)

    0.0001

    0.001

    0.01

    0.1

    1

    10

    100

    1000

    AMPLITUDE

    SPECTRA

    1 10 100 1 10 100

    1 10 100 1 10 10

    1 10 100 1 10 100

    FREQUENCY (Hz)

    0.001

    0.01

    0.1

    1

    10

    100

    1000KSL KTD

    Fig. 2 Examples of fitting

    of Brune displacement

    spectra obtained from esti-

    mated parameters to the ob-

    served spectra

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    Figure 3 shows the comparison between the es-

    timated P and S wave corner frequencies. The

    estimated values of P wave corner frequency,

    fc(P), are in the range of 1.494.58 Hz, while those

    of S wave corner frequency, fc(S), vary from 1.51

    to 3.26 Hz. The ratios of P wave corner frequency

    to S wave corner frequency, fc(P)/fc(S), are withinthe range of 0.721.46 with an average of 1.13.

    This is lower than the ratio / expected for simple

    source model. This may be due to nondouble cou-

    ple source and/or specific takeoff angle of observa-

    tion. For more than 80 % of events studied here,

    the ratio is >1 and bounded between the lines

    fc(P)0fc(S) and fc(P)0(/)fc(S) (Fig. 3). Similar

    observations have been made in a number of stud-

    ies and is attributed to enrichment of P waves in

    high frequency compared to the S waves for the

    same earthquake (e.g., Furuya, 1969; Masuda andTakagi 1978; Hanks 1981; Majer and McEvilly

    1979; Fletcher 1980; Somerville et al. 1980; Prieto

    et al. 2004). Based on the analysis of spectra of

    earthquakes in the magnitude range of 0.54.5,

    Molnar et al. (1973) observed that the corner fre-

    quency for P waves is systematically larger than

    that for S waves for the physically reasonable dis-

    location models. Upadhyay and Duda (1980) found

    that the corner frequencies for P waves are about

    twice those for S waves for Himalayan earthquakes.

    This phenomenon of corner frequency shift has

    been reported even when attenuation is accounted

    for (Hanks 1981; Fletcher and Boatwright 1991;

    Abercrombie 1995; Garca et al. 2004). Hanks

    (1981) concluded on the basis of spectral analysis

    and time-domain modeling that the corner frequen-cy shift is the manifestation of an intrinsic prop-

    erty of earthquakes, source finiteness. The average

    values of source radii vary from 179 to 885 m.

    The mean ratio r(P)/r(S) is found to be 1.5, sim-

    ilar to those obtained by Garca et al. 2004. The

    difference in the estimated values of source radii

    from P and S waves may be due to corner fre-

    quency shift.

    The seismic moments estimated from P waves,

    M0(P), range from 1.391013 to 7.691015Nm and

    those from S waves, M0(S), range from 1.571013

    to5.781015N m. The corresponding moment magni-

    tudes range from 2.98 to 4.54 for P waves and from

    2.77 to 4.35 for S waves. The average ratio M0(P)/

    M0(S) is 1.04 (Fig. 4). The agreement between the

    seismic moments estimated from two waves indicates

    the validity of the procedure adopted in this study.

    The total seismic energy, estimated for the frequen-

    cy band 0.210 Hz, varies from 2.15107 to 7.30

    1011J. We note here that the total seismic energy may

    be underestimated here due to the limited frequency

    band used. Figure 5 shows the correlation between P

    1 2 3 4 5

    S-wave corner frequency, fc (S), (Hz)

    1

    2

    3

    4

    5

    P-wave

    cornerfrequency,

    fc(

    P),(Hz) f

    c(P)/

    f c(S)

    =1.

    7

    fc(P)/f

    c(S)

    =1

    Fig. 3 Comparison between P and S waves corner frequencies.

    The solid lines represent different scaling factors

    1E+013 1E+014 1E+015 1E+016

    seismic moment M0 (S) N-m

    1E+013

    1E+014

    1E+015

    1E+016

    seismic

    momentM0(P)N-m

    Fig. 4 Correlation between the seismic moments estimated

    from P and S waves along with the least square fitted line

    J Seismol (2013) 17:579592 587

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    and S wave energy with the lines of equal energy

    ratios. We note that that almost all the events lies

    between the energy ratio E(P)/E(S) of 0.011. Similar

    results are obtained by Fletcher and Boatwright 1991;

    Garca et al. 2004.

    T he m ea n s tr es s d ro p v ar ie s f ro m 0 .6 t o16 bars. More than 80 % of the events analyzed

    here show the average stress drop values

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    stress drop scaling for small earthquakes in the region.

    A decrease in stress drop with decreasing seismic

    moment has been found to be a scaling relation for

    small earthquakes (e.g., Archuleta et al. 1982; Haar et

    al. 1984; Dysart et al. 1988; Abercrombie 1995; Garca

    et al. 2004; Ide et al. 2003; Mayeda et al. 2005;

    Venkataraman et al. 2006). The plot of source radius with

    seismic moment is shown in Fig. 8 along with the lines of

    constant stress drop. We note that most of the events

    (>70 %) analyzed here lie in the stress drop values

    1E+013 1E+014 1E+015 1E+016

    Seismic moment (N m)

    0

    0.4

    0.8

    1.2

    1.6

    2

    ZunigaParameter,

    1

    23

    4

    5

    6

    7

    8 9

    10

    11

    12 13

    14

    15

    16

    17

    18

    19

    2021

    22

    23

    24

    25

    26

    27

    28 29

    30

    Partial Stress drop

    Frictional Overshoot

    Fig. 6 Ziga parameter, ,

    for the events with respect to

    moment. The corresponding

    event numbers are indicated

    below the solid blue circles

    0.1 1.0 10.0 100.0

    stress drop (bars)

    1E+13

    1E+14

    1E+15

    1E+16

    seis

    micmoment(N-m)

    Fig. 7 Relation between seismic moment and static stress drop

    along with the least square fitted line

    0001001

    source radius (m)

    1E+013

    1E+014

    1E+015

    1E+016

    seism

    icmoment(Nm)

    1 bar

    (0.1MP

    a)

    10bar (

    1 MPa

    )

    40bar (

    4 MPa

    )

    Fig. 8 Seismic moment versus source radius along with the

    lines of constant stress drop

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    between 1 and 10 bars. The source radius appears to be

    uncorrelated with the moment in this analysis, and there is

    a scatter in the values of source radius for the same

    moment. This observation, together with the observed

    increase in stress drop with seismic moment for Kumaon

    Himalaya, is evidence for the breakdown of the concept of

    similarity among smaller earthquakes. This breakdown ofsimilarity may be attributed to the anomalous behavior of

    small earthquakes that shows the corner frequencies are

    independent of moment/magnitude (e.g. Frankel 1981;

    Takeo 1983; Dysart et al. 1988; Mayeda et al. 2005;

    Venkataraman et al. 2006). Studies citing similar results

    by Okada et al. 1981 and Takeo (1983) reported a group

    of earthquakes with moments differing by up to a factor of

    1,000 but with essentially identical corner frequencies.

    Aki (1984) interpreted these events as examples of

    barrier-type earthquakes where stable regions on the fault

    plane can limit the extent of fracture but allow variableslip. However, the role of site effects needs to be investi-

    gated especially, in the light of the variation of source radii

    for the events of similar moments in the region.

    Kumar et al. (2008) suggested the self-similar na-

    ture of Himalayan earthquake sources with seismic

    moments in the range of 1.410161.71019N m.

    Their analysis is based on the 80 accelerograms of

    12 earthquakes in the Himalayan region. The present

    analysis suggests the breakdown of similarity of the

    earthquakes with seismic moments in the range 1.6

    1013

    5.81015

    Nm in the Kumaon Himalaya.Figure 9 shows the plot of the total seismic

    energy versus seismic moment along with the lines

    of constant apparent stress drop. This shows the

    energy may vary for a given seismic moment.

    Garca et al. 2004 have found the similar observa-

    tion for the earthquakes in the region of Granada

    Basin (Southern Spain).

    6 Conclusions

    Based on the source parameters estimated from the

    spectral analysis of P and S wave digital broad-

    band records of 30 events from Kumaon Hima-

    laya, we draw the following inferences. The

    agreement between the seismic moments from P

    and S waves and good fitting of theoretical Brune

    spectra to the observed one justifies robustness of

    the methodology. One of the important findings of

    present analysis is the breakdown of the constant

    stress drop scaling for the earthquakes with seis-mic moments in the range of 1.610135.81015N

    m in the region. The low stress drop values esti-

    mated in the study can be explained by partial

    stress drop mechanism in the region. A phenome-

    non of corner frequency shift has been observed in

    the region in consistent with the similar studies of

    other active regions. The estimated source radii are

    found to be uncorrelated with the seismic moments

    showing the corner frequency independence of

    seismic moments for the small earthquakes ana-

    lyzed here. The increase in stress drop with in-creasing moment and noncorrelation of source

    radius with seismic moment shows that the stress

    drop is the dominant scaling factor for moments

    1.0E+7 1.0E+8 1.0E+9 1.0E+10 1.0E+11 1.0E+12

    Seismic Energy (J)

    1.0E+11

    1.0E+12

    1.0E+13

    1.0E+14

    1.0E+15

    1.0E+16

    1.0E+17

    1.0E+18

    SeismicMom

    ent(N-m)

    0.5bar

    10ba

    r

    Fig. 9 Total seismic energy

    versus seismic moment

    along with the lines of ap-

    parent stress drop. These

    lines show the range of en-

    ergy variation for a given

    seismic moment

    590 J Seismol (2013) 17:579592

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    considered here. This has important bearing on the

    estimates of seismic hazard in the region as the stress

    drop controls the high frequency ground motions.

    Acknowledgments The above project was sanctioned from

    the grants by the Department of Science & Technology, India

    to CSIR-National Geophysical Research Institute (NGRI),

    Hyderabad, India (Research grant: DST/MMS-2/SU/2003).The authors acknowledge the support of NGRI, Hyderabad,

    and Kurukshetra University, Kurukshetra, India. The authors

    are grateful to Grzegorz Kwiatek, an anonymous reviewer, and

    the associate editor for their extremely constructive comments,

    which helped us to improve the manuscript significantly.

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    http://dx.doi.org/10.1785/0120110328http://dx.doi.org/10.1029/2005GL022405http://dx.doi.org/10.1029/2005GL022405http://dx.doi.org/10.1029/2004JB003084http://dx.doi.org/10.1029/2004JB003084http://dx.doi.org/10.1111/j.1365-246X.2009.04233.xhttp://dx.doi.org/10.1029/2005JB003834http://dx.doi.org/10.1029/2005JB003834http://dx.doi.org/10.1111/j.1365-246X.2009.04233.xhttp://dx.doi.org/10.1029/2004JB003084http://dx.doi.org/10.1029/2004JB003084http://dx.doi.org/10.1029/2005GL022405http://dx.doi.org/10.1029/2005GL022405http://dx.doi.org/10.1785/0120110328