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  <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">2156-8367</issn>
      <issn pub-type="ppub">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.2025.1610034</article-id>
      <article-id pub-id-type="publisher-id">ijg-146386</article-id>
      <article-categories>
        <subj-group>
          <subject>Article</subject>
        </subj-group>
        <subj-group>
          <subject>Earth</subject>
          <subject>Environmental Sciences</subject>
        </subj-group>
      </article-categories>
      <title-group>
        <article-title>Lithospheric Magnetic Anomaly in the Surrounding Area of the Dingri M6.8 Earthquake, Xizang</article-title>
      </title-group>
      <contrib-group>
        <contrib contrib-type="author">
          <name name-style="western">
            <surname>Li</surname>
            <given-names>Bo</given-names>
          </name>
          <xref ref-type="aff" rid="aff1">1</xref>
          <xref ref-type="aff" rid="aff2">2</xref>
        </contrib>
        <contrib contrib-type="author">
          <name name-style="western">
            <surname>Mao</surname>
            <given-names>Fenglong</given-names>
          </name>
          <xref ref-type="aff" rid="aff1">1</xref>
          <xref ref-type="aff" rid="aff2">2</xref>
        </contrib>
      </contrib-group>
      <aff id="aff1"><label>1</label> Baoding Central Seismic Station of Hebei Province, Baoding, China </aff>
      <aff id="aff2"><label>2</label> Hebei Hongshan National Observatory on Thick Sediments and Seismic Hazards, Xingtai, China </aff>
      <author-notes>
        <fn fn-type="conflict" id="fn-conflict">
          <p>The authors declare no conflicts of interest regarding the publication of this paper.</p>
        </fn>
      </author-notes>
      <pub-date pub-type="epub">
        <day>15</day>
        <month>10</month>
        <year>2025</year>
      </pub-date>
      <pub-date pub-type="collection">
        <month>10</month>
        <year>2025</year>
      </pub-date>
      <volume>16</volume>
      <issue>10</issue>
      <fpage>685</fpage>
      <lpage>700</lpage>
      <history>
        <date date-type="received">
          <day>24</day>
          <month>08</month>
          <year>2025</year>
        </date>
        <date date-type="accepted">
          <day>12</day>
          <month>10</month>
          <year>2025</year>
        </date>
        <date date-type="published">
          <day>15</day>
          <month>10</month>
          <year>2025</year>
        </date>
      </history>
      <permissions>
        <copyright-statement>© 2025 by the authors and Scientific Research Publishing Inc.</copyright-statement>
        <copyright-year>2025</copyright-year>
        <license license-type="open-access">
          <license-p> This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license ( <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link> ). </license-p>
        </license>
      </permissions>
      <self-uri content-type="doi" xlink:href="https://doi.org/10.4236/ijg.2025.1610034">https://doi.org/10.4236/ijg.2025.1610034</self-uri>
      <abstract>
        <p>The occurrence and development of earthquakes can cause abnormal changes in the lithospheric magnetic field. High-precision geomagnetic observations on both sides of the Dingri M6.8 epicenter revealed a −120 nT difference in the lithospheric magnetic field between the west and east sides, reflecting the local difference characteristics of the properties of the crustal medium around the epicenter. From 2018 to 2020, the annual variation of the magnetic field changed from −2.2 nT to +3.9 nT, which may be the precursor anomaly of the Dingri M5.9 earthquake in 2020. Calculations show that in the coseismic magnetic field variation of the M6.8 earthquake, the piezomagnetic effect is small while the electrokinetic effect is large, so the precursor anomaly of the M5.9 earthquake may be related to the electrokinetic effect produced by underground fluid migration.</p>
      </abstract>
      <kwd-group kwd-group-type="author-generated" xml:lang="en">
        <kwd>Dingri M6.8 Earthquake</kwd>
        <kwd>Lithospheric Magnetic Field</kwd>
        <kwd>Piezomagnetic Effect</kwd>
        <kwd>Electrokinetic Effect</kwd>
      </kwd-group>
    </article-meta>
  </front>
  <body>
    <sec id="sec1">
      <title>1. Introduction</title>
      <p>According to the official measurement of the China Earthquake Networks Center, on January 7, 2025, a magnitude 6.8 earthquake (hereinafter referred to as the Dingri earthquake) occurred in Dingri County, Xizang, with the epicenter at (28.5˚N, 87.45˚E). This earthquake occurred on the Dengmocuo fault in the southern section of the Xainza-Dingye fault system, which runs in a nearly north-south direction [<xref ref-type="bibr" rid="B1">1</xref>]. It is a normal fault-type earthquake (<xref ref-type="fig" rid="fig1">Figure 1</xref>). Due to the north-south collision and east-west tension between the Indian Plate and the Eurasian Plate [<xref ref-type="bibr" rid="B2">2</xref>], multiple catastrophic earthquakes have occurred in southern Xizang, with a high seismic risk [<xref ref-type="bibr" rid="B3">3</xref>]. There was a 5.9 magnitude earthquake around the Dingri earthquake in 2020 [<xref ref-type="bibr" rid="B4">4</xref>], but there is not much research on the seismogenic environment and regional seismic risk of the Dingri 5.9 magnitude earthquake. This may be due to the high altitude of the region, the difficulty of data collection, and most of the research focusing on large fractures at the block boundaries [<xref ref-type="bibr" rid="B3">3</xref>]. The occurrence of the Dingri earthquake once again demonstrates that small and medium-sized faults or internal faults within blocks also have the potential to cause catastrophic earthquakes [<xref ref-type="bibr" rid="B5">5</xref>]. Compared to other surrounding faults, the Dengmocuo Fault has a higher activity rate, and its seismic hazard should be taken seriously [<xref ref-type="bibr" rid="B6">6</xref>]. On-site investigation shows that the earthquake rupture mainly occurred along the epicenter towards the north, and the maximum vertical displacement found on the surface has reached 3 m [<xref ref-type="bibr" rid="B1">1</xref>], indicating the significant shallow sliding and huge energy released by the 6.8 magnitude earthquake in Dingri. Therefore, using historical observation data to conduct research on regional earthquake background and basic models is of certain significance for understanding the seismic hazard of the region, and can provide a reference for subsequent geological, geophysical, and other observations.</p>
      <fig id="fig1">
        <label>Figure 1</label>
        <graphic xlink:href="https://html.scirp.org/file/2802696-rId13.jpeg?20260616051043" />
      </fig>
      <p><bold>Figure 1.</bold> Tectonic setting of the research area (drawn according to the earthquake catalog of China Earthquake Networks Center).</p>
      <p>There is a good correspondence between earthquakes and geomagnetic field anomalies. Earthquakes with a magnitude of 6.0 or above in the Sichuan-Yunnan region often occur in areas with negative anomalies at the junction of positive and negative lithospheric magnetic fields. Recently, satellite data provides a good chance to detect pre-earthquake magnetic anomalies [<xref ref-type="bibr" rid="B7">7</xref>]-[<xref ref-type="bibr" rid="B10">10</xref>]. Many researches indicate that geomagnetic field anomalies can provide a reference for earthquake risk analysis [<xref ref-type="bibr" rid="B11">11</xref>]-[<xref ref-type="bibr" rid="B13">13</xref>]. There are few geomagnetic observation data in southern Xizang, especially in the area south of the Indus-Yarlung suture. From the fine lithospheric magnetic field model, it can only be recognized that the region is mainly a weak negative anomaly [<xref ref-type="bibr" rid="B14">14</xref>]. Whether the Dingri earthquake is at the boundary of positive and negative anomalies of the lithospheric magnetic field needs further research according to the measured data. </p>
      <p>Earthquake-induced rupture or material transport related to seismogenesis can often cause disturbances in the geomagnetic field [<xref ref-type="bibr" rid="B15">15</xref>]-[<xref ref-type="bibr" rid="B17">17</xref>], providing references for earthquake prediction, earthquake warning, earthquake rupture, and other research [<xref ref-type="bibr" rid="B18">18</xref>][<xref ref-type="bibr" rid="B19">19</xref>]. Domestic researchers have extracted multiple abnormal changes in the geomagnetic field before earthquakes through repeated observations of the geomagnetic field. These changes are usually of large magnitude, and the mechanism is not clear [<xref ref-type="bibr" rid="B20">20</xref>]-[<xref ref-type="bibr" rid="B22">22</xref>]. Unlike pre-earthquake anomaly studies, coseismic geomagnetic field anomalies exhibit characteristics of smaller magnitude and range [<xref ref-type="bibr" rid="B19">19</xref>]. Some persistent coseismic geomagnetic field anomalies can be quantitatively explained by the pressure magnetic effect [<xref ref-type="bibr" rid="B19">19</xref>][<xref ref-type="bibr" rid="B23">23</xref>], which greatly inspires earthquake geomagnetic research. Some researchers believe that the abnormal geomagnetic field before earthquakes is related to the stress changes during the pre-earthquake process [<xref ref-type="bibr" rid="B22">22</xref>]-[<xref ref-type="bibr" rid="B24">24</xref>], but they have not explained the significant changes, indicating that there are huge differences between the qualitative analysis and quantitative calculation of lithospheric magnetic field anomalies, which seriously restricts the study of seismic magnetic anomalies. The large shallow sliding of the 6.8-magnitude earthquake on Dingri may cause significant coseismic geomagnetic field anomalies. Quantitative calculation of its coseismic geomagnetic changes can provide references for subsequent regional geomagnetic field analysis.</p>
      <p>Observable seismomagnetic anomalies are correlated with both earthquake magnitude and epicentral distance. Based on analyses of case studies, Hattori <italic>et al</italic><italic>.</italic> (2004) [<xref ref-type="bibr" rid="B25">25</xref>] proposed an empirical relationship expressed as 0.025R &lt; M4.5 (where R denotes epicentral distance and M represents magnitude). This implies that the maximum epicentral distances for detecting anomalies at geomagnetic stations would be approximately 60 km for M6.0 earthquakes and 100 km for M7.0 earthquakes. For earthquakes with shallow focal depths, the spatial extent of detectable geomagnetic anomalies may be larger. To study the potential anomalous characteristics of the geomagnetic field around the Dingri earthquake, this paper obtained the variation of the geomagnetic field perpendicular to the direction of the Dengmocuo fault based on repeated observation data of the geomagnetic field obtained at 30 km on both sides of the epicenter from 2018 to 2020. At the same time, based on quantitative calculations of the geomagnetic effects of synchronous earthquakes, the changes in the magnetic field of synchronous earthquakes were obtained, and the mechanisms of synchronous and pre-earthquake magnetic field anomalies were analyzed. No geomagnetic observations have been conducted in this region since 2020, making the latest data unavailable.</p>
      <p>S1 and S2 are geomagnetic repeat measurement points; XDF is the Xainza-Dingye fault; TYKF is the TangraYumco-Kongco fault; DMC is the Dengmocuo fault; STDS is the Southern Xizang Detachment System; IYS is the Indus-Yarlung suture; Beach balls in lower left subplot are earthquakes with <italic>M</italic><italic><sub>W</sub></italic> &gt; 7.0 that occurred in the Qinghai-Yibet plateau; thick white arrow indicates the motion of the Indian plate relative to the Eurasian plate; black white arrows indicate the dilatation motion in the southern Qinghai-Xizang plateau; the red line area is the research area. </p>
    </sec>
    <sec id="sec2">
      <title>2. Data and Methods</title>
      <p>From 2018 to 2020, relevant units of the China Earthquake Administration carried out a large number of repeated observations of the geomagnetic field on the Qinghai-Xizang Plateau to fill the gap in geomagnetic field observations in the region. Each measuring point is equipped with duplicate positioning markers to ensure that repeated measurements are taken at the same measuring point, with an instrument installation error of less than 10 cm. An auxiliary measuring point is set up at a distance of 20 - 30 meters from each measuring point, and the horizontal gradient of the magnetic field within 5 meters of the measuring point and the auxiliary measuring point is less than 2 nT/m, and the vertical gradient of the magnetic field within 2 meters is less than 3 nT/m. The repeat positioning error can be controlled within 0.3 nT. During each observation, double-check the magnetic field gradient at the measuring point and the magnetic field difference between the measuring point and the auxiliary measuring point to ensure that there is no obvious human interference around the measuring point. Six sets of observations of the total intensity of the geomagnetic field will be conducted within approximately 30 minutes of each measurement, with 10 values observed in each set. The observation instruments are all GSM-19T proton precession magnetometers with a sensitivity of 0.15 nT@1Hz. The resolution is 0.01 nT and the absolute accuracy is ±0.2 nT [<xref ref-type="bibr" rid="B26">26</xref>]. </p>
      <p>Referring to the observation data of Lhasa geomagnetic station, daily variation correction is carried out to eliminate the majority of external interference. The method is shown in formula (1). The natural orthogonal component model, based on the observation data of 36 geomagnetic stations in the Chinese Mainland, is used to correct the daily variation correction results in 2018, 2019, and 2020 to the same day, so as to eliminate the long-term variation of the geomagnetic field [<xref ref-type="bibr" rid="B27">27</xref>][<xref ref-type="bibr" rid="B28">28</xref>]. The correction error of daily variation is related to the distance between the measuring point and the reference station [<xref ref-type="bibr" rid="B23">23</xref>][<xref ref-type="bibr" rid="B29">29</xref>]. The distance between the Lhasa geomagnetic station and the two measuring points is about 350 km. Using the data from the Lhasa geomagnetic station for daily variation correction may result in an error of 1 - 2 nT. To eliminate this error, the difference between the daily variation correction results of the two measurement points was calculated, which also eliminated the main magnetic field and obtained the difference <italic>dF</italic> of the lithospheric magnetic field at the two measurement points. </p>
      <disp-formula id="FD1">
        <label>(1)</label>
        <mml:math display="inline">
          <mml:mrow>
            <mml:msub>
              <mml:mi>F</mml:mi>
              <mml:mrow>
                <mml:mi>o</mml:mi>
                <mml:mi>b</mml:mi>
                <mml:mi>s</mml:mi>
              </mml:mrow>
            </mml:msub>
            <mml:mrow>
              <mml:mo>(</mml:mo>
              <mml:mrow>
                <mml:mi>t</mml:mi>
                <mml:mn>0</mml:mn>
              </mml:mrow>
              <mml:mo>)</mml:mo>
            </mml:mrow>
            <mml:mo>=</mml:mo>
            <mml:msub>
              <mml:mi>F</mml:mi>
              <mml:mrow>
                <mml:mi>o</mml:mi>
                <mml:mi>b</mml:mi>
                <mml:mi>s</mml:mi>
              </mml:mrow>
            </mml:msub>
            <mml:mrow>
              <mml:mo>(</mml:mo>
              <mml:mi>t</mml:mi>
              <mml:mo>)</mml:mo>
            </mml:mrow>
            <mml:mo>−</mml:mo>
            <mml:mrow>
              <mml:mo>(</mml:mo>
              <mml:mrow>
                <mml:msub>
                  <mml:mi>F</mml:mi>
                  <mml:mrow>
                    <mml:mi>r</mml:mi>
                    <mml:mi>e</mml:mi>
                    <mml:mi>f</mml:mi>
                  </mml:mrow>
                </mml:msub>
                <mml:mrow>
                  <mml:mo>(</mml:mo>
                  <mml:mi>t</mml:mi>
                  <mml:mo>)</mml:mo>
                </mml:mrow>
                <mml:mo>−</mml:mo>
                <mml:msub>
                  <mml:mi>F</mml:mi>
                  <mml:mrow>
                    <mml:mi>r</mml:mi>
                    <mml:mi>e</mml:mi>
                    <mml:mi>f</mml:mi>
                  </mml:mrow>
                </mml:msub>
                <mml:mrow>
                  <mml:mo>(</mml:mo>
                  <mml:mrow>
                    <mml:mi>t</mml:mi>
                    <mml:mn>0</mml:mn>
                  </mml:mrow>
                  <mml:mo>)</mml:mo>
                </mml:mrow>
              </mml:mrow>
              <mml:mo>)</mml:mo>
            </mml:mrow>
          </mml:mrow>
        </mml:math>
      </disp-formula>
      <p>In the formula, <italic>F</italic><italic><sub>obs</sub></italic>(<italic>t</italic>0) is the daily variation correction result of the measured value at the measuring point; <italic>F</italic><italic><sub>obs</sub></italic>(<italic>t</italic>) is the measurement value at measuring point <italic>t</italic> at time <italic>t</italic>; <italic>F</italic><italic><sub>ref</sub></italic>(t) is the observed value at time <italic>t</italic> at the reference station; <italic>F</italic><italic><sub>ref</sub></italic>(<italic>t</italic>0) is the measurement value at zero point corrected for the daily variation of the reference station. The daily change correction for each period is from 00:00 to 03:00 Beijing time on a certain day. </p>
      <disp-formula id="FD2">
        <label>(2)</label>
        <mml:math display="inline">
          <mml:mrow>
            <mml:mi>d</mml:mi>
            <mml:mi>F</mml:mi>
            <mml:mo>=</mml:mo>
            <mml:msub>
              <mml:mi>F</mml:mi>
              <mml:mrow>
                <mml:mi>S</mml:mi>
                <mml:mn>1</mml:mn>
              </mml:mrow>
            </mml:msub>
            <mml:mo>−</mml:mo>
            <mml:msub>
              <mml:mi>F</mml:mi>
              <mml:mrow>
                <mml:mi>S</mml:mi>
                <mml:mn>2</mml:mn>
              </mml:mrow>
            </mml:msub>
          </mml:mrow>
        </mml:math>
      </disp-formula>
      <p>In the formula, <italic>dF</italic> represents the difference in the lithospheric magnetic field between measurement points S1 and S2, while <italic>F</italic><italic><sub>S1</sub></italic> and <italic>F</italic><italic><sub>S2</sub></italic> represent the correction results of the observed changes at observation points S1 and S2, respectively. </p>
      <p>The main sources of data result errors are instrument installation and long-term variation correction. The data fitting accuracy of the natural orthogonal component model is better than 1 nT [<xref ref-type="bibr" rid="B17">17</xref>], and the instrument installation error is better than 0.3 nT. Therefore, it can be considered that the data result error is better than 1 nT. </p>
    </sec>
    <sec id="sec3">
      <title>3. Results</title>
      <sec id="sec3dot1">
        <title>3.1. Lithospheric Magnetic Field and Changes</title>
        <p>Based on the previous method, <italic>dF</italic> values from 2018 to 2020 were obtained, and the results are shown in <bold>Table 1</bold>. The difference in the lithospheric magnetic field between the two measurement points is about −120 nT, indicating the presence of significant magnetic anomalies between the two measurement points. Considering that the horizontal and vertical gradients of the two measuring points are relatively small, this anomaly cannot be a local anomaly of the measuring points, but more likely reflects the characteristics of the regional lithospheric magnetic field. </p>
        <p>The changes in the magnetic field of the lithosphere from 2018 to 2020 were -2.2 nT in 2018-2019 and +3.9 nT in 2019-2020. The crustal compression or tension strain generated by tectonic loading in the Qinghai-Xizang Plateau region is usually around 10<sup>−</sup><sup>8</sup>, which can only produce magnetic field changes of 10<sup>−</sup><sup>1</sup> nT [<xref ref-type="bibr" rid="B30">30</xref>]. In the absence of severe crustal material migration, such as earthquakes and volcanic eruptions, it is generally believed that the changes in the magnetic field of the lithosphere do not change with time [<xref ref-type="bibr" rid="B28">28</xref>]. From 2018 to 2020, there was a change of about 6 nT in the lithospheric magnetic field, indicating that there may have been significant changes in crustal material during this period. At the same time, the reverse changes in the lithospheric magnetic field from 2018 to 2019 and from 2019 to 2020 indicate that the lithospheric magnetic field at the two measurement points experienced different effects in 2018, 2019, and 2020, thus exhibiting significant reversal changes. </p>
        <p><bold>Table 1.</bold> The<italic>dF</italic> values from 2018 to 2020.</p>
        <table-wrap id="tbl1">
          <label>Table 1</label>
          <table>
            <tbody>
              <tr>
                <td>Observed Time</td>
                <td>2018</td>
                <td>2019</td>
                <td>2020</td>
              </tr>
              <tr>
                <td>
                  <italic>dF</italic>
                  /nT
                </td>
                <td>−118.7</td>
                <td>−120.9</td>
                <td>−117.0</td>
              </tr>
            </tbody>
          </table>
        </table-wrap>
      </sec>
      <sec id="sec3dot2">
        <title>3.2. Coseismic Piezomagnetic Effect</title>
        <p>The seismic coseismic process is accompanied by significant stress release, which can lead to abnormal changes in the geomagnetic field, known as the piezomagnetic effect. The calculation methods for the piezomagnetic effect are divided into analytical methods and numerical calculation methods [<xref ref-type="bibr" rid="B31">31</xref>]. The analytical method has a small computational cost and is not prone to distortion, but it can only use uniform medium parameters. Although numerical calculation methods can consider three-dimensional medium parameters, their computational complexity is enormous and distortion may occur at fault planes. Considering the difficulty in obtaining accurate medium parameters, this section uses analytical methods to calculate the piezomagnetic field that may be generated by the Dingri earthquake. The parameters mainly include magnetization intensity (<italic>J</italic>), stress sensitivity coefficient (<italic>β</italic>), medium shear modulus (<italic>G</italic>), and sliding distribution (<italic>S</italic>) [<xref ref-type="bibr" rid="B31">31</xref>]. The values of <italic>β</italic> and <italic>J</italic> vary with factors such as lithology and burial depth [<xref ref-type="bibr" rid="B23">23</xref>], and precise determination is challenging [<xref ref-type="bibr" rid="B19">19</xref>]. Due to the linear relationship between the calculated piezomagnetic field and the product of magnetization and stress sensitivity coefficient (<italic>β J</italic>) [<xref ref-type="bibr" rid="B19">19</xref>], both <italic>β</italic> and <italic>J</italic> can be selected as 1 × 10<sup>−</sup><sup>9</sup>Pa and 1 A/m to calculate the initial piezomagnetic field. When <italic>β J</italic> changes, the final result is the initial piezomagnetic field multiplied by the corresponding multiple of <italic>β J</italic>. The shear modulus of crustal media has an impact on the calculated piezomagnetic field [<xref ref-type="bibr" rid="B32">32</xref>], especially the mechanical properties of the shallow crust have a significant influence on the calculated piezomagnetic field [<xref ref-type="bibr" rid="B31">31</xref>]. Considering that the Dingri earthquake occurs in the crust with low wave velocity, corresponding to a P-wave velocity of about 5 km/s, the shear modulus of the crust is selected as 22 GPa. The magnetic declination and tilt angle refer to the results of IGRF14 [<xref ref-type="bibr" rid="B33">33</xref>], which are +0.3˚ (positive values indicate north northeast) and 45.2˚, respectively.</p>
        <p>After the Dingri earthquake, different research institutions provided the slip distribution of coseismic faults based on seismic wave data. The rupture surface is roughly 50 to 80 km, and the rupture is mainly distributed north of the epicenter. However, the slip distribution given by different results varies greatly. Based on the preliminary results of the field survey, the surface dislocation in some areas is more than 3 m, and there is a possibility of a greater surface fault. Therefore, this paper selects a slip distribution model that is more consistent with the surface survey for calculation (from the Institute of Qinghai-Xizang Plateau Research, Chinese Academy of Sciences [<xref ref-type="bibr" rid="B34">34</xref>], see <xref ref-type="fig" rid="fig2">Figure 2</xref>). </p>
        <p>The calculation results of the coseismic piezomagnetic field show (see <xref ref-type="fig" rid="fig3">Figure 3</xref>) that a significant piezomagnetic field appears at the upper edge and both ends of the sliding surface, with a maximum piezomagnetic field exceeding 1 nT, reflecting the controlling effect of shallow stress changes on the piezomagnetic field. The majority of the area along the sliding surface has a negative piezomagnetic field, with only a small range of positive values appearing on the north side. This is because the sliding amount is mainly distributed in the area north of the sliding surface. The piezomagnetic field at the epicenter is about +0.2 nT, and the piezomagnetic fields at the two measuring points are +0.04 nT and −0.04 nT, respectively, indicating that the piezomagnetic field decays rapidly with distance. Due to the relatively small values of <italic>β</italic> and <italic>J</italic> used in this article, most studies have used <italic>β</italic> and <italic>J</italic> that are 1.5 to 3 times higher than in this article [<xref ref-type="bibr" rid="B13">13</xref>], that is, <italic>β J</italic> is 3 to 10 times higher than in this article, and some studies have used larger dielectric magnetic parameters. When choosing <italic>β J</italic> to be 3 to 10 times that of this article, the piezomagnetic field at the epicenter can reach 0.5 to 2 nT, but the piezomagnetic field at the two measuring points is still relatively small, possibly 0.1 to 0.3 nT, which is difficult to observe by instruments.</p>
        <fig id="fig2">
          <label>Figure 2</label>
          <graphic xlink:href="https://html.scirp.org/file/2802696-rId18.jpeg?20260616051044" />
        </fig>
        <p><bold>Figure 2.</bold>Coseismic slip model of Dingri M6.8 earthquake.</p>
        <fig id="fig3">
          <label>Figure 3</label>
          <graphic xlink:href="https://html.scirp.org/file/2802696-rId19.jpeg?20260616051044" />
        </fig>
        <p><bold>Figure 3.</bold> Coseismic piezomagnetic fields expected from Dingri M6.8 earthquake.</p>
      </sec>
      <sec id="sec3dot3">
        <title>3.3. Coseismic Electrokinetic Effect</title>
        <p>Another magnetic field effect related to earthquakes is the electrokinetic effect, which can generate a flowing electric potential when liquid flows through a discontinuous underground interface, thereby producing a magnetic field [<xref ref-type="bibr" rid="B35">35</xref>][<xref ref-type="bibr" rid="B36">36</xref>]. This article is based on the analytical method of the electrokinetic effect generated by dislocation sources given in reference [<xref ref-type="bibr" rid="B36">36</xref>] to calculate the changes in the coseismic magnetic field of the Dingri earthquake. The model parameters include the length of the fracture surface (<italic>l</italic>), the burial depth at the top of the fracture surface (<italic>a</italic>), the burial depth at the bottom of the fracture surface (<italic>b</italic>), the conductivity on both sides of the fracture surface (<italic>σ</italic><sub>1</sub> and <italic>σ</italic><sub>2</sub>), and the flow potential (<italic>S</italic>). According to the research results of electrical structure, there are high conductors and high resistance bodies in the crust of the Qinghai-Xizang Plateau and its surrounding areas, and violent earthquakes often occur at the junction of high conductors and high resistance bodies. Therefore, we choose <italic>σ</italic><sub>1</sub> and <italic>σ</italic><sub>2</sub> as 0.1 S/m and 0.01 S/m here. The flow potential generated by earthquake action is 0.1 to 10 V [<xref ref-type="bibr" rid="B35">35</xref>][<xref ref-type="bibr" rid="B37">37</xref>], and 1 V is selected in this paper. Based on the above parameters and the coseismic sliding distribution shown in <xref ref-type="fig" rid="fig2">Figure 2</xref> (<italic>l</italic> is 54 km; <italic>a</italic> is 0 km; <italic>b</italic> is 25.3 km), the possible coseismic electromagnetic effects of the Dingri earthquake were calculated, as shown in <xref ref-type="fig" rid="fig4">Figure 4</xref>. Unlike the piezomagnetic effect, the range of magnetic field changes in the electrokinetic effect generated by the Dingri earthquake is relatively large. Magnetic fields greater than 0.1 nT are distributed along the rupture surface for about 300 km and perpendicular to the rupture surface for about 200 km. The electrokinetic effect magnetic field at the epicenter is +0.5 nT, and the magnetic fields at the two measuring points are +0.15 nT and −0.1 nT, respectively. The magnetic field changes at both ends of the rupture surface exceed 4 nT.</p>
        <fig id="fig4">
          <label>Figure 4</label>
          <graphic xlink:href="https://html.scirp.org/file/2802696-rId20.jpeg?20260616051044" />
        </fig>
        <p><bold>Figure 4.</bold> Coseismic electrokinetic fields expected from Dingri M6.8 earthquake.</p>
        <p>The electrokinetic effect is not related to the sliding amount, but is closely related to the size of the sliding surface. The sliding distribution length used in this section is nearly 52 km, while some other models provide larger sliding surface sizes. The geothermal resources in southern Xizang are abundant, and there are hot water explosions, boiling springs, and other resources around the Dingri earthquake [<xref ref-type="bibr" rid="B38">38</xref>][<xref ref-type="bibr" rid="B39">39</xref>], which may cause an increase in electrical conductivity [<xref ref-type="bibr" rid="B40">40</xref>]. During the post-earthquake investigation, a large number of sand blasting and water emitting phenomena were found, indicating that the source of the electrokinetic effect is not limited to the sliding surface. From this, it can be inferred that the variation range of the electrokinetic effect magnetic field is larger, which is sufficient to generate the magnetic field changes observed by the instrument. In particular, the S2 measuring point is located in the high gradient zone of the magnetic field. </p>
      </sec>
    </sec>
    <sec id="sec4">
      <title>4. Discussions</title>
      <sec id="sec4dot1">
        <title>4.1. Lithosphere Magnetic Field Anomalies</title>
        <p>Some researchers have analyzed the relationship between the lithospheric magnetic field and earthquakes and structures based on geomagnetic anomaly grid data (EMAG). Earthquakes usually occur in areas where the lithospheric magnetic field is weakly negative or at the junction of positive and negative anomalies [<xref ref-type="bibr" rid="B11">11</xref>][<xref ref-type="bibr" rid="B13">13</xref>][<xref ref-type="bibr" rid="B41">41</xref>], and important active faults are also located in the transition zone between positive and negative anomalies of the lithospheric magnetic field [<xref ref-type="bibr" rid="B12">12</xref>][<xref ref-type="bibr" rid="B42">42</xref>]. Based on EMAG, the difference in lithospheric magnetic field between the two measurement points is about +18 nT, indicating that the lithospheric magnetic field at the two measurement points is basically the same. However, there is a significant difference from the measured results (about −120 nT). This difference may be due to that EMAG model incorporates no ground-based data and limited aeromagnetic data in the Qinghai-Xizang Plateau region, relying primarily on satellite magnetic measurements that only reflect long-wavelength (&gt;400 km) components of the lithospheric magnetic field. Furthermore, as satellite magnetic surveys are conducted at altitudes exceeding 300 km above the Earth’s surface, the lithospheric magnetic field derived from the EMAG model in the Qinghai-Xizang Plateau area is essentially an inverted result, which leads to significant deviations from actual ground observations. This article only used data from two measurement points, so it is unclear whether the two measurement points are located in the negative anomaly zone and the positive anomaly zone, respectively. Based on the EMAG, it is speculated that the range of differences in the lithospheric magnetic field in this area is relatively small and should belong to local magnetic anomalies.</p>
        <p>The lithospheric magnetic field contains rich information on tectonic evolution, crustal structure, and seismogenic background [<xref ref-type="bibr" rid="B43">43</xref>]. The composition of the lithospheric material in the Dingri area is relatively complex, including the High Himalayan crystalline complex, the North Ao Formation greenschist to amphibolite metamorphic complex, and the Southern Xizang Tethys sedimentary rocks. The boundaries of different lithologies are a series of normal faults [<xref ref-type="bibr" rid="B44">44</xref>][<xref ref-type="bibr" rid="B45">45</xref>]. The S1 measurement point is located in the Tethys sedimentary rock area, while the epicenter and S2 measurement points are located in the high-grade metamorphic rock area of the High Himalaya, exposing ferromagnesian granulite [<xref ref-type="bibr" rid="B45">45</xref>]. Therefore, the magnetic susceptibility of the medium on the west side of the epicenter should be lower than that on the east side. Based on this, a simple crustal magnetic susceptibility model was established to calculate the possible lithospheric magnetic field (<xref ref-type="fig" rid="fig5">Figure 5</xref>). The side with high magnetic susceptibility has a larger magnetic field, while the side with low magnetic susceptibility has a smaller magnetic field, which is consistent with the measured results and confirms the difference in rock properties on both sides of the epicenter.</p>
        <fig id="fig5">
          <label>Figure 5</label>
          <graphic xlink:href="https://html.scirp.org/file/2802696-rId21.jpeg?20260616051045" />
        </fig>
        <p><bold>Figure 5.</bold>Forward simulation of the magnetic field resulted from magnetic substances. cm is the susceptibility of the medium. Red, green, blue, and black lines are the magnetic anomaly 2 km, 1 km, 0.5 km, and 0 km above ground, respectively.</p>
        <p>The Dengmocuo fault, which gave birth to the Dingri 6.8 magnitude earthquake, is a relatively small normal fault in the Southern Xizang Rift system. It is located on the southern edge of the Xainza-Dingye fault zone and is one of the more active faults in the region [<xref ref-type="bibr" rid="B6">6</xref>][<xref ref-type="bibr" rid="B46">46</xref>]. Many studies have shown that the normal faults within the Southern Xizang Rift system are regulated by the weak middle crust and serve as important channels for the exposure of lower crustal materials to the surface [<xref ref-type="bibr" rid="B2">2</xref>][<xref ref-type="bibr" rid="B44">44</xref>]. The high Himalayan metamorphic rocks that appear locally in the Dengmocuo fault indicate that the fault displaced Tethys sedimentary rocks and became a channel for high Himalayan metamorphic rocks to fold back into the upper crust [<xref ref-type="bibr" rid="B45">45</xref>]. The low-velocity layer of the middle crust is widely distributed below the Dengmocuo fault, which may correspond to high-temperature partial melting or water-bearing fluids. The low-velocity body on the west side of the fault is more widely distributed [<xref ref-type="bibr" rid="B47">47</xref>], resulting in negative magnetic anomalies on the west side of the fault, causing the magnetic field of the lithosphere on the west side to be smaller than that on the east side.</p>
      </sec>
      <sec id="sec4dot2">
        <title>4.2. Seismic Geomagnetic Anomalies</title>
        <p>Research based on repeated observation data of the geomagnetic field shows that earthquakes often occur in areas with weak annual variations in the lithospheric magnetic field [<xref ref-type="bibr" rid="B22">22</xref>][<xref ref-type="bibr" rid="B41">41</xref>] or in areas where the annual variations of the lithospheric magnetic field have been continuously changing for many years [<xref ref-type="bibr" rid="B48">48</xref>][<xref ref-type="bibr" rid="B49">49</xref>]. This article is based on the repeated observation data of the geomagnetic field from 2018 to 2020. It was found that there was a significant turning point in the lithospheric magnetic field before the 6.8 magnitude earthquake, with an amplitude of about 6 nT. Is this an anomaly before the earthquake? A 5.9 magnitude earthquake occurred on March 20, 2020, with the epicenter located about 15 km northwest of the Dingri earthquake. Is the abnormal change in the lithospheric magnetic field discovered in this study related to the 2020 Dingri 5.9 magnitude earthquake? </p>
        <p>From the quantitative calculation of the coseismic piezomagnetic effect and electrokinetic effect in the previous text, it can be seen that the piezomagnetic effect is mainly related to stress changes and the magnetic properties of the medium. Even with larger magnetic parameters, medium strong earthquakes such as the Dingri earthquake are difficult to generate geomagnetic field changes exceeding 1 nT at a distance of 20 km from the force source [<xref ref-type="bibr" rid="B50">50</xref>]. Therefore, pre-earthquake structural loading or micro-rupture stress disturbances are more difficult to produce significant geomagnetic field changes [<xref ref-type="bibr" rid="B48">48</xref>], which is different from some studies that suggest that pre-earthquake geomagnetic field anomalies may be related to stress changes [<xref ref-type="bibr" rid="B49">49</xref>].</p>
        <p>The electrokinetic effect is mainly related to the distribution range of fluids, and fluid anomalies related to earthquakes usually have a wide distribution range. Fluid anomalies may exist within a range of several times the length of the fault rupture from the epicenter before and during the same earthquake [<xref ref-type="bibr" rid="B51">51</xref>], such as sustained water level anomalies and abnormal geomagnetic fields around the epicenter [<xref ref-type="bibr" rid="B52">52</xref>][<xref ref-type="bibr" rid="B53">53</xref>]. Based on previous analysis, the electrokinetic effect may generate geomagnetic anomalies exceeding 1 nT, and the range is large. Therefore, the geomagnetic field anomaly before the earthquake may be related to the electrokinetic effect generated by underground fluid anomalies. The Dingri earthquake is more than 5 years away from the anomaly of the lithospheric magnetic field from 2018 to 2020. Statistical results on fluid and magnetic anomalies indicate that the pre-earthquake anomaly for a 6.8 magnitude earthquake can occur from several hours to several months, even 1 year [<xref ref-type="bibr" rid="B9">9</xref>][<xref ref-type="bibr" rid="B51">51</xref>][<xref ref-type="bibr" rid="B54">54</xref>], and the possibility of anomalies occurring 5 years or even longer before the earthquake is unlikely. Therefore, it is inferred that the anomaly of the lithospheric magnetic field from 2018 to 2020 should not be related to the Dingri earthquake, but is more likely to be related to the 5.9 magnitude Dingri earthquake in 2020. The distance between two geomagnetic measurement points for the 5.9 magnitude earthquake in Dingri is about 35 km, while statistical analysis results indicate that the possible pre-earthquake anomaly range for the 5.9 magnitude earthquake in Dingri is about 200 km [<xref ref-type="bibr" rid="B55">55</xref>]. </p>
        <p>Based on the quantitative calculations in the previous text, it can be seen that significant magnetic field anomalies occur near faults and decay rapidly with distance. Although fluid and geomagnetic field anomalies before earthquakes may also occur in locations farther away from faults, the vast majority of anomalies occur in locations closer to faults. Therefore, setting up geomagnetic monitoring points near important faults makes it easier to observe magnetic field anomalies. At present, the geomagnetic repeated observation network is basically spatially uniformly distributed [<xref ref-type="bibr" rid="B56">56</xref>], which is advantageous for conducting research on the spatial distribution of the geomagnetic field and can observe some far-field anomalies, but it is not easy to observe more obvious near-fault anomalies. </p>
        <p>Besides, temperature variations associated with seismic activity can also alter the geomagnetic field through thermomagnetic effects, where rock magnetism decreases with rising temperature and increases with cooling. According to Okubo <italic>et al</italic><italic>.</italic> (2006) [<xref ref-type="bibr" rid="B57">57</xref>], temperature changes of several tens of degrees are required to generate significant magnetic variations (&gt;1 nT), yet the magnitude of stress-induced thermal response is merely 1 mK/MPa [<xref ref-type="bibr" rid="B58">58</xref>], rendering the magnetic field changes caused by stress-derived temperature variations negligible. Whether other heat sources (e.g., heat transfer from subsurface fluid migration) could contribute to geomagnetic alterations remains unclear; future studies should incorporate regional thermal infrared anomalies, ground temperature data, and hydrological records to enable quantitative analysis.</p>
      </sec>
    </sec>
    <sec id="sec5">
      <title>5. Conclusions</title>
      <p>This article uses geomagnetic field observation data obtained from 2018 to 2020 on both sides of the epicenter of the Dingri earthquake to analyze local lithospheric magnetic field anomalies. Based on the piezomagnetic effect and electrokinetic effects, the possible magnetic field anomalies caused by the Dingri earthquake were quantitatively calculated. The main conclusions are as follows:</p>
      <p>There is a difference of about −120 nT in the magnetic field of the lithosphere on the west and east sides of the epicenter of the Dingri earthquake, reflecting the different properties of the magnetic media on the east and west sides. The annual variation of the lithospheric magnetic field showed a significant turning point from −2.2 nT to +4 nT from 2018 to 2020, which may be a precursor anomaly before the earthquake. This anomaly should be related to the 5.9 magnitude earthquake in 2020. </p>
      <p>(2) The magnitude and distribution range of the coseismic piezomagnetic field are relatively small, and even if the medium has strong magnetism, the magnetic field anomaly generated at the measuring point is only 0.3 nT. The magnitude and range of the electrokinetic effect are relatively large, with a maximum magnetic field of 4 nT at both ends of the fault and 0.5 nT at the epicenter. Considering the uncertainty of the sliding distribution, this effect may produce significant magnetic anomalies at the measuring point.</p>
    </sec>
    <sec id="sec6">
      <title>Acknowledgements</title>
      <p>We thank the anonymous reviewers for their valuable comments and suggestions. The study was supported by Hebei Earthquake Science and Technology Spark Program Project (Grant No. DZ2024112200008).</p>
    </sec>
  </body>
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              <string-name>Yang, X.</string-name>
              <string-name>Lin, W.</string-name>
              <string-name>Tadai, O.</string-name>
              <string-name>Zeng, X.</string-name>
              <string-name>Yu, C.</string-name>
              <string-name>Yeh, E.</string-name>
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            <year>2017</year>
            <article-title>Experimental and Numerical Investigation of the Temperature Response to Stress Changes of Rocks</article-title>
            <source>Journal of Geophysical Research: Solid Earth</source>
            <volume>122</volume>
            <pub-id pub-id-type="doi">10.1002/2016jb013645</pub-id>
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