<?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">OJG</journal-id><journal-title-group><journal-title>Open Journal of Geology</journal-title></journal-title-group><issn pub-type="epub">2161-7570</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/ojg.2024.141002</article-id><article-id pub-id-type="publisher-id">OJG-130442</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>
 
 
  Insight from Lithostructural and Aeromagnetic Data from the L&#233;o Square Degree, Central-Western Burkina Faso
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Adama</surname><given-names>Ouédraogo Yaméogo</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>Pascal</surname><given-names>Ouiya</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>Gounwendmanaghré</surname><given-names>Hubert Zongo</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>Omar</surname><given-names>Akonyiré</given-names></name><xref ref-type="aff" rid="aff4"><sup>4</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Abraham</surname><given-names>Seydoux Traoré</given-names></name><xref ref-type="aff" rid="aff4"><sup>4</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Saga</surname><given-names>Sawadogo</given-names></name><xref ref-type="aff" rid="aff4"><sup>4</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Séta</surname><given-names>Naba</given-names></name><xref ref-type="aff" rid="aff4"><sup>4</sup></xref></contrib></contrib-group><aff id="aff4"><addr-line>Unité de Formation et de Recherche en Sciences de la Vie et de la Terre, Laboratoire Géosciences et Environnement (LaGE), Département des Sciences de la Terre, Université Joseph Ki-Zerbo, Ouaga, Burkina Faso</addr-line></aff><aff id="aff3"><addr-line>Ecole Supérieure d’Ingénieries, Université de Fada N’gourma, Fada N’Gourma, Burkina Faso</addr-line></aff><aff id="aff1"><addr-line>Unité de Formation et de Recherche en Sciences et Technologies, Département des Sciences de la Vie et de la Terre, Université Norbert Zongo, Koudougou, Burkina Faso</addr-line></aff><aff id="aff2"><addr-line>Ecole Normale Supérieure (ENS)/Institut des Sciences et de Technologie (IST), Ouaga, Burkina Faso</addr-line></aff><pub-date pub-type="epub"><day>05</day><month>01</month><year>2024</year></pub-date><volume>14</volume><issue>01</issue><fpage>19</fpage><lpage>28</lpage><history><date date-type="received"><day>14,</day>	<month>December</month>	<year>2023</year></date><date date-type="rev-recd"><day>9,</day>	<month>January</month>	<year>2024</year>	</date><date date-type="accepted"><day>12,</day>	<month>January</month>	<year>2024</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>
 
 
  This study, carried out in the L&#233;o square degree (west-central Burkina Faso) in the Palaeoproterozoic domain of the Man/L&#233;o ridge, aims to define the shapes and positions of granitic plutons and the organisation of deformation structures using aeromagnetic data. These data have shown that there are small sub-circular granitic bodies to the north of the granitic masses in this region, and a large sub-circular granitic body to the south, around which are other smaller granitic bodies. The lineament map shows that the deformation structures are organised along three main directions and largely form these sub-circular plutonic bodies. We suggest that the granitic plutons are coalescent, pending identification of the internal structures of these granites to further refine the geodynamic model.
 
</p></abstract><kwd-group><kwd>Burkina Faso</kwd><kwd> Lineaments</kwd><kwd> Belts Rocks</kwd><kwd> Leo’s Leaf</kwd><kwd> Granito&amp;#239;d</kwd><kwd> Airbornes Magn&#233;tics</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>The Paleoproterozoic basement of the Man/Leo shield, also known as the Baoul&#233;-Mossi domain (<xref ref-type="fig" rid="fig1">Figure 1</xref>), consists of belts of greenstone and granitoids that represent interesting targets for mining exploration [<xref ref-type="bibr" rid="scirp.130442-ref1">1</xref>] . The emplacement of biotite-granite plutons is very often related to the functioning of the large</p><p>transcurrent shear zones that characterise Eburnian tectonics [<xref ref-type="bibr" rid="scirp.130442-ref2">2</xref>] [<xref ref-type="bibr" rid="scirp.130442-ref3">3</xref>] [<xref ref-type="bibr" rid="scirp.130442-ref4">4</xref>] . These large transcurrent shear zones are also known for their importance in the history of gold mineralisation [<xref ref-type="bibr" rid="scirp.130442-ref5">5</xref>] - [<xref ref-type="bibr" rid="scirp.130442-ref12">12</xref>] . Examples show that these are often close to deposits of economic size, such as the Essakane gold mine in Burkina Faso, the Kiaka deposit in Burkina Faso, the Sissingu&#233; gold mine in C&#244;te d’Ivoire, ... (<xref ref-type="fig" rid="fig1">Figure 1</xref>). However, in certain areas of the Baoul&#233;-Mossi region, most of the geological formations and many of the deformation structures that affect them are covered by thick layers of sedimentary rock, making geological mapping and mining exploration difficult [<xref ref-type="bibr" rid="scirp.130442-ref13">13</xref>] [<xref ref-type="bibr" rid="scirp.130442-ref14">14</xref>] . Therefore, the use of aeromagnetic data is a solution to study these types of terrain.</p><p>Aeromagnetic data are an essential source of information for regional geological mapping and the exploration of mineral and water resources. These data can be easily integrated into all stages of geological mapping, and the various treatments of the magnetic field make it possible to define geophysical anomalies associated with the presence of geological formations and deformation structures.</p><p>This study focuses on the L&#233;o square degree in Burkina Faso, where the basement formations are largely covered by sedimentary formations. Pending detailed field investigations, this work helps to determine the shape and position of the granitoids and to define the major and/or secondary structures likely to be associated with the emplacement of these granitoids.</p></sec><sec id="s2"><title>2. Geological Setting</title><p>The Leo square degree covers part of west-central Burkina Faso, between 2˚ and 3˚ west longitude and between 11˚ and 12˚ north latitude (<xref ref-type="fig" rid="fig2">Figure 2</xref>). The Leo square degree consists of Paleoproterozoic formations that represent a period of major crustal accretion during the Eburnian orogeny. These formations are essentially composed of volcanic-sedimentary and plutonic terrains metamorphosed during the Eburnian and plutonic formations intrusive into the latter [<xref ref-type="bibr" rid="scirp.130442-ref15">15</xref>] .</p><p>The Eburnian metamorphosed volcano-sedimentary and plutonic formations outcrop in the north-south trending Boromo belt to the west of the (<xref ref-type="fig" rid="fig2">Figure 2</xref>). The intrusive plutonic formations consist of TTG granitoids and biotite granites, which outcrop over most of the sheet (<xref ref-type="fig" rid="fig2">Figure 2</xref>).</p><p>Outcrop conditions are generally poor. Nevertheless, deformation structures can be observed and measured in the outcrops. These structural features take the form of contacts, planar structures and ductile detachment corridors. The work of [<xref ref-type="bibr" rid="scirp.130442-ref15">15</xref>] highlighted major shear zones, including the Boromo shear zone to the west of the L&#233;o sheet. The functioning of this shear zone has induced secondary shear zones in the geological formations. The belt formations are highly deformed and oriented approximately north-south along the major shear corridor. The outcropping TTG granitoids are affected by a ribboning pattern running roughly in this direction. Overall, the biotite granites show no measurable structures.</p></sec><sec id="s3"><title>3. Methodology</title><p>Aeromagnetic data are used in geological mapping studies and offer the advantage of rapid coverage of large study areas with the possibility of investigation at depth. The aeromagnetic data acquired by BUMIGEB were processed using GEOSOFT’s OASIS MONTAJ software. The use of filters is essential in order to obtain accurate and meaningful images suitable for the interpretation of geological formations and structures. The following processing operations were carried out at this stage:</p><p>- Pole reduction (RTP) is an operation that transforms an asymmetric anomaly measured at any latitude into a simulated symmetric anomaly at the pole. This transformation corresponds to a calculation of the change in phase of the magnetic signal that returns the magnetic anomaly to its source.</p><p>- The vertical derivative (first vertical derivative) or vertical gradient is the vertical gradient of the residual magnetic field. It assesses the rate of change of the magnetic field of the sources with depth. The vertical gradient map is based on the detection of surface structures, i.e. it is a digital high-pass filter.</p><p>- The analysis signal allows the distribution of lithologies and their magnetic properties to be observed. Conversely, information about the structures is lost.</p><p>- Shading is an additional processing that enhances the hue of the black and white image to highlight structures and regional anomalies.</p><p>The second phase of the study involved an interpretation of the major lineaments in the study area as revealed by the magnetic signatures.</p></sec><sec id="s4"><title>4. Results</title><p>The total magnetic field map shows that the strongest anomalies are observed in the western and central parts of the L&#233;o sheet (<xref ref-type="fig" rid="fig3">Figure 3</xref>). These strong magnetic anomalies are associated with basic and ultrabasic rocks.</p><p>In places, short negative anomalies cross the geological formations in a NW-SE direction, clearly visible on the total magnetic field map and highlighted on the 45˚ shaded analytical signal map. Their orientation coincides with that of the dolerite dykes.</p><p>Weak to non-magnetic anomalies occur to the north and south of the square degree and generally correspond to acidic rocks (<xref ref-type="fig" rid="fig3">Figure 3</xref>). The 45˚ shaded analytical signal map shows sub-circular bodies corresponding to zones of weak to non-magnetic anomalies, which are confirmed by significant uranium anomalies on the U-Th-K ternary maps (<xref ref-type="fig" rid="fig4">Figure 4</xref>(a) and <xref ref-type="fig" rid="fig4">Figure 4</xref>(b)). This feature is unique to felsic bodies.</p><p>Strong magnetic anomalies corresponding to more or less elongated bodies are clearly highlighted on the 45˚ shaded analytical signal map (<xref ref-type="fig" rid="fig4">Figure 4</xref>(a) and <xref ref-type="fig" rid="fig4">Figure 4</xref>(b)). On the U-Th-K ternary maps, the dark areas correspond to basic to ultrabasic formations with low levels of natural radioactivity. However, there is a strong uranium anomaly to the west of the square degree at the location of the belt rocks, probably due to rainwater drainage of the granitoid alteration products (<xref ref-type="fig" rid="fig4">Figure 4</xref>(b)).</p><p>The L&#233;o sheet is affected by intense deformation. These are expressed by structures that can be observed on the lineament map and are organised in three main directions (<xref ref-type="fig" rid="fig5">Figure 5</xref>). On the 45˚ shaded analytical signal map, certain structures mould the subcircular bodies, which are clearly the granitoids. The main directions are : NNE-SSW, NE-SW and NW-SE.</p></sec><sec id="s5"><title>5. Discussion</title><p>By superimposing the aeromagnetic data (magnetic field) on the 1:200,000 geological map of the L&#233;o sheet [<xref ref-type="bibr" rid="scirp.130442-ref15">15</xref>] , the strong magnetic anomalies correspond to basic rocks and the weak magnetic anomalies to acidic rocks [<xref ref-type="bibr" rid="scirp.130442-ref16">16</xref>] [<xref ref-type="bibr" rid="scirp.130442-ref17">17</xref>] [<xref ref-type="bibr" rid="scirp.130442-ref18">18</xref>] . Using aeromagnetic data, petrographic facies can be clearly distinguished and the lithology of the L&#233;o sheet confirmed (<xref ref-type="fig" rid="fig2">Figure 2</xref>, <xref ref-type="fig" rid="fig3">Figure 3</xref>). The mainly NW-SE-trending dolerite dykes have been identified on the aeromagnetic maps by their strong, linear signal (e.g., [<xref ref-type="bibr" rid="scirp.130442-ref19">19</xref>] [<xref ref-type="bibr" rid="scirp.130442-ref20">20</xref>] ).</p><p>This lithology is diverse and largely dominated by a large mass of granitoids, particularly biotite granites of variable texture. On the map of the analytical signal shaded at 45˚, we can see that in this large mass of granitoids, the subcircular bodies moulded by curvilinear structures are clearly visible. In the field, this feature is not observable because of the thick layer of weathering in the area. On the</p><p>basis of previous work [<xref ref-type="bibr" rid="scirp.130442-ref3">3</xref>] [<xref ref-type="bibr" rid="scirp.130442-ref4">4</xref>] [<xref ref-type="bibr" rid="scirp.130442-ref21">21</xref>] which has explained similar situations, we suggest that the presence of subcircular granitic bodies associated with curvilinear structures could be explained by coalescence. On the basis of the organisation of lineaments around biotite granites and their internal structures in the Dori region, Yam&#233;ogo et al. 2023 [<xref ref-type="bibr" rid="scirp.130442-ref4">4</xref>] show that the Gorom-Gorom granite, which appears homogeneous from field observation, consists of coalescing plutons. In this case, we do not have the internal structures of biotite granites.</p><p>The lineament map clearly shows that the flow schistosity (S1) is taken up by the N-S to NE-SW shear. In the volcanic sedimentary formations, the structures are vertical schistosities of variable intensity [<xref ref-type="bibr" rid="scirp.130442-ref15">15</xref>] . These structures are related to D1 and D2. D1 deformation phase structures are characterised in Burkina Faso and elsewhere in the West African craton by major faults, foliations and folds, and thrusts [<xref ref-type="bibr" rid="scirp.130442-ref9">9</xref>] [<xref ref-type="bibr" rid="scirp.130442-ref10">10</xref>] [<xref ref-type="bibr" rid="scirp.130442-ref22">22</xref>] - [<xref ref-type="bibr" rid="scirp.130442-ref27">27</xref>] . D2 deformation phase structures are N-S to NE trending sub-vertical shear zones in Burkina-Faso [<xref ref-type="bibr" rid="scirp.130442-ref22">22</xref>] [<xref ref-type="bibr" rid="scirp.130442-ref23">23</xref>] .</p></sec><sec id="s6"><title>6. Conclusion</title><p>The magnetic data have highlighted the diversity of the geological formations of the square degree of Leo through their magnetic signatures. The study clearly shows that the granite plutons of the square degree of Leo, which appear homogeneous in the field, are coalescing. Lineament analysis also indicates several deformation structures, some of which are organised around the biotite granites. Further studies using Anisotropy of Magnetic Susceptibility (AMS) and microstructural studies will clarify the internal structures of the biotite granites. At this stage, we will be able to show the relationship between the emplacement of the biotite granites and the functioning of the shear zones.</p></sec><sec id="s7"><title>Acknowledgements</title><p>We are very grateful to Prof. NABA S&#233;ta of the Joseph Ki-Zerbo University for his invaluable contribution to this work.</p></sec><sec id="s8"><title>Conflicts of Interest</title><p>The authors declare no conflicts of interest regarding the publication of this paper.</p></sec><sec id="s9"><title>Cite this paper</title><p>Yam&#233;ogo, A.O., Ouiya, P., Zongo, G.H., Akonyir&#233;, O., Trao- r&#233;, A.S., Sawadogo, S. and Naba, S. (2024) Insight from Lithostructural and Aeromagnetic Data from the L&#233;o Square Degree, Central-Western Burkina Faso. 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