<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article  PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd"><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article"><front><journal-meta><journal-id journal-id-type="publisher-id">OJER</journal-id><journal-title-group><journal-title>Open Journal of Earthquake Research</journal-title></journal-title-group><issn pub-type="epub">2169-9623</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/ojer.2014.32007</article-id><article-id pub-id-type="publisher-id">OJER-46459</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>EARTH &amp; ENVIRONMENTAL SCIENCES</subject></subj-group></article-categories><title-group><article-title>First Determination of Source Parameters of Moderate Earthquakes (4.1 ≤ M ≤ 5.1) in Morocco from Spectral Analysis</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Ihsane</surname><given-names>Bensaid</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Lahcen</surname><given-names>Bahi</given-names></name><xref ref-type="aff" rid="aff2"><sup>2</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Fida</surname><given-names>Medina</given-names></name><xref ref-type="aff" rid="aff3"><sup>3</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib></contrib-group><aff id="aff2"><addr-line>Université Mohammed V-Agdal, Ecole Mohammedia d’Ingénieurs, Rabat, Morocco</addr-line></aff><aff id="aff3"><addr-line>Université Mohammed V-Agdal, Institut Scientifique, Laboratoire de Géologie et Télédétection (URAC 46), Equipe Télédétection, Risques et Ressources Naturelles, Rabat, Morocco</addr-line></aff><aff id="aff1"><addr-line>Université Mohammed V-Agdal, Institut Scientifique, Laboratoire de Physique du Globe, Equipe Géophysique de Subsurface, Rabat, Morocco;Université Mohammed V-Agdal, Ecole Mohammedia d’Ingénieurs, Rabat, Morocco</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>bensaid@israbat.ac.ma(IB)</email>;<email>bahi@emi.ac.ma(LB)</email>;<email>medina@israbat.ac.ma(FM)</email>;</corresp></author-notes><pub-date pub-type="epub"><day>29</day><month>05</month><year>2014</year></pub-date><volume>03</volume><issue>02</issue><fpage>55</fpage><lpage>65</lpage><history><date date-type="received"><day>18</day>	<month>February</month>	<year>2014</year></date><date date-type="rev-recd"><day>20</day>	<month>March</month>	<year>2014</year>	</date><date date-type="accepted"><day>27</day>	<month>April</month>	<year>2014</year></date></history><permissions><copyright-statement>&#169; Copyright  2014 by authors and Scientific Research Publishing Inc. </copyright-statement><copyright-year>2014</copyright-year><license><license-p>This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/</license-p></license></permissions><abstract><p>
	Recent installation of an array of broad band seismological stations in Morocco allowed us to study the records of five recent (2005-2008) moderate earthquakes (4.1 ≤ M ≤ 5.1) in order to determine their source parameters (seismic moment, fault slip, rupture area and stress drop) from P-wave spectra. We also studied the older Rissani events of 1992 using teleseismic data. Values of <em>Mo</em>, <em>r</em>, <em>Δu</em> and <em>Δσ</em> are, respectively, 1.1 × 10<sup>13</sup> - 6 × 10<sup>16</sup> Nm; 0.50 - 3.9 km; 0.8 - 5.8 cm and 0.3 - 1.49 MPa. The results are in accordance with the seismotectonic and geodynamic setting of Morocco as, for instance, the amount of slip along the faults with respect to the relative displacement of Nubia to Iberia (~4 mm·yr<sup>-1</sup>) determined from GPS data, taking into account the period of stress accumulation. However, some events show very variable corner frequency and low-frequency amplitude values which lead to considerably higher stress drop and fault slip values, especially at the nearest stations, which may reflect some site effects or uncertainties on depth and take-off angles.
</p></abstract><kwd-group><kwd>Morocco</kwd><kwd> Seismicity</kwd><kwd> Fault-Plane Solutions</kwd><kwd> P-Wave Spectra</kwd><kwd> Source Parameters</kwd><kwd> Seismotectonics</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Morocco is located at the westernmost extremity of the complex Ibero-Maghrebian area, where the Azores-Gi- braltar fault zone enters the continental lithosphere of the Betics-Rif-Alboran block. Along this boundary, the present-day convergent plate motion of the Nubian plate with respect to Iberia occurs along a NW-SE trend, as shown by plate kinematic, focal mechanism and GPS studies [<xref ref-type="bibr" rid="scirp.46459-ref1">1</xref>] -[<xref ref-type="bibr" rid="scirp.46459-ref11">11</xref>] . The amount of convergence is about 4 mm∙yr<sup>−1</sup>, most of which is accommodated by earthquakes (<xref ref-type="fig" rid="fig1">Figure 1</xref>). Within this setting, a remarkable discrepancy is the NE-SW escape of the Central Rif block determined by GPS observations [<xref ref-type="bibr" rid="scirp.46459-ref4">4</xref>] [<xref ref-type="bibr" rid="scirp.46459-ref8">8</xref>] [<xref ref-type="bibr" rid="scirp.46459-ref12">12</xref>] -[<xref ref-type="bibr" rid="scirp.46459-ref14">14</xref>] and fault- plane solutions [<xref ref-type="bibr" rid="scirp.46459-ref10">10</xref>] in conformity with geological studies e.g. [<xref ref-type="bibr" rid="scirp.46459-ref14">14</xref>] [<xref ref-type="bibr" rid="scirp.46459-ref15">15</xref>] .</p><p>Earthquakes in Morocco have shallow foci [<xref ref-type="bibr" rid="scirp.46459-ref16">16</xref>] -[<xref ref-type="bibr" rid="scirp.46459-ref22">22</xref>] , but a few events have focal depths of 100 km beneath the Middle Atlas [<xref ref-type="bibr" rid="scirp.46459-ref20">20</xref>] [<xref ref-type="bibr" rid="scirp.46459-ref23">23</xref>] and in northwestern Morocco and adjacent Alboran area [<xref ref-type="bibr" rid="scirp.46459-ref2">2</xref>] [<xref ref-type="bibr" rid="scirp.46459-ref20">20</xref>] .</p><p>Although there is a large dataset on the fault-plane solutions of earthquakes in Morocco (see exhaustive compilation in [<xref ref-type="bibr" rid="scirp.46459-ref24">24</xref>] ), little information exists on the other source parameters. The published studies were conducted only on the largest shocks, in particular on the 1994 and 2004 Al Hoceima, and the 1992 Rissani earthquakes, on the base of waveform analysis [<xref ref-type="bibr" rid="scirp.46459-ref4">4</xref>] [<xref ref-type="bibr" rid="scirp.46459-ref21">21</xref>] [<xref ref-type="bibr" rid="scirp.46459-ref25">25</xref>] , but no studies based on spectral analysis were carried out, with the exception of that published by Bensaid et al. [<xref ref-type="bibr" rid="scirp.46459-ref26">26</xref>] on the Rissani earthquakes.</p><p>Since 2006, numerous broad band stations (BBS) were installed around the western Mediterranean in the context of international cooperation and projects ([<xref ref-type="bibr" rid="scirp.46459-ref27">27</xref>] [<xref ref-type="bibr" rid="scirp.46459-ref28">28</xref>] , <xref ref-type="fig" rid="fig2">Figure 2</xref>); these BBS provided high-quality digital data which allowed us to obtain a certain number of spectra, and therefore, to attempt determining the source parameters which have been done for other Mediterranean seismogenic areas from P-waves e.g. [<xref ref-type="bibr" rid="scirp.46459-ref29">29</xref>] [<xref ref-type="bibr" rid="scirp.46459-ref30">30</xref>] and S- waves e.g. [<xref ref-type="bibr" rid="scirp.46459-ref31">31</xref>] .</p><p>In this paper, we expose the results of the study of the source parameters of 5 moderate shocks that occurred in Morocco during the period 2005-2008 together with two stronger shocks in 1992, corresponding to the Rissani earthquakes. Our leading objective was to attempt to determine the source parameters from these shocks from the P-wave spectra, such as the seismic moment, the fault dimension and displacement, the “stress drop”, and to compare the results to available data on the kinematics and seismicity of the Africa-Iberia plate boundary.</p></sec><sec id="s2"><title>2. Database and Methodology</title><sec id="s2_1"><title>2.1. Data and Processing</title><p>We selected 5 events with magnitude M ≥ 4 that occurred during the period 2005-2008 [<xref ref-type="bibr" rid="scirp.46459-ref10">10</xref>] , and the Rissani events, two older shocks with magnitudes M ~ 5.2 which affected the Anti-Atlas area in 1992 [<xref ref-type="bibr" rid="scirp.46459-ref26">26</xref>] (<xref ref-type="fig" rid="fig2">Figure 2</xref> and <xref ref-type="table" rid="table1">Table 1</xref>).</p><p>As exposed in a previous paper [<xref ref-type="bibr" rid="scirp.46459-ref10">10</xref>] , the hypocentral relocations were determined using the revised version of the HYPO71 computer program [<xref ref-type="bibr" rid="scirp.46459-ref32">32</xref>] , and a standard crustal model for Morocco with Vp/Vs = 1.74 [<xref ref-type="bibr" rid="scirp.46459-ref18">18</xref>] .</p><fig id="fig1"><label>Figure 1</label><caption><p> Seismicity of northern Morocco and adjacent area for the period 1990-2010, magnitudes &gt; 3.5 (after [10] )</p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\2-2740054x\75b40c29-a9ca-4b53-8f39-30d31bb15993.png"/></fig><fig id="fig2"><label>Figure 2</label><caption><p> Location of the earthquakes (stars) and Moroccan and southern Spanish stations (dots) used in the present study. See Table 1 for earthquake parameters</p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\2-2740054x\8833e152-a49d-4e5a-bb9c-59d80bdeb570.png"/></fig><table-wrap id="table1"  position="float"><object-id pub-id-type="pii">Table 1</object-id><label>Table 1</label><caption><p>. List of studied earthquakes.</p></caption><table><thead><tr><th align="center" valign="middle" >Ref</th><th align="center" valign="middle" >Date (dd/mm/yy)</th><th align="center" valign="middle" >Time</th><th align="center" valign="middle" >Latitude</th><th align="center" valign="middle" >Longitude</th><th align="center" valign="middle" >Magnitude</th><th align="center" valign="middle" >Depth in km</th><th align="center" valign="middle" >Location</th></tr></thead><tbody><tr><td align="center" valign="middle" >1</td><td align="center" valign="middle" >23/10/1992</td><td align="center" valign="middle" >09:11:08</td><td align="center" valign="middle" >31.36</td><td align="center" valign="middle" >−4.18</td><td align="center" valign="middle" >5.2</td><td align="center" valign="middle" >2</td><td align="center" valign="middle" >Rissani</td></tr><tr><td align="center" valign="middle" >2</td><td align="center" valign="middle" >30/10/1992</td><td align="center" valign="middle" >10:43:58</td><td align="center" valign="middle" >31.28</td><td align="center" valign="middle" >−4.34</td><td align="center" valign="middle" >5.1</td><td align="center" valign="middle" >2</td><td align="center" valign="middle" >Rissani</td></tr><tr><td align="center" valign="middle" >3</td><td align="center" valign="middle" >22/03/2005</td><td align="center" valign="middle" >09:03:15</td><td align="center" valign="middle" >35.05</td><td align="center" valign="middle" >−2.97</td><td align="center" valign="middle" >4.7</td><td align="center" valign="middle" >5</td><td align="center" valign="middle" >Nador</td></tr><tr><td align="center" valign="middle" >4</td><td align="center" valign="middle" >11/08/2007</td><td align="center" valign="middle" >20:46:01</td><td align="center" valign="middle" >33.14</td><td align="center" valign="middle" >−5.21</td><td align="center" valign="middle" >5.1</td><td align="center" valign="middle" >7</td><td align="center" valign="middle" >Kh&#233;nifra</td></tr><tr><td align="center" valign="middle" >5</td><td align="center" valign="middle" >21/01/2008</td><td align="center" valign="middle" >02:24:03</td><td align="center" valign="middle" >35,12</td><td align="center" valign="middle" >−3.94</td><td align="center" valign="middle" >4.1</td><td align="center" valign="middle" >8</td><td align="center" valign="middle" >Al Hoceima</td></tr><tr><td align="center" valign="middle" >6</td><td align="center" valign="middle" >25/01/2008</td><td align="center" valign="middle" >13:19:40</td><td align="center" valign="middle" >33.01</td><td align="center" valign="middle" >−5.36</td><td align="center" valign="middle" >4.3</td><td align="center" valign="middle" >6</td><td align="center" valign="middle" >Kh&#233;nifra</td></tr><tr><td align="center" valign="middle" >7</td><td align="center" valign="middle" >28/09/2008</td><td align="center" valign="middle" >02:11:21</td><td align="center" valign="middle" >33.59</td><td align="center" valign="middle" >−5.89</td><td align="center" valign="middle" >4.5</td><td align="center" valign="middle" >22</td><td align="center" valign="middle" >Tiflet</td></tr></tbody></table></table-wrap><p>Data in Standard for Exchange of Earthquake Data (SEED) format (FDSN) were retrieved from files of digital stations located in Morocco (Institut Scientifique, ING-CNRST, Siberia and WM networks), Algeria (GEOFON) and Europe (IGN network and German stations) at various epicentral distances between 43 and 2454 km.</p><p>SEED data were read using Rdseed software, and then converted into SAC (Seismic Analysis Code) or ASCII formats. SAC software was used to accomplish all mathematical operations such as Fourier transform, spectral estimation, IIR and FIR filtering, decimation, interpolation correlation, seismic phase picking and graphical output.</p></sec><sec id="s2_2"><title>2.2. Fault-Plane Solutions</title><p>Fault-plane solutions based on P-wave arrivals on the recordings of the selected events were already published in previous papers [<xref ref-type="bibr" rid="scirp.46459-ref10">10</xref>] [<xref ref-type="bibr" rid="scirp.46459-ref26">26</xref>] . Summarizing, first motions of P-waves were read on available paper records and digital files of permanent and temporary stations. Take-off angles for stations at regional distances (less than 1000 km) were obtained for a crustal model formed by two flat layers (15 km each) with constant velocities 6.1 km∙s<sup>−1</sup> and 6.7 km∙s<sup>−1</sup>. The IASPEI model was used for stations at larger distances. Solutions were obtained using the algorithm of Brillinger et al. [<xref ref-type="bibr" rid="scirp.46459-ref33">33</xref>] .</p></sec><sec id="s2_3"><title>2.3. P-Wave Spectra</title><p>The bulk seismograms were cut at the onset of the P- and S-waves. The mean and the linear tendency were removed in order to centre the signal at zero and to stabilize the numerical operations respectively. Since the signal corresponds to velocity, data were integrated to obtain displacements (<xref ref-type="fig" rid="fig3">Figure 3</xref>). Once picked, the seismogram was deconvoluted by the velocity response of the recording instrument. Spectra were obtained from the original digital records using software SAC (<xref ref-type="fig" rid="fig3">Figure 3</xref>). Finally, the low-frequency (plateau) part (Ω<sub>o</sub>) and the corner frequency f<sub>c</sub> were automatically obtained from the signal using software KIV, and subsequently the source parameters.</p><p>As spectra can be affected by attenuation, we used two to six stations at variable epicentral distances in order to obtain a mean value.</p></sec><sec id="s2_4"><title>2.4. Source Parameters</title><p>The source dimensions and scalar seismic moment were determined by spectral analysis using the circular fault model [<xref ref-type="bibr" rid="scirp.46459-ref34">34</xref>] [<xref ref-type="bibr" rid="scirp.46459-ref35">35</xref>] , which is the most suitable for small/moderate earthquakes generated along short faults that generally do not crosscut the Earth’s surface and do not show a well-defined aftershock pattern [<xref ref-type="bibr" rid="scirp.46459-ref36">36</xref>] .</p><p>The radiation pattern (R) for each station was computed from the fault-plane solution, and the scalar seismic moment M<sub>0</sub> was estimated using the amplitude spectra of P-waves [<xref ref-type="bibr" rid="scirp.46459-ref37">37</xref>] .</p><disp-formula id="scirp.46459-formula10"><label>(1)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\2-2740054x\3e1351c8-78e1-45e8-af6f-934e75c32e9f.png"/></disp-formula><fig-group id="fig3"><caption><title>Figure 3</title><p> P-wave amplitude spectrum at station AVE for the event of 11 January 2008. (a) chosen window in the velocity record; (b) obtained displacement record after removing the instrument effect and integration; (c) amplitude spectrum showing plateau Ω<sub>o</sub> and corner frequency f<sub>c</sub></p></caption><fig id ="fig3_1"><label>(a)</label><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\2-2740054x\16d5aa8a-7d72-40c1-a65c-5402a1006f0d.png"/></fig><fig id ="fig3_2"><label>(b)</label><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\2-2740054x\54e471c0-e8c2-4dd4-b669-0a06fa623586.png"/></fig><fig id ="fig3_3"><label>(c)</label><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\2-2740054x\69c3e778-d498-4d72-91e3-27d375ca05bc.png"/></fig></fig-group><p>where ρ is the density, a is the fault radius, r is the distance from the focus to the receiving station, g(∆) is the geometric attenuation, C(i<sub>o</sub>) is the effect of free surface on amplitude, Ω<sub>o</sub> is the spectral amplitude at low frequency of P-wave displacement, ω is the angular frequency, Q is the quality factor of P-wave (taken here as 300) and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\2-2740054x\94779641-820c-473c-b7a1-23d28f638cdc.png" xlink:type="simple"/></inline-formula> is the radiation factor corresponding to the source orientation given by<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\2-2740054x\217f3957-a626-4114-a00c-50072f3bbc39.png" xlink:type="simple"/></inline-formula>, i<sub>h</sub> where <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\2-2740054x\ff47e2f8-0cbd-4bdf-806f-2881f88baa3f.png" xlink:type="simple"/></inline-formula> is the azimut of the station with respect to the fault, <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\2-2740054x\4ed5b77f-090d-4e60-b124-de19ce225f46.png" xlink:type="simple"/></inline-formula>is the dip of the fault-plane, <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\2-2740054x\c5f6dcca-34df-4581-9897-6b4876a8954c.png" xlink:type="simple"/></inline-formula>is the rake and i<sub>h</sub> is the take-off angle.</p><p>The dimension of the rupture (a) was evaluated from the corner frequency (f<sub>c</sub>) [<xref ref-type="bibr" rid="scirp.46459-ref37">37</xref>] :</p><disp-formula id="scirp.46459-formula11"><label>(2)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\2-2740054x\470c5942-0dbf-432b-a89b-4eebe2d8e4fd.png"/></disp-formula><p>where α is the P-wave velocity.</p><p>The average displacement and stress drop were estimated from the scalar moment (M<sub>0</sub>) and dimensions [<xref ref-type="bibr" rid="scirp.46459-ref38">38</xref>] :</p><disp-formula id="scirp.46459-formula12"><label>(3)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\2-2740054x\bae451ac-8de4-41c4-b16f-75b33da1e6e5.png"/></disp-formula><p>The stress drop <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\2-2740054x\c41765fe-95f9-4d31-b302-02022a0afc0c.png" xlink:type="simple"/></inline-formula> was determined using the equation [<xref ref-type="bibr" rid="scirp.46459-ref34">34</xref>] -[<xref ref-type="bibr" rid="scirp.46459-ref37">37</xref>] [<xref ref-type="bibr" rid="scirp.46459-ref39">39</xref>] :</p><disp-formula id="scirp.46459-formula13"><label>(4)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\2-2740054x\5f3f5df3-0bd9-4303-981a-dcbb3ad03ae7.png"/></disp-formula><p>Computations were performed at the Complutense University (Madrid) using softwares KIV and SAC (IRIS [<xref ref-type="bibr" rid="scirp.46459-ref40">40</xref>] ) to obtain the spectra of the P-wave, and MOS2 for determining M<sub>0</sub> and source dimensions. The epicentral distance, azimut, and take-off angle were determined with the help of subroutine CASSOL. The radiation pattern R was obtained with MECSTA. The choice of the software was based on its availability at Madrid University and because it is the same than that used by Spanish researchers who have installed the WM network in Morocco.</p></sec></sec><sec id="s3"><title>3. Results</title><sec id="s3_1"><title>3.1. Focal Mechanisms</title><p>The fault-plane solutions and numerical parameters of the studied earthquakes [<xref ref-type="bibr" rid="scirp.46459-ref10">10</xref>] are respectively shown in <xref ref-type="fig" rid="fig4">Figure 4</xref> and <xref ref-type="fig" rid="fig5">Figure 5</xref> and listed in <xref ref-type="table" rid="table2">Table 2</xref> respectively. In the central and eastern Rif (solutions 3 and 5), the solutions correspond to either almost-pure normal faulting or to strike-slip faulting with a normal component. The T-axes have an E-W trend. The solutions determined in the Middle Atlas chain and in the Meseta (solutions 4, 6 and 7) show almost-pure reverse faulting in two cases and strike-slip faulting with a normal component in another. In the three cases, the P-axis is oriented NW-SE. Finally, the solutions south of the High Atlas correspond to strike-slip faulting with a NW-SE oriented P-axis.</p><fig id="fig4"><label>Figure 4</label><caption><p> Location of the fault-plane solutions of the studied earthquakes, after [10] </p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\2-2740054x\0d2e30ba-6a67-43e1-8e79-8d014f6530ab.png"/></fig><fig id="fig5"><label>Figure 5</label><caption><p> Detailed fault-plane solutions of the studied earthquakes (see Table 2 for the numerical parameters). Full circles = compression; empty circles = dilatation; squares = direct arrivals; P = pressure axis; T = tension axis; dashed traces in solutions 1 and 2 = solutions given by Harvard</p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\2-2740054x\5b6f01a6-5f43-4efe-a254-615a9ef26740.png"/></fig><table-wrap id="table2"  position="float"><object-id pub-id-type="pii">Table 2</object-id><label>Table 2</label><caption><p>. Fault-plane solutions of the studied earthquakes, after [10] .</p></caption><table><thead><tr><th align="center" valign="middle" >Ref</th><th align="center" valign="middle" >Date (D/M/Y)</th><th align="center" valign="middle" >Lat. N Lon. W</th><th align="center" valign="middle" >M</th><th align="center" valign="middle" >Depth (km)</th><th align="center" valign="middle" >Fault planes (˚) (Φ, δ, λ)</th><th align="center" valign="middle" >P axis (˚) (Tr; pl)</th><th align="center" valign="middle" >T axis (˚) (Tr; pl)</th><th align="center" valign="middle" >N</th><th align="center" valign="middle" >Score (%)</th></tr></thead><tbody><tr><td align="center" valign="middle" >1</td><td align="center" valign="middle" >23/10/1992</td><td align="center" valign="middle" >31.36˚; 4.18˚</td><td align="center" valign="middle" >5.2</td><td align="center" valign="middle" >2 &#177; 5.2</td><td align="center" valign="middle" >A: 359 &#177; 9; 71 &#177; 9; 1 &#177; 11 B: 89 &#177; 11; 89 &#177; 10; −161 &#177; 9</td><td align="center" valign="middle" >316 &#177; 10;  14 &#177; 10</td><td align="center" valign="middle" >223 &#177; 09; 13 &#177; 09</td><td align="center" valign="middle" >30</td><td align="center" valign="middle" >97</td></tr><tr><td align="center" valign="middle" >2</td><td align="center" valign="middle" >30/10/1992</td><td align="center" valign="middle" >31.28˚; 4.34˚</td><td align="center" valign="middle" >5.1</td><td align="center" valign="middle" >2 &#177; 6.0</td><td align="center" valign="middle" >A: 9 &#177; 11; 73 &#177; 14; 7 &#177; 11 B: 277 &#177; 12; 83 &#177; 10; 163 &#177; 14</td><td align="center" valign="middle" >324 &#177; 12; 7 &#177; 12</td><td align="center" valign="middle" >232 &#177; 11; 16 &#177; 12</td><td align="center" valign="middle" >13</td><td align="center" valign="middle" >100</td></tr><tr><td align="center" valign="middle" >3</td><td align="center" valign="middle" >22/03/05</td><td align="center" valign="middle" >35.05˚; 2.97˚</td><td align="center" valign="middle" >4.7</td><td align="center" valign="middle" >5 &#177; 4</td><td align="center" valign="middle" >A: 33 &#177; 59; 40 &#177; 38; −44 &#177; 53 B: 160 &#177; 35; 63 &#177; 20; −121 &#177; 52</td><td align="center" valign="middle" >25 &#177; 43;  59 &#177; 45</td><td align="center" valign="middle" >272 &#177; 37;  13 &#177; 19</td><td align="center" valign="middle" >29</td><td align="center" valign="middle" >97</td></tr><tr><td align="center" valign="middle" >4</td><td align="center" valign="middle" >11/08/07</td><td align="center" valign="middle" >33.14˚; 5.21˚</td><td align="center" valign="middle" >5.1</td><td align="center" valign="middle" >7 &#177; 3.7</td><td align="center" valign="middle" >A: 14 &#177; 13; 59 &#177; 20; −7 &#177; 35 B: 108 &#177; 24; 84 &#177; 29; −149 &#177; 21</td><td align="center" valign="middle" >336 &#177; 14;  26 &#177; 19</td><td align="center" valign="middle" >237 &#177; 24;  17 &#177; 31</td><td align="center" valign="middle" >23</td><td align="center" valign="middle" >91</td></tr><tr><td align="center" valign="middle" >5</td><td align="center" valign="middle" >21/01/08</td><td align="center" valign="middle" >35.12˚; 3.94˚</td><td align="center" valign="middle" >4.1</td><td align="center" valign="middle" >8.2 &#177; 3.0</td><td align="center" valign="middle" >A: 200 &#177; 9; 70 &#177; 12; −9 &#177; 20 B: 293 &#177; 12; 82 &#177; 19; −159 &#177; 12</td><td align="center" valign="middle" >158 &#177; 9;  20 &#177; 16</td><td align="center" valign="middle" >65 &#177; 11;  8 &#177; 15</td><td align="center" valign="middle" >19</td><td align="center" valign="middle" >95</td></tr><tr><td align="center" valign="middle" >6</td><td align="center" valign="middle" >25/01/08</td><td align="center" valign="middle" >33.01˚; 5.36˚</td><td align="center" valign="middle" >4.3</td><td align="center" valign="middle" >5.6 &#177; 3.5</td><td align="center" valign="middle" >A: 80 &#177; 6; 40 &#177; 4; 69 &#177; 13 B: 233 &#177; 24; 53 &#177; 4; 107 &#177; 16</td><td align="center" valign="middle" >335 &#177; 7;  7 &#177; 3</td><td align="center" valign="middle" >90 &#177; 30;  75 &#177; 10</td><td align="center" valign="middle" >12</td><td align="center" valign="middle" >100</td></tr><tr><td align="center" valign="middle" >7</td><td align="center" valign="middle" >28/09/08</td><td align="center" valign="middle" >33.59˚; 5.89˚</td><td align="center" valign="middle" >4.5</td><td align="center" valign="middle" >21.8 &#177; 2.7</td><td align="center" valign="middle" >A: 80 &#177; 7; 21 &#177; 2; 66 &#177; 8 B: 234 &#177; 4; 71 &#177; 2; 99 &#177; 3</td><td align="center" valign="middle" >331 &#177; 4;  25 &#177; 2</td><td align="center" valign="middle" >130 &#177; 7;  63 &#177; 2</td><td align="center" valign="middle" >13</td><td align="center" valign="middle" >85</td></tr></tbody></table></table-wrap></sec><sec id="s3_2"><title>3.2. Source Parameters from P-Wave Spectra</title><p>The characteristics of 29 spectra of the studied earthquakes such, as the low-frequency spectral amplitudes and the corner frequencies observed are indicated in <xref ref-type="table" rid="table3">Table 3</xref>. Selected examples for each event are shown in <xref ref-type="fig" rid="fig6">Figure 6</xref>. The source parameters (seismic moment, fault radius, moment magnitude, fault displacement and stress drop) calculated from these data are given in <xref ref-type="table" rid="table4">Table 4</xref>. For the largest events (#1 and 2), which correspond to the Rissani twin earthquakes of 23 and 30 October 1992, the fault radii are close to 4 km, the displacements are about 4 cm and the stress drops are 0.3 - 0.4 MPa.</p><p>The three smallest events show very similar parameters with fault radii close to 0.6 km, fault displacements of 1.26 to 2.41 cm and stress drops of 0.96 to 2.45 MPa. However, the parameters of the 22 March 2005 event ap-</p><table-wrap id="table3"  position="float"><object-id pub-id-type="pii">Table 3</object-id><label>Table 3</label><caption><p>. Spectral characteristics obtained from the stations for each studied earthquakes. R: radiation pattern; Ω<sub>o</sub>: flat low- frequency amplitude; fc: corner frequency.</p></caption><table><thead><tr><th align="center" valign="middle" ></th><th align="center" valign="middle" >Ref</th><th align="center" valign="middle" >Event (dd/mm/yy)</th><th align="center" valign="middle" >Number of spectra</th><th align="center" valign="middle" >Stations</th><th align="center" valign="middle" >Epicentral distance (km)</th><th align="center" valign="middle" >Take-off angle</th><th align="center" valign="middle" >R (θ, φ)</th><th align="center" valign="middle" >Ω<sub>o</sub> (m)</th><th align="center" valign="middle"  colspan="2"  >fc (Hz)</th></tr></thead><tbody><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" >1</td><td align="center" valign="middle" >23/10/92</td><td align="center" valign="middle" >4</td><td align="center" valign="middle" >FUR AQU WET TAM</td><td align="center" valign="middle" >2439 1980 2439 1350</td><td align="center" valign="middle" >32 39 30 42</td><td align="center" valign="middle" >0.595 0.811 0.624 0.638</td><td align="center" valign="middle" >5 &#215; 10<sup>−6</sup> 1 &#215; 10<sup>−5</sup> 1 &#215; 10<sup>−6</sup> 2 &#215; 10<sup>−6</sup></td><td align="center" valign="middle"  colspan="2"  >0.5 0.8 0.6 0.5</td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" >2</td><td align="center" valign="middle" >30/10/92</td><td align="center" valign="middle" >4</td><td align="center" valign="middle" >FUR AQU WET TAM</td><td align="center" valign="middle" >2294 1980 2454 1357</td><td align="center" valign="middle" >32 33 30 43</td><td align="center" valign="middle" >0.025 0.812 0.040 0.610</td><td align="center" valign="middle" >5 &#215; 10<sup>−6</sup> 1 &#215; 10<sup>−5</sup> 3 &#215; 10<sup>−6</sup> 3 &#215; 10<sup>−6</sup></td><td align="center" valign="middle"  colspan="2"  >0.5 0.6 0.5 0.5</td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" >3</td><td align="center" valign="middle" >22/03/05</td><td align="center" valign="middle" >2</td><td align="center" valign="middle" >EALB ECOG</td><td align="center" valign="middle" >100 254</td><td align="center" valign="middle" >62 41</td><td align="center" valign="middle" >−0.6035 −0.7285</td><td align="center" valign="middle" >1 &#215; 10<sup>−6</sup> 1 &#215; 10<sup>−7</sup></td><td align="center" valign="middle"  colspan="2"  >4 5</td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" >4</td><td align="center" valign="middle" >11/08/07</td><td align="center" valign="middle" >5</td><td align="center" valign="middle" >IFR AVE EALB ECEU EMIJ</td><td align="center" valign="middle" >43 206 370 380 383</td><td align="center" valign="middle" >85 42 42 42 42</td><td align="center" valign="middle" >−0.3500 0.3700 −0.4100 −0.7500 −0.6900</td><td align="center" valign="middle" >1 &#215; 10<sup>−5</sup> 1 &#215; 10<sup>−5</sup> 1 &#215; 10<sup>−7</sup> 1 &#215; 10<sup>−7</sup> 2 &#215; 10<sup>−7</sup></td><td align="center" valign="middle"  colspan="2"  >3 2 3 3 3</td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" >5</td><td align="center" valign="middle" >21/01/08</td><td align="center" valign="middle" >6</td><td align="center" valign="middle" >M006 M008 M014 M012 M018 IFR</td><td align="center" valign="middle" >79 114 134 145 175 211</td><td align="center" valign="middle" >71 61 56 43 43 43</td><td align="center" valign="middle" >0.7619 −0.1388 −0.8301 0.2695 −0.4706 −0.2073</td><td align="center" valign="middle" >1 &#215; 10<sup>−7</sup> 1 &#215; 10<sup>−7</sup> 1 &#215; 10<sup>−7</sup> 1 &#215; 10<sup>−7</sup> 1 &#215; 10<sup>−7</sup> 2 &#215; 10<sup>−7</sup></td><td align="center" valign="middle"  colspan="2"  >6 4 6 3 5 3</td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" >6</td><td align="center" valign="middle" >25/01/08</td><td align="center" valign="middle" >4</td><td align="center" valign="middle" >M011 M017 M018 IFR</td><td align="center" valign="middle" >61 98 109 111</td><td align="center" valign="middle" >75 63 60 59</td><td align="center" valign="middle" >−0.37019 −0.75248 0.35968 −0.51466</td><td align="center" valign="middle" >1 &#215; 10<sup>−7</sup> 1 &#215; 10<sup>−7</sup> 1 &#215; 10<sup>−7</sup> 1 &#215; 10<sup>−7</sup></td><td align="center" valign="middle"  colspan="2"  >5 4 5 4</td></tr><tr><td align="center" valign="middle"  colspan="2"  >7</td><td align="center" valign="middle" >28/09/08</td><td align="center" valign="middle" >5</td><td align="center" valign="middle" >M010 M018 M006 M019</td><td align="center" valign="middle" >81 133 184 225</td><td align="center" valign="middle" >81 51 51 51</td><td align="center" valign="middle" >−0.8458 0.6701 −0.0758 0.6397</td><td align="center" valign="middle" >3 &#215; 10<sup>−7</sup> 1 &#215; 10<sup>−7</sup> 1 &#215; 10<sup>−8</sup> 3 &#215; 10<sup>−8</sup></td><td align="center" valign="middle" >6 6 3 4</td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr></tbody></table></table-wrap><p>pear to be too high with respect to the other events, certainly because of the small number of available spectra. We also had to remove station M010 from the calculations of the 28 September 2008 source parameters, because it led to too high values.</p><p>In contrast, the M ~ 5 event that occurred in the Middle Atlas on 11 August 2007 shows very variable values of fault displacement (0.8 cm at ECEU to 87 cm at IFR) and stress drops (0.52 MPa at ECEU to 63 MPa at IFR), although the fault radii values are homogeneous (0.83 to 0.99 km). Therefore, we recalculated the source parameters shown in <xref ref-type="table" rid="table4">Table 4</xref> without taking into account stations IFR and AVE, which provided too large values.</p></sec></sec><sec id="s4"><title>4. Discussion</title><sec id="s4_1"><title>4.1. Influence of the Quality of Data and Processing on the Obtained Results</title><p>Our study was initially intended to attempt determining the source parameters of the Moroccan moderate events for seismotectonic analysis. However, the results show that the variability of the parameters that lead to them may have a large influence on the obtained values.</p><p>First, it appears that the corner frequency values obtained from the spectra are not always homogeneous for the same event, especially at the nearest stations which display large discrepancies, as for instance in the case of stations IFR and AVE for the event recorded on 11 August 2008. This may be due to several parameters such as:</p><p>1) Site effects related to the geological composition of the basement, which may also have an influence on the stress drop.</p><p>2) Uncertainty on the hypocentral depth (<xref ref-type="table" rid="table2">Table 2</xref>), which may dramatically influence the estimation of the radiation pattern and subsequent calculations. Such discrepancies may currently be observed even within closely spaced stations, but within 30% of the mean value [<xref ref-type="bibr" rid="scirp.46459-ref41">41</xref>] .</p><fig id="fig6"><label>Figure 6</label><caption><p> Selected examples of P-wave spectra for the studied earthquakes</p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\2-2740054x\fbb00d9c-f606-4535-a0bf-c04e702ee10b.png"/></fig><table-wrap id="table4"  position="float"><object-id pub-id-type="pii">Table 4</object-id><label>Table 4</label><caption><p>. Spectral characteristics obtained from the stations for each studied earthquakes. R: radiation pattern; Ω<sub>o</sub>: plateau amplitude; fc: corner frequency.</p></caption><table><thead><tr><th align="center" valign="middle" >Ref</th><th align="center" valign="middle" >Event</th><th align="center" valign="middle" >Mean M<sub>0 </sub>(Nm)</th><th align="center" valign="middle" >Mean r (km)</th><th align="center" valign="middle" >Mw</th><th align="center" valign="middle" >N</th><th align="center" valign="middle" >Δu (cm)</th><th align="center" valign="middle" >(MPa)</th></tr></thead><tbody><tr><td align="center" valign="middle" >1</td><td align="center" valign="middle" >23/10/92</td><td align="center" valign="middle" >6.03 &#177; 3.03 &#215; 10<sup>16</sup></td><td align="center" valign="middle" >3.90 &#177; 0.70</td><td align="center" valign="middle" >5.1</td><td align="center" valign="middle" >4</td><td align="center" valign="middle" >4.00 &#177; 2.10</td><td align="center" valign="middle" >0.4 &#177; 0.20</td></tr><tr><td align="center" valign="middle" >2</td><td align="center" valign="middle" >30/10/92</td><td align="center" valign="middle" >5.07 &#177; 2.28 &#215; 10<sup>16</sup></td><td align="center" valign="middle" >3.70 &#177; 0.60</td><td align="center" valign="middle" >5.0</td><td align="center" valign="middle" >4</td><td align="center" valign="middle" >3.70 &#177; 1.85</td><td align="center" valign="middle" >0.3 &#177; 0.16</td></tr><tr><td align="center" valign="middle" >3</td><td align="center" valign="middle" >22/03/05</td><td align="center" valign="middle" >1.1 &#177; 0.6 &#215; 10<sup>15</sup></td><td align="center" valign="middle" >0.50 &#177; 0.00</td><td align="center" valign="middle" >4.00</td><td align="center" valign="middle" >2</td><td align="center" valign="middle" >4.31 &#177; 2.38</td><td align="center" valign="middle" >3.8 &#177; 0.00</td></tr><tr><td align="center" valign="middle" >4</td><td align="center" valign="middle" >11/08/07</td><td align="center" valign="middle" >5.8 &#177; 4.6 &#215; 10<sup>15</sup></td><td align="center" valign="middle" >0.88 &#177; 0.07</td><td align="center" valign="middle" >5.00</td><td align="center" valign="middle" >3</td><td align="center" valign="middle" >5.80 &#177; 4.80</td><td align="center" valign="middle" >1.30 &#177; 0.57</td></tr><tr><td align="center" valign="middle" >5</td><td align="center" valign="middle" >21/01/08</td><td align="center" valign="middle" >9.1 &#177; 0.88 &#215; 10<sup>14</sup></td><td align="center" valign="middle" >0.60 &#177; 0.26</td><td align="center" valign="middle" >3.90</td><td align="center" valign="middle" >6</td><td align="center" valign="middle" >2.04 &#177; 1.13</td><td align="center" valign="middle" >1.49 &#177; 0.62</td></tr><tr><td align="center" valign="middle" >6</td><td align="center" valign="middle" >25/01/08</td><td align="center" valign="middle" >4.3 &#177; 0.22 &#215; 10<sup>14</sup></td><td align="center" valign="middle" >0.59 &#177; 0.05</td><td align="center" valign="middle" >3.70</td><td align="center" valign="middle" >4</td><td align="center" valign="middle" >1.26 &#177; 0.63</td><td align="center" valign="middle" >0.96 &#177; 0.51</td></tr><tr><td align="center" valign="middle" >7</td><td align="center" valign="middle" >28/09/08</td><td align="center" valign="middle" >2.6 &#177; 0.73 &#215; 10<sup>14</sup></td><td align="center" valign="middle" >0.62 &#177; 0.16</td><td align="center" valign="middle" >3.74</td><td align="center" valign="middle" >3</td><td align="center" valign="middle" >0.80 &#177; 0.44</td><td align="center" valign="middle" >0.70 &#177; 0.50</td></tr></tbody></table></table-wrap><p>3) The use of the circular fault model of Brune [<xref ref-type="bibr" rid="scirp.46459-ref34">34</xref>] [<xref ref-type="bibr" rid="scirp.46459-ref35">35</xref>] , because we consider that a rectangular fault surface would be more realistic tectonically, but it was impossible to use it because of several parameters such as the small size of the earthquakes, the large depth of some of them and therefore the absence of an aftershock series which could have provided more information on the fault surface.</p><p>Therefore, we consider that a more systematic study, using a larger number of stations by event is needed in order to constraint the role of each parameter in the determination of the spectrum.</p></sec><sec id="s4_2"><title>4.2. Seismotectonic Implications and Risk Assessment</title><p>As exposed in the first section, the amount of convergence of Nubia to Iberia is about 4 mm∙yr<sup>−1</sup> in Morocco according to the recent GPS studies [<xref ref-type="bibr" rid="scirp.46459-ref4">4</xref>] [<xref ref-type="bibr" rid="scirp.46459-ref5">5</xref>] [<xref ref-type="bibr" rid="scirp.46459-ref8">8</xref>] [<xref ref-type="bibr" rid="scirp.46459-ref11">11</xref>] -[<xref ref-type="bibr" rid="scirp.46459-ref13">13</xref>] . The Rif and High Atlas chains accomodate ~1 mm∙yr<sup>−1</sup> by earthquakes of low to moderate magnitude (maximum Mw = 6.3 at Al Hoceima in 2004), while the Alboran area, the Mesetas and the Anti Atlas accommodate the remaining.</p><p>Our results show that the moderate earthquakes are associated to fault slip values of 1 - 4 cm, which may represent 10 to 40 years of stress accumulation at a strain rate of 1 mm∙yr<sup>−1</sup> or less at a higher strain rate. This may be a suitable explanation for the diffuse distribution of the Moroccan earthquakes, especially in the Atlas chains, where the shocks occur randomly which indicates that stress may be released at different segments.</p><p>Another point is that our results can be used for seismic hazard assessment in Morocco, obviously together with other methods such as Coulomb stress; for instance, it appears that for moderate earthquakes (M = 4 - 5), stress is released on faults by slip of about 4 mm to 4 cm. Recent GPS monitoring studies show that in several areas in Morocco, the relative motion of fault blocks can be more or less precisely evaluated. This is the case of the SW-displacement of the Rif units onto their foreland, with velocities of 1 - 4 mm∙yr<sup>−1</sup>. If the date of the last significant earthquake in a given area can be known, the magnitude of the next one can be predicted on the base of the time interval. For instance, we can predict that an earthquake of magnitude M = 4 can occur each year in an area showing relative (convergence) velocities of 4 mm∙yr<sup>−1</sup>, or each two years if it is 2 mm∙yr<sup>−1</sup>, and that larger ones with M = 5 each 10 years in a 4 mm∙yr<sup>−1</sup> displacement area, as for instance near the city of F&#232;s [<xref ref-type="bibr" rid="scirp.46459-ref14">14</xref>] .</p></sec></sec><sec id="s5"><title>5. Conclusion</title><p>In this paper, we exposed the first results of the use of P-wave spectra obtained from broad band station recordings in Morocco for determining the source parameters of some moderate earthquakes that occurred in the country. The main conclusion is that the spectra can be useful for determining the source parameters, and provide results which are in accordance with the seismotectonic and geodynamic setting of Morocco. For instance, the amount of slip along the faults with respect to the relative displacement of Nubia to Iberia and that of Morocco to Nubia can be evaluated for earthquakes whose faults do not reach the surface. However, some events show very variable corner frequencies and low frequency amplitudes which lead to considerably higher values of source parameters such as stress drop and fault slip, especially at the nearest stations, which may reflect some site effects or uncertainties on depth and take-off angles. Therefore, it appears necessary to increase the number of studied spectra in order to improve the values of the source parameters.</p></sec><sec id="s6"><title>Acknowledgements</title><p>This study has been partially supported by the Universidad Complutense de Madrid, project AE1/09-16586 to I. Bensaid. We are deeply grateful to Professor Elisa Buforn (Universidad Complutense, Madrid) for having provided the calculation programs and receiving I.B. for numerous training stays. 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