<?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">IJG</journal-id><journal-title-group><journal-title>International Journal of Geosciences</journal-title></journal-title-group><issn pub-type="epub">2156-8359</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/ijg.2017.87050</article-id><article-id pub-id-type="publisher-id">IJG-77685</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>
 
 
  Subsurface Structural Mapping Using Combined Terrestrial and Grace Gravity Data of the Adamawa Plateau (North-Cameroon)
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Bouba</surname><given-names>Apollinaire</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>Kamguia</surname><given-names>Joseph</given-names></name><xref ref-type="aff" rid="aff2"><sup>2</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Tabod</surname><given-names>Charles Tabod</given-names></name><xref ref-type="aff" rid="aff2"><sup>2</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Yap</surname><given-names>Loudi</given-names></name><xref ref-type="aff" rid="aff2"><sup>2</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Nouayou</surname><given-names>Robert</given-names></name><xref ref-type="aff" rid="aff2"><sup>2</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Kande</surname><given-names>Houetchak Ludovic</given-names></name><xref ref-type="aff" rid="aff3"><sup>3</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Oyoa</surname><given-names>Valentin</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib></contrib-group><aff id="aff1"><addr-line>Department of Physics, Higher Teachers’ Training College, University of Maroua, Maroua, Cameroon</addr-line></aff><aff id="aff3"><addr-line>National Institute of Cartography, Yaounde, Cameroon</addr-line></aff><aff id="aff2"><addr-line>Department of Physics, Faculty of Science, University of Yaounde I, Yaounde, Cameroon</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>boubaapollinaire@yahoo.fr(BA)</email>;</corresp></author-notes><pub-date pub-type="epub"><day>14</day><month>07</month><year>2017</year></pub-date><volume>08</volume><issue>07</issue><fpage>869</fpage><lpage>887</lpage><history><date date-type="received"><day>May</day>	<month>27,</month>	<year>2017</year></date><date date-type="rev-recd"><day>Accepted:</day>	<month>July</month>	<year>14,</year>	</date><date date-type="accepted"><day>July</day>	<month>17,</month>	<year>2017</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>
 
 
  In order to analyze and determine the geological structures of the Adamawa plateau, the terrestrial gravity data were combined to data computed from GGM02C gravity model. The dense gravity net obtained were further introduced into qualitative and quantitative interpretations. The resulting Bouguer anomaly map obtained from combined data shows NE-SW direction which nearly coincides with the main direction of the fractures affecting the basement in the region and indicates strong gradients marking the presence of discontinuities between heavy and negative gravity anomaly. In order to conduct the quantitative interpretation of the combined gravity data, three profiles were drawn on the residual Bouguer anomaly map and therefore were interpreted using spectral analysis method and 3D density inversion. The knowledge of the depth and density of the geological structures show an uplift of dense rocks under the granite-gneiss substratum. This dense material found in the ENE-WSW direction of the Adamawa Plateau is interpreted as basaltic intrusion probably resulting from tectonic processes. According to this study, the depths of 3.83 km and 9.62 km are the new values of depths obtained for futures investigations in the Adamawa plateau.
 
</p></abstract><kwd-group><kwd>GGM02C</kwd><kwd> Adamawa Plateau</kwd><kwd> Bouguer Anomaly</kwd><kwd> 3D Density Model</kwd><kwd> Spectral Analysis</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>The study area lies over the Adamawa Plateau (northern Cameroon) between latitudes 5˚ and 8˚N, and longitudes 13˚ to 15˚E. Previous geophysical and geological studies have been conducted in this area. These include the works of [<xref ref-type="bibr" rid="scirp.77685-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.77685-ref2">2</xref>] [<xref ref-type="bibr" rid="scirp.77685-ref3">3</xref>] [<xref ref-type="bibr" rid="scirp.77685-ref4">4</xref>] [<xref ref-type="bibr" rid="scirp.77685-ref5">5</xref>] . Some of the above mentioned studies are based on the geophysical signatures of geological units deduced from gravity analyses and their quantitative interpretation. However, a closer look to the terrestrial gravity net of the study area shows that there are many gaps. This might lead to many approximations in geophysical gravity anomaly analyses and interpretations in the region. Hence, the analyses and interpretations should be based on maps showing the real signatures of the geological features. To achieve this goal, a dense gravity net is needed. New gravity campaigns are indicated to fill the gaps. A global geopotential model can also be a solution. Merry [<xref ref-type="bibr" rid="scirp.77685-ref6">6</xref>] showed that GRACE models are more representative of geoid undulations and gravity anomalies in Africa. From statistical studies, [<xref ref-type="bibr" rid="scirp.77685-ref7">7</xref>] [<xref ref-type="bibr" rid="scirp.77685-ref8">8</xref>] showed that gravity data from GGM02C and terrestrial ones have the same precision. In this work, GGM02C gravity data combined to terrestrial ones will be exploited to reinforce the precision of the previous works.</p><p>The main objective in this work is to interpret a new Bouguer anomaly map obtained from combined terrestrial and GRACE gravity model GGM02C, then determine the depth and density of the geological structure associated with the crustal formation from a dense gravity net in the study area. On residual Bouguer anomaly map, spectral analysis technic and 3D density inversion were obtained. This method has already been successfully used by [<xref ref-type="bibr" rid="scirp.77685-ref9">9</xref>] [<xref ref-type="bibr" rid="scirp.77685-ref10">10</xref>] to determine the major subsurface structure in the northern edge of the Congo-Craton. With these approaches, we complete the previous geophysical works which used only the terrestrial gravity data.</p></sec><sec id="s2"><title>2. Geological Setting</title><p>Previous geological and geophysical studies conducted in the Adamawa plateau (<xref ref-type="fig" rid="fig1">Figure 1</xref>) indicated that this area is predominantly composed by Precambrian rocks such as migmatic, gneisses and granites that were granitized during the Pan-African tectonic event [<xref ref-type="bibr" rid="scirp.77685-ref12">12</xref>] [<xref ref-type="bibr" rid="scirp.77685-ref13">13</xref>] . It is covered by a sequence of tertiary basaltic lavas [<xref ref-type="bibr" rid="scirp.77685-ref14">14</xref>] (<xref ref-type="fig" rid="fig2">Figure 2</xref>). These lavas are alkaline, indicating affinity with continental rifts [<xref ref-type="bibr" rid="scirp.77685-ref15">15</xref>] . Sedimentary formations consist mainly of conglomerates, arkosic sandstone and limestone from the Cretaceous Djerem basin and Mbere ditch [<xref ref-type="bibr" rid="scirp.77685-ref14">14</xref>] . These formations have undergone intense volcanic activity leading to the establishment of the basin structure, covered by volcanic materials which reach the surface through deep fractures. These fractures have a location at the base of major crustal lineaments [<xref ref-type="bibr" rid="scirp.77685-ref16">16</xref>] . Three major tectonic structures are associated with the Adamawa Plateau: the Cameroon Volcanic Line (CVL), the Foumban Shear Zone (FSZ) and the South Adamawa Trough (SAT). The CVL is a chain of intra-plate volcano shaped Y which extends from the island of Pagalu in the Atlantic Ocean west of Africa until about 2000 km [<xref ref-type="bibr" rid="scirp.77685-ref17">17</xref>] . The first branch (north) corresponds to the Benue through and the second branch (east) the Adamawa plateau. Volcanic rocks on this line are composed of alkali basalt, trachyte</p><fig id="fig1"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref></label><caption><title> Location map of the Adamawa region-Cameroon modified after [<xref ref-type="bibr" rid="scirp.77685-ref11">11</xref>] </title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/2-2801462x2.png"/></fig><p>lavas and tuffs. The Foumban Shear Zone is a succession of major accident covered by a series of tertiary volcanoes that one follows from Sudan, through the Central African Republic and Chad up to Foumban in Cameroon [<xref ref-type="bibr" rid="scirp.77685-ref18">18</xref>] . To the west, it is an extension of the pernambuco fault in the north-east of Brazil [<xref ref-type="bibr" rid="scirp.77685-ref19">19</xref>] . The FSZ in Cameroon center displays a dextral sense of displacement [<xref ref-type="bibr" rid="scirp.77685-ref13">13</xref>] [<xref ref-type="bibr" rid="scirp.77685-ref18">18</xref>] . The South Adamawa Trough includes the Cretaceous Mbere ditch and Djerem basin. It is a deep scarps bounded by two faults up to 600 m high command [<xref ref-type="bibr" rid="scirp.77685-ref14">14</xref>] . This gap is due to the movement of the south Atlantic to the Upper Cretaceous [<xref ref-type="bibr" rid="scirp.77685-ref16">16</xref>] [<xref ref-type="bibr" rid="scirp.77685-ref20">20</xref>] .</p></sec><sec id="s3"><title>3. Gravity Data and Methods</title><p>In this study terrestrial gravity data and data from the global geopotential model GGM02C are available.</p><sec id="s3_1"><title>3.1. Terrestrial Gravity Data</title><p>In this study, terrestrial gravity data were obtained by the “Office de la Recherche Scientifique et Technique d’Outre-Mer” (ORSTOM) [<xref ref-type="bibr" rid="scirp.77685-ref12">12</xref>] [<xref ref-type="bibr" rid="scirp.77685-ref21">21</xref>] . This</p><fig id="fig2"  position="float"><label><xref ref-type="fig" rid="fig2">Figure 2</xref></label><caption><title> Geological map of the Adamawa region-Cameroon modified from [<xref ref-type="bibr" rid="scirp.77685-ref14">14</xref>] </title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/2-2801462x3.png"/></fig><p>organization has a very large database and excellent quality recognized internationally. These data were acquired with the Worden and Lacoste Romberg gravimeters. All gravity measurements are tied to the International Gravity Standardization Network 1971 (IGSN71) datum after correction of luni-solar effect and instrumental drift. To determine the free air anomaly, the linear vertical gradient of 0.3086 mGal/m was used to approximate free air correction. Coordinates stations were determined from topographic maps. Elevation values were obtained with Wallace and Tiernan altimeters. An average rock density of 2.67 g/m<sup>3</sup> was introduced for simple Bouguer reduction. Due to the presence of relatively smooth topography, no terrain correction was added. The resulting Bouguer anomaly contour map in the study area <xref ref-type="fig" rid="fig3">Figure 3</xref> constructed using the Generic Mapping Tools (GMT) [<xref ref-type="bibr" rid="scirp.77685-ref22">22</xref>] shows three gravity sectors.</p><p>The first sector, located in the central part of the study area consists of a vast negative anomaly that goes from Garoua-Boulai to Djohong passing through</p><fig id="fig3"  position="float"><label><xref ref-type="fig" rid="fig3">Figure 3</xref></label><caption><title> Bouguer anomaly map of the region obtained by using terrestrial gravity data</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/2-2801462x4.png"/></fig><p>Meiganga, covers the entire city of Ngaoundere. An overview of the configuration of anomalies shows a dominant direction NE-SW, which corresponds to the large fault that extends from Foumban to the Mbere Ditch. The magnitude of these anomalies is approximately −100 mGal with minimums reaching −120 mGal. They can be interpreted as the effect of low density formations. The second sector, situated in the southern part of the study area consists of heavy gravity anomaly. This anomaly with amplitude of about −50 mGal can be link to the presence of dense rocks in this sector. The third sector, situated in the northern part of the region, between parallels 7.30˚ to 8˚N, which covers the Ngaoundere mountain zone is characterized by negative anomaly (−75 mGal) with dominant EW trend. This anomaly does not indicate any geological formation, because the zone is composed of basaltic rocks inside the basement. It is due probably either to the lack of gravity data in the region, or the effect of neighboring formations. The orientation of iso-lines of anomalies in this zone does not objectively identify the direction of the Ngaoundere mountain. The Bouguer anomaly map shows some limitations making a difficult to do the proper gravity investigations. The structure of Adamawa plateau remains poorly knows. To solve this problem, terrestrial gravity data must undergo using data from the global geopotential model GGM02C [<xref ref-type="bibr" rid="scirp.77685-ref7">7</xref>] [<xref ref-type="bibr" rid="scirp.77685-ref23">23</xref>] .</p></sec><sec id="s3_2"><title>3.2. Global Geopotentiel Model: GGM02C</title><p>In this part of study data from the Global Geopotential Model were used [<xref ref-type="bibr" rid="scirp.77685-ref23">23</xref>] [<xref ref-type="bibr" rid="scirp.77685-ref24">24</xref>] . The GGM02C model has been publicly released by Deutsches Zentrum f&#252;r Luftund Raumfahrt (DZLR). This model has several advantages: (1) It provides good information in areas previously inaccessible or having terrestrial data gaps and extends across natural and artificial boundary; (2) it incorporates data from different sources including satellite altimetry over oceans, satellite gravity and the terrestrial gravity [<xref ref-type="bibr" rid="scirp.77685-ref20">20</xref>] . In addition, this model represents better the gravity anomalies in the Adamawa plateau. The GGM02C model is complete to spherical harmonic degree and order 200 [<xref ref-type="bibr" rid="scirp.77685-ref7">7</xref>] [<xref ref-type="bibr" rid="scirp.77685-ref8">8</xref>] [<xref ref-type="bibr" rid="scirp.77685-ref25">25</xref>] . The data are first obtained as free-air gravity anomalies and then corrected to underline topographic effects using a Digital Elevation Model (DEM) GLOBE [<xref ref-type="bibr" rid="scirp.77685-ref24">24</xref>] . A reduction density of 2.67 g/m<sup>3</sup> was used for the Simple Bouguer correction. According to [<xref ref-type="bibr" rid="scirp.77685-ref7">7</xref>] [<xref ref-type="bibr" rid="scirp.77685-ref8">8</xref>] , the GGM02C gravity data and terrestrial ones have the same precision; so they are stackable and can be superimposed. The better coverage of gravity data has undoubtedly permitted us to draw a better simple Bouguer anomaly map of the region. This map has strengthened some hypotheses already supported by the geological data but not addressed by previous geophysical studies carried out in the study area so far. The orientation of the anomalies agrees well with the overall direction of the tectonic and geological structures. Same as the previous map, the Bouguer anomaly map obtained by combination of terrestrial and GGM02C gravity data (<xref ref-type="fig" rid="fig4">Figure 4</xref>) reveals three gravity sectors.</p><p>The first sector, located in the middle part of the study area is constituted by negative anomaly with NE-SE direction that goes from Betare-Oya to Djohong passing through Graoua-Boulai and covers the entire city of Ngaoundere and Belel. This anomaly with amplitude of −120 mGal can be considered as the effect of the low densities formations. In this sector heavy anomalies (−20 to −30 mGal) appear in the Mbere basin area. The shape of these anomalies indicates that they would have been affected by folding which occurred during different tectonic phases that have affected the region [<xref ref-type="bibr" rid="scirp.77685-ref26">26</xref>] . The presence of heavy anomalies with NE-SO direction is due to the presence of dense formations under the sedimentary environment. These results are in agreement with geological observations which show that the entire sedimentary series is swung northward [<xref ref-type="bibr" rid="scirp.77685-ref13">13</xref>] [<xref ref-type="bibr" rid="scirp.77685-ref14">14</xref>] . The second sector that covers the south-west of Kongolo is characterized by heavy anomalies (−40 mGal) indicating the presence of dense formations. It is composed mainly of migmatic rocks. The third sector, which situated in the south of Mbe and covers the Volcanic mountain zone, consists of heavy anomalies (−20 mGal) and weak anomalies (−140 mGal) with NE-SO direction. This</p><fig id="fig4"  position="float"><label><xref ref-type="fig" rid="fig4">Figure 4</xref></label><caption><title> Bouguer anomaly map of the region obtained after densification of gravity data</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/2-2801462x5.png"/></fig><p>map shows that weak anomalies appear in the central part of the massif. These anomalies are due to the collapsing of the crust or are due to the presence of granitic rocks constituting the socle. Heavy anomalies appear in the northern and southern slope of the mountain corresponds to the basaltic intrusion in this area. The direction of anomalies in this map is visibly more developed than that before densification. This direction coincides perfectly with ENE-WSW direction of the Adamawa Plateau and suggests that the intrusion could have been controlled by the tectonic processes.</p><p>In gravity method, the Bouguer anomaly map generally overshadow the effects of density contrasts, deep and shallow, wide and local. Regional-residual separation allows to isolate the anomaly due to deep sources and extended than those from density contrast reduced and shallower extension. This separation was made in our previous works and the residual of order 5 was the best amenable for the geological structures near surface in the Adamawa plateau [<xref ref-type="bibr" rid="scirp.77685-ref7">7</xref>] . In the present work the residual of order 5 will be exploited.</p><p>The regional anomaly map (<xref ref-type="fig" rid="fig5">Figure 5</xref>) is characterized by a negative gravity anomaly in the center bounded by gradients increasing towards the north. These observations show that the basement is deepening towards the south of the region. Indeed, using geophysical analysis of gravity data, the crustal thickness beneath the northern edge of the Adamawa plateau is about 23 km and 33 km in the north and south respectively [<xref ref-type="bibr" rid="scirp.77685-ref5">5</xref>] [<xref ref-type="bibr" rid="scirp.77685-ref27">27</xref>] . We noticed that, the regional Bouguer</p><fig id="fig5"  position="float"><label><xref ref-type="fig" rid="fig5">Figure 5</xref></label><caption><title> Fifth-order of regional Bouguer anomaly map of the region obtained after densification of the gravity data</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/2-2801462x6.png"/></fig><p>anomaly is dominated by the effect of structures located beyond the Moho. At the level of Mbe the iso-lines of anomalies were NE-SW direction then passed EW to ESE-WNW in the center of study area. This multiple direction of iso- lines indicates that the basement has found at great depth [<xref ref-type="bibr" rid="scirp.77685-ref13">13</xref>] [<xref ref-type="bibr" rid="scirp.77685-ref16">16</xref>] . To the east of meridian 6˚N, the region is constituted by the −100 mGal contour line within which is Garoua-Boulai and Meiganga. This contour line is close and represents the thinning of the lithosphere due to asthenospheric uplift under the Adamawa [<xref ref-type="bibr" rid="scirp.77685-ref2">2</xref>] [<xref ref-type="bibr" rid="scirp.77685-ref27">27</xref>] .</p><p>Residual Bouguer anomaly map of the study area (<xref ref-type="fig" rid="fig6">Figure 6</xref>) shows two different sectors: positive sector and negative sector which amplitudes are respectively (+40 and −70 mGal). The positive sector is founded between Ngaoundere</p><fig id="fig6"  position="float"><label><xref ref-type="fig" rid="fig6">Figure 6</xref></label><caption><title> Fifth-order of residual Bouguer anomaly map of the region obtained after densification of gravity data</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/2-2801462x7.png"/></fig><p>and Mbe (P1), north-east of Ngaoundere (P2) and north-east of Djohong (P3) localities indicates uplift basement and lateral high dense rocks. In geological considerations, at level of Djohong the positive residual Bouguer anomaly is assigned to the thinning down of the crust on the one hand and on the other hand to the existence of invisible basaltic rocks under the granite-gneisses basement. Between Ngaoundere and Mbe and north-east of Ngaoundere, the positive anomaly corresponds to the intrusion of dense rock of high density under the low density formation. The negative sector observed around Ngaoundere and north of Belel trending NE-SW. A comparison of this negative anomaly with the geological map shows that, this anomaly is due to the collapsing of the crust and the effect of low density formation. In south and east of Mbe, three peaks of negative anomalies appear in the central part of the massif, the average value of these Bouguer anomalies is −30 mGal. In general Bouguer anomalies are usually negative in the massif and mountains because of the isostasy. The rock density of their root is lower than that of the surrounding earth’s mantle. The presence of these peaks of anomalies indicates that, the massif has a variable thickness and is more rooted in these areas than elsewhere. The setting of this massif is linked to a general collapse of the socle in the region. The positive and negative sector is separated by a steep gradient, which corresponds to the effect of discontinuity between two different structures. In order to provide more information in the study area and to show the capability of densified data to detect unknown geological structures, spectral analysis and 3D density inversion based on the geological map were used along three profiles drawn on the residual Bouguer anomaly map.</p></sec></sec><sec id="s4"><title>4. Method</title><sec id="s4_1"><title>4.1. Power Spectrum Analysis</title><p>Spectral analysis as described by [<xref ref-type="bibr" rid="scirp.77685-ref28">28</xref>] is a technical method based on the property of the energy spectrum of the gravity data. It estimates the depths of perturbing bodies. Generally extended anomaly with amplitude which decreases rapidly is characterized by high frequency. However, large anomaly which amplitude decreases slightly is characterized by low frequency spectrum [<xref ref-type="bibr" rid="scirp.77685-ref29">29</xref>] [<xref ref-type="bibr" rid="scirp.77685-ref30">30</xref>] . The estimation of the depths is controlled by the choice of the line defining the slopes. When the energy spectrum logarithm is plotted versus wavenumber, we choose the straight-line segments whose slopes are proportional to the depth of the perturbing body according to the following relation [<xref ref-type="bibr" rid="scirp.77685-ref31">31</xref>] [<xref ref-type="bibr" rid="scirp.77685-ref32">32</xref>] :</p><disp-formula id="scirp.77685-formula105"><label>(1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-2801462x8.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2801462x9.png" xlink:type="simple"/></inline-formula> is the variation of the logarithm of the energy spectrum <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2801462x10.png" xlink:type="simple"/></inline-formula> a wavenumber and h (km) is the depth of perturbing bodies. In this case, h1 corresponds to the deep density contrast plane and h2: shallow density contrast plane. According to [<xref ref-type="bibr" rid="scirp.77685-ref33">33</xref>] the errors value on each profile is 5% of the mean depth value.</p></sec><sec id="s4_2"><title>4.2. 3D Density Inversion</title><p>For 3D density inversion of the structures in the Adamawa plateau we used GRABLOX2 (version 2.1) by [<xref ref-type="bibr" rid="scirp.77685-ref34">34</xref>] . This program calculates the gravity field for 3D block model. A block model is a block divided into cubes. For each cube we note constant density. The program uses two methods: Occam inversion and Singular Value Decomposition (SVD) [<xref ref-type="bibr" rid="scirp.77685-ref35">35</xref>] . For each method there are three options for setting the model (density, height and density + height) [<xref ref-type="bibr" rid="scirp.77685-ref9">9</xref>] [<xref ref-type="bibr" rid="scirp.77685-ref10">10</xref>] . Occam inversion needs to solve much larger matrix system than the SVD. The SVD inversion creates a smooth and continuous model if the gravity data are dense. In such situations the Occam inversion gets unstable and generates very rugged structures. In this study, the Singular Value Decomposition will be used for 3D density inversion. The coefficients of the base of anomaly can be optimized separately for the gravity and gradient data. Spectral analysis is used to constrain depths of bodies responsible for positives anomalies which correlated to the surface geology. The residual and regional anomalies were read with separated format. The inversion will resolve residual density where the mean density of the modeled volume should be added to give geologically realistic density values. For our study densities of the blocks fixed by recent works [<xref ref-type="bibr" rid="scirp.77685-ref9">9</xref>] are used to define the initial model. In this case, the background value should be set to the mean of the density value used in Bouguer corrections (2.67 g/m<sup>3</sup>). We used Grablox2 program to optimize densities of the minor blocks model then compare it with the observed Bouguer anomaly. When the observed and calculated Bouguer anomaly is realized, the inversion is obtained. After inversion the distribution of the densities inside the resulting blocks models can be used in geological interpretations.</p></sec></sec><sec id="s5"><title>5. Results and Discussions</title><sec id="s5_1"><title>5.1. Power Spectrum Analysis</title><p>To estimate the average depths of perturbing bodies responsible for gravity data, we used spectral analysis of three profiles (P1, P2, P3) drawn on the residual Bouguer anomaly map. These profiles are executed perpendicular to the main direction of the structure under study and crossed largely the zone where the structure is suspected [<xref ref-type="bibr" rid="scirp.77685-ref29">29</xref>] . For the three previous profiles <xref ref-type="fig" rid="fig7">Figure 7</xref> presented the power spectrum curves. Two major discontinuities of densities have been identified, the first h1 represents the low frequency associated to deep-seated bodies and h2 represents the high frequency causes by bodies near surface. The deepest discontinuity result of profile P1, P2 and P3 are 8.64 km, 14.41 and 5.80 km respectively for a mean of 9.62 km. These depths could be correspond to the Moho depth in the study area. These results agree with those obtained by [<xref ref-type="bibr" rid="scirp.77685-ref33">33</xref>] . According to this author, the discontinuity of structure in the Adamawa uplift is between 7 and 13 km (with a mean of 11 km). Our result and those obtained by [<xref ref-type="bibr" rid="scirp.77685-ref33">33</xref>] have few differences.</p><p>The depths obtained by [<xref ref-type="bibr" rid="scirp.77685-ref33">33</xref>] are based on only terrestrial gravity data while</p><fig id="fig7"  position="float"><label><xref ref-type="fig" rid="fig7">Figure 7</xref></label><caption><title> Power spectrum of profiles P1, P2 and P3 from spectral analysis program</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/2-2801462x11.png"/></fig><p>our results are integrating new gravity data in the existing. The second discontinuity associated with the shallowest depths for profiles P1, P2 and P3 is respectively 3.52 km, 5.86 and 2.10 km for a mean of 3.83 km. This value indicates that the sources of anomalies are not deep in the sedimentary basin. These depths are probably due to the base of Mbere sedimentary basin which could be associated with volcanic intrusions due to the positive gravity anomaly. These bodies may be due to the intrusions of dense materials in the basement and could be the boundary between the lower crust and the upper crust. The depths of 3.83 km and 9.62 km are the new values of depths obtained for futures investigations in the Adamawa plateau.</p></sec><sec id="s5_2"><title>5.2. 3D Density Inversion</title><p>The 3D density inversion was obtained using three profiles P1, P2 and P3 trending NE-SE. This inversion informs us to the structure of the Adamawa Plateau.</p><p>The structural model associated with profile (P1) (<xref ref-type="fig" rid="fig8">Figure 8</xref>) consists of three</p><fig id="fig8"  position="float"><label><xref ref-type="fig" rid="fig8">Figure 8</xref></label><caption><title> Interpreted 3D density model of profile (P1) from Grablox2 program showing different formations: 1: Granites; 2: Gneisses; 3: Basaltic rocks</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/2-2801462x12.png"/></fig><p>bodies with different compositions. The first body (1) with lower densities between 2.60 g/m<sup>3</sup> and 2.73 g/m<sup>3</sup> is situated at 5 km in the middle and 8 km in the north and south of the model. This formation corresponds to the granitic rock under the crust which the signature is due to the negative Bouguer anomalies observed in this zone. The second body (2) located at the end of the model has a lateral extension and roof that can reach 4 km. This formation with densities ranging from 2.75 g/m<sup>3</sup> to 2.78 g/m<sup>3</sup> can be associated to the gneisses formations. The third body (3) extended laterally beneath the granites in the study area has high density between 2.8 g/m<sup>3</sup> and 2.8 g/m<sup>3</sup>. This body corresponds to the basaltic intrusion which the signature is due to positive gravity anomaly observed on the Bouguer anomaly map.</p><p>The structural model of the second profile (P2) (<xref ref-type="fig" rid="fig9">Figure 9</xref>) consists of three bodies with different shapes, positions and thicknesses. The body (1) starts and</p><fig id="fig9"  position="float"><label><xref ref-type="fig" rid="fig9">Figure 9</xref></label><caption><title> Interpreted 3D density model of profile (P2) from GRABLOX showing different formations: 1: Granites; 2: Gneisses; 3: Basaltic rocks</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/2-2801462x13.png"/></fig><p>ends of the model, is constituted with lower density ranging from 2.60 g/m<sup>3</sup> to 2.73 g/m<sup>3</sup>. This body corresponds to the granitic intrusion at great deep with an extension of about 40 km. The second body (2) with density ranging from 2.75 g/m<sup>3</sup> to 2.78 g/m<sup>3</sup> designed gneisses formations in the basement of the study area. This body begins from surface area and reaches at 8 km in the middle of the model. A layer with density between 2.80 g/m<sup>3</sup> and 2.90 g/m<sup>3</sup> corresponds to the high basement structure body (3) located in the middle of the model. This body constitutes the main pluton of the complex, extends laterally at depth beyond the gneisses and corresponds to the basaltic formations. These formations have been put in place with the aid of the asthenospheric rise which leads to a lithospheric bulge. They are responsible for the positive Bouguer anomaly observed in this area.</p><p>Like the other profiles, the general features of profile (P3) (<xref ref-type="fig" rid="fig1">Figure 1</xref>0) have three principal bodies. The first body (1) with lower density ranging from 2.20 to</p><fig id="fig10"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref>0</label><caption><title> Interpreted 3D density model of profile (P3) from GRABLOX showing different formations: 1: Sedimentary formations; 2: Granites; 3: Basaltic rocks</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/2-2801462x14.png"/></fig><p>2.45 g/m<sup>3</sup> is located in the north and south extremity of the model. This body begins at 6 km and 4 km respectively at the start and at the end of model. The negative Bouguer anomaly observed in the northern and southern border of the profile can be attributed to the sedimentary deposit with low density in the study area. The second body (2) with density ranging from 2.68 to 2.78 g/m<sup>3</sup> in the middle of the model can be associated with gneiss formation. This formation is at the origins of the positive Bouguer anomaly observed in this zone and related the crustal thickening of the region followed by the fracturing which must have lead to the collapse of large blocks of crust with dimensions of several kilometers. The third body (3) with density between 2.84 g/m<sup>3</sup> and 3.00 g/m<sup>3</sup>, corresponds to the main pluton of the complex and extends laterally at depth beyond granites. This body with high density has a depth beyond 6 km and an extension of about 18 km under the basement. This body is interpreted as a rise of the basaltic rocks in the socle. It generates a positive Bouguer anomaly observed in this area and it installation is carried out in the following way: During a volcanic eruption, the magma crystallizes in deep into magmatic pockets without completely crossing the crust. In this study we observed a spectacular ascent of magmatic rocks, whose roof is about 2.5 km. The topographic expression of this process is the formation of the Adamawa plateau which is accompanied by brittle tectonics characterized by cracks and fractures.</p></sec></sec><sec id="s6"><title>6. Conclusion</title><p>In this work, the main objective is to analyze the new Bouguer anomaly map and to determine the depth and density of subsurface structure of the Adamawa plateau by using combined gravity data. The resulting residual Bouguer anomaly map shows positive and negative anomaly. Positive residual anomalies are due to the basaltic structures under granite-gneisses basement while negative gravity anomalies are due to the granite formations or the sedimentary basin. Spectral analysis and 3D density inversion show the depths and densities of geological structures associated with the positive residual Bouguer anomaly. The depths of 3.83 km and 9.62 km are the new values of depths obtained for futures investigations in the study area. This area is composed by granitic formation with density ranging from 2.60 to 2.73 g/m<sup>3</sup>, sedimentary formation with density ranging from 2.20 to 2.45 g/m<sup>3</sup>, gneisses and basaltic rocks with density between 2.75 to 2.78 g/m<sup>3</sup> and 2.84 to 3.0 g/m<sup>3</sup> respectively. Our results contain more additional information than those obtained from terrestrial gravity data. Some recent models such as GOCE are also available, but have not yet been fully tested in the study area. For future investigation we will compare several field models from GOCE to choose the one that represents the best gravity data in order to improve the gravity analysis in the Adamawa plateau.</p></sec><sec id="s7"><title>Acknowledgements</title><p>The authors would like to thank Markku Pirttij&#228;rvi (Universty of Oulu Finland) for helpful the 3D density inversion and Late Henry Duquenne (LAREG, France) for putting at our disposal the GGM program. The authors also acknowledge all the reviewers for their constructive comments.</p></sec><sec id="s8"><title>Cite this paper</title><p>Apollinaire, B., Joseph, K., Tabod, T.C., Loudi, Y., Robert, N., Ludovic, K.H. and Valentin, O. (2017) Subsurface Structural Mapping Using Com- bined Terrestrial and Grace Gravity Data of the Adamawa Plateau (North-Cameroon). International Journal of Geosciences, 8, 869-887. https://doi.org/10.4236/ijg.2017.87050</p></sec></body><back><ref-list><title>References</title><ref id="scirp.77685-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Poudjom-Djomani, Y.H., Diament, M. and Albouy, Y. (1992) Mechanical Behaviour of the Lithosphere beneath the Adamawa Uplift (Cameroon, West Africa) Based on Gravity Data. Journal of Africa Earth Sciences, 15, 81-90.  
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