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<front>
<journal-meta>
<journal-id journal-id-type="publisher-id">Front. Earth Sci.</journal-id>
<journal-title>Frontiers in Earth Science</journal-title>
<abbrev-journal-title abbrev-type="pubmed">Front. Earth Sci.</abbrev-journal-title>
<issn pub-type="epub">2296-6463</issn>
<publisher>
<publisher-name>Frontiers Media S.A.</publisher-name>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="publisher-id">881425</article-id>
<article-id pub-id-type="doi">10.3389/feart.2022.881425</article-id>
<article-categories>
<subj-group subj-group-type="heading">
<subject>Earth Science</subject>
<subj-group>
<subject>Brief Research Report</subject>
</subj-group>
</subj-group>
</article-categories>
<title-group>
<article-title>Earthquake Productivity Law in a Wide Magnitude Range</article-title>
<alt-title alt-title-type="left-running-head">Shebalin et al.</alt-title>
<alt-title alt-title-type="right-running-head">Earthquake Productivity in a Wide Magnitude Range</alt-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname>Shebalin</surname>
<given-names>Peter</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<uri xlink:href="https://loop.frontiersin.org/people/867981/overview"/>
</contrib>
<contrib contrib-type="author" corresp="yes">
<name>
<surname>Baranov</surname>
<given-names>Sergey</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
<xref ref-type="corresp" rid="c001">&#x2a;</xref>
<uri xlink:href="https://loop.frontiersin.org/people/1565181/overview"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Vorobieva</surname>
<given-names>Inessa</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<uri xlink:href="https://loop.frontiersin.org/people/1573275/overview"/>
</contrib>
</contrib-group>
<aff id="aff1">
<sup>1</sup>
<institution>Institute of Earthquake Prediction Theory and Mathematical Geophysics</institution>, <institution>Russian Academy of Sciences</institution>, <addr-line>Moscow</addr-line>, <country>Russia</country>
</aff>
<aff id="aff2">
<sup>2</sup>
<institution>Geophysical Survey</institution>, <institution>Kola Branch</institution>, <institution>Russian Academy of Sciences</institution>, <addr-line>Apatity</addr-line>, <country>Russia</country>
</aff>
<author-notes>
<fn fn-type="edited-by">
<p>
<bold>Edited by:</bold> <ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/1021898/overview">Claudia Piromallo</ext-link>, Istituto Nazionale di Geofisica e Vulcanologia (INGV), Italy</p>
</fn>
<fn fn-type="edited-by">
<p>
<bold>Reviewed by:</bold> <ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/988593/overview">Cataldo Godano</ext-link>, University of Campania Luigi Vanvitelli, Italy</p>
<p>
<ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/176925/overview">Angelo De Santis</ext-link>, Istituto Nazionale di Geofisica e Vulcanologia (INGV), Italy</p>
</fn>
<corresp id="c001">&#x2a;Correspondence: Sergey Baranov, <email>bars.vl@gmail.com</email>
</corresp>
<fn fn-type="other">
<p>This article was submitted to Solid Earth Geophysics, a section of the journal Frontiers in Earth Science</p>
</fn>
</author-notes>
<pub-date pub-type="epub">
<day>04</day>
<month>05</month>
<year>2022</year>
</pub-date>
<pub-date pub-type="collection">
<year>2022</year>
</pub-date>
<volume>10</volume>
<elocation-id>881425</elocation-id>
<history>
<date date-type="received">
<day>22</day>
<month>02</month>
<year>2022</year>
</date>
<date date-type="accepted">
<day>19</day>
<month>04</month>
<year>2022</year>
</date>
</history>
<permissions>
<copyright-statement>Copyright &#xa9; 2022 Shebalin, Baranov and Vorobieva.</copyright-statement>
<copyright-year>2022</copyright-year>
<copyright-holder>Shebalin, Baranov and Vorobieva</copyright-holder>
<license xlink:href="http://creativecommons.org/licenses/by/4.0/">
<p>This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) and the copyright owner(s) are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms.</p>
</license>
</permissions>
<abstract>
<p>Earthquakes are usually followed by aftershocks. The number of aftershocks&#x2014;the so-called productivity&#x2014;depends on the magnitude of the earthquake. In seismic modeling it is usually assumed that the number of aftershocks is approximately the same for earthquakes with the same magnitude. This is one of the key assumptions on which the calculations are based. Although it is known that in reality this number can vary widely, only recently a pattern of such changes, called the earthquake productivity law, has been established. If we consider only direct aftershocks in a fixed magnitude range relative to the magnitude of the main shocks, then their number for a set of earthquakes in some spatiotemporal volume has an exponential distribution form. This means that fewer aftershocks are more likely. The most likely outcome is the complete absence of aftershocks. This pattern is quite counterintuitive, especially when considering aftershocks over a wide range of magnitudes. Here we managed to confirm the fulfillment of the earthquake productivity law for the wide range of magnitudes. For earthquakes of magnitude 6 and higher in the land part of Japan, it is confirmed that the frequency distribution of the number of their direct aftershocks with a minimum magnitude of 5 units less has an exponential shape. In seismicity modeling the validated earthquake productivity law makes it possible to replace the incorrect assumption of constant earthquake productivity with an exponential distribution. The single parameter of this regularity is easily determined from the actual data.</p>
</abstract>
<kwd-group>
<kwd>models of seismicity</kwd>
<kwd>seismic hazard assessment</kwd>
<kwd>aftershocks</kwd>
<kwd>earthquake productivity</kwd>
<kwd>statistical seismology</kwd>
<kwd>earthquake interaction</kwd>
<kwd>earthquake catalog declustering</kwd>
</kwd-group>
<contract-sponsor id="cn001">Russian Science Foundation<named-content content-type="fundref-id">10.13039/501100006769</named-content>
</contract-sponsor>
</article-meta>
</front>
<body>
<sec id="s1">
<title>1 Introduction</title>
<p>It has recently been found that the number of aftershocks of large earthquakes in the world and the number of direct aftershocks of earthquakes in different regions of the world, considered in a fixed magnitude range relative to the main shock, obeys an exponential distribution (<xref ref-type="bibr" rid="B8">Shebalin et al., 2020a</xref>; <xref ref-type="bibr" rid="B9">Shebalin et al., 2020b</xref>). This law, called earthquake productivity law, was established for different magnitudes of the main shocks, different ways of identifying direct aftershocks, in a wide range of parameters of the algorithm for identifying aftershocks (<xref ref-type="bibr" rid="B9">Shebalin et al., 2020b</xref>). The data used made it possible to consider ranges of aftershock magnitudes with a lower threshold within the range of up to 2.5 units of magnitude less than the magnitude of the main shock. A further increase in the range in the reviewed catalogs was impossible, since the entire range of considered magnitudes should be above the general completeness threshold. Therefore, an increase in the range is possible only by increasing the magnitude threshold for the main shocks, which leads to their number being too small.</p>
<p>The exponential shape of the distribution means that the most probable number of direct aftershocks (the mode of the distribution) is 0. This property of earthquake productivity seems so counterintuitive that testing whether this shape of the distribution persists as the range of aftershock magnitudes increases has an important independent meaning. The importance of this verification is also reinforced by the fact that the exponential form of productivity contradicts one of the key elements of the ETAS stochastic model (<xref ref-type="bibr" rid="B7">Ogata, 1998</xref>) widely used for modeling seismicity. It is assumed in ETAS model that the productivity of earthquakes is a function of their magnitude. Under this assumption, productivity should have the form of a Poisson distribution with a non-zero mode. The same assumption is used in stochastic methods for declustering earthquake catalogs, in particular, the method based on the ETAS model (<xref ref-type="bibr" rid="B13">Zhuang et al., 2002</xref>) and in the model-independent MISD method (<xref ref-type="bibr" rid="B6">Marsan and Lengline, 2008</xref>).</p>
<p>The aim of this work is to investigate whether the exponential form of the distribution of earthquake productivity will be preserved with a significant expansion of the range of aftershock magnitudes. This can only be done in a region with a dense network of seismic stations and, at the same time, a high frequency of large earthquakes. We chose the land part of Japan, where the representative magnitude for crustal earthquakes since 2000 is about 1.0, and earthquakes of magnitude 6 and above occur several times a year.</p>
</sec>
<sec id="s2">
<title>2 Methods</title>
<p>We follow the definition of earthquake productivity adopted by <xref ref-type="bibr" rid="B9">Shebalin et al. (2020b)</xref>. In the earthquake flow, each event is considered as a potential &#x201c;parent&#x201d; of subsequent earthquakes, and vice versa, each event can have a &#x201c;parent&#x201d;, in which case it is considered an &#x201c;offspring&#x201d;. The offsprings can be interpreted as immediate aftershocks. We use the nearest neighbor scheme by <xref ref-type="bibr" rid="B12">Zaliapin and Ben-Zion (2013)</xref>. In this scheme, each parent (triggering event) can have multiple offsprings (triggered events), but each offspring can only have one parent. The parent of a given event is determined by the minimum of the proximity function (&#x201c;nearest neighbor&#x201d;). The proximity function determines the extent to which &#x201c;parent&#x201d; and &#x201c;offspring&#x201d; can be considered related. In this paper, following <xref ref-type="bibr" rid="B12">Zaliapin and Ben-Zion (2013)</xref>, we use the proximity function proposed by <xref ref-type="bibr" rid="B1">Baiesi and Paczuski (2004)</xref>:<disp-formula id="e1">
<mml:math id="m1">
<mml:msub>
<mml:mrow>
<mml:mi>&#x3b7;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>i</mml:mi>
<mml:mi>j</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mo>&#x3d;</mml:mo>
<mml:mfenced open="{" close="">
<mml:mrow>
<mml:mtable class="cases">
<mml:mtr>
<mml:mtd columnalign="left">
<mml:msub>
<mml:mrow>
<mml:mi>t</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>i</mml:mi>
<mml:mi>j</mml:mi>
</mml:mrow>
</mml:msub>
<mml:msup>
<mml:mrow>
<mml:mfenced open="(" close=")">
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>r</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>i</mml:mi>
<mml:mi>j</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>d</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>f</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:msup>
<mml:mn>1</mml:mn>
<mml:msup>
<mml:mrow>
<mml:mn>0</mml:mn>
</mml:mrow>
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:mi>b</mml:mi>
<mml:msub>
<mml:mrow>
<mml:mi>m</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>i</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:msup>
<mml:mo>,</mml:mo>
<mml:mspace width="1em"/>
</mml:mtd>
<mml:mtd columnalign="left">
<mml:msub>
<mml:mrow>
<mml:mi>t</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>i</mml:mi>
<mml:mi>j</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mo>&#x3e;</mml:mo>
<mml:mn>0</mml:mn>
<mml:mo>,</mml:mo>
</mml:mtd>
</mml:mtr>
<mml:mtr>
<mml:mtd columnalign="left">
<mml:mo>&#x2b;</mml:mo>
<mml:mi>&#x221e;</mml:mi>
<mml:mo>,</mml:mo>
<mml:mspace width="1em"/>
</mml:mtd>
<mml:mtd columnalign="left">
<mml:msub>
<mml:mrow>
<mml:mi>t</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>i</mml:mi>
<mml:mi>j</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mo>&#x2264;</mml:mo>
<mml:mn>0</mml:mn>
<mml:mo>,</mml:mo>
</mml:mtd>
</mml:mtr>
</mml:mtable>
</mml:mrow>
</mml:mfenced>
</mml:math>
<label>(1)</label>
</disp-formula>where <italic>t</italic>
<sub>
<italic>ij</italic>
</sub> &#x3d; <italic>t</italic>
<sub>
<italic>j</italic>
</sub> &#x2212; <italic>t</italic>
<sub>
<italic>i</italic>
</sub> is the interevent time, <italic>r</italic>
<sub>
<italic>ij</italic>
</sub> the spatial distance between the epicenters, <italic>m</italic>
<sub>
<italic>i</italic>
</sub> the magnitude of event <italic>i</italic>, <italic>d</italic>
<sub>
<italic>f</italic>
</sub> the fractal dimension of the epicenter distribution and <italic>b</italic> the slope of the earthquake-size distribution.</p>
<p>
<xref ref-type="bibr" rid="B12">Zaliapin and Ben-Zion (2013)</xref> have shown that the distribution of the nearest neighbor proximity function usually has a bimodal distribution, in which small values correspond to related events (aftershocks, foreshocks, swarms), and large values correspond to independent events. To separate related and independent events, a threshold value for the proximity function is introduced. <xref ref-type="bibr" rid="B12">Zaliapin and Ben-Zion (2013)</xref> proposed to approximate this bimodal distribution by the sum of two log-normal distributions. However, in reality, the form of distribution can be more complex. Therefore, <xref ref-type="bibr" rid="B9">Shebalin et al. (2020b)</xref> proposed to approximate the right side of the distribution using a randomized catalog of earthquakes. We believe that the distribution of the nearest neighbor proximity function in the randomized catalog is the same as for independent events. The distribution of related events is then defined as the difference between the overall distribution and the distribution for the randomized catalog. The threshold is defined in such a way as to equalize the error rates (related events with a proximity function above the threshold and independent events with a proximity function below the threshold).</p>
<p>After introducing the threshold, it turns out that some of the events do not have a &#x201c;parent&#x201d; because the proximity to the nearest neighbor exceeds the threshold. We call such events &#x201c;background&#x201d;. If the proximity is below the threshold the event has a &#x201c;parent&#x201d;. We call such events offsprings. The productivity of an earthquake then is the number of its offsprings. Here, as in (<xref ref-type="bibr" rid="B9">Shebalin et al., 2020b</xref>), we will use &#x394;<italic>M</italic>-productivity. We count the number of offsprings of magnitude <italic>M</italic>
<sub>
<italic>a</italic>
</sub> &#x2265; <italic>M</italic>
<sub>
<italic>m</italic>
</sub> &#x2212; &#x394;<italic>M</italic>, where <italic>M</italic>
<sub>
<italic>m</italic>
</sub> is the magnitude of the parent and <italic>M</italic>
<sub>
<italic>a</italic>
</sub> is the magnitude of the offspring. Note that the magnitude of the offspring may be greater than the magnitude of the parent.</p>
<p>The scheme used here differs from the traditional mainshock-aftershock outline, which usually assumes that aftershocks are weaker than the mainshock. Another difference is that an aftershock sequence consists of a hierarchical tree of parent-offspring sequences with several levels of hierarchy (offspring of offspring, etc.). In the traditional scheme (<xref ref-type="bibr" rid="B12">Zaliapin and Ben-Zion, 2013</xref>), the total number of aftershocks is calculated. We count the number of offsprings at one level of the hierarchy, which can be interpreted as direct aftershocks. In this scheme, each earthquake is characterized by its &#x394;<italic>M</italic>-productivity value. It makes sense to analyze the values of &#x394;<italic>M</italic>-productivity for earthquakes with magnitude <italic>M</italic> &#x2265; <italic>M</italic>
<sub>
<italic>c</italic>
</sub> &#x2b; &#x394;<italic>M</italic>. In this case, the offsprings are counted above the magnitude of complete registration <italic>M</italic>
<sub>
<italic>c</italic>
</sub>.</p>
</sec>
<sec id="s3">
<title>3 Results</title>
<sec id="s3-1">
<title>3.1 Data Preparation</title>
<p>In this study we use the data of the catalog of the Japan Meteorological Agency (JMA)<xref ref-type="fn" rid="fn1">
<sup>1</sup>
</xref>. Data analysis has shown that the completeness of the catalog has improved significantly since 2000. Using the multiscale analysis of the frequency-magnitude distribution (<xref ref-type="bibr" rid="B11">Vorobieva et al., 2013</xref>), we have constructed a completeness magnitude map from earthquake data since 2000 with a hypocenter depth <italic>h</italic> &#x2264; 40&#xa0;km (<xref ref-type="fig" rid="F1">Figure 1</xref>). We associate ranges of smaller magnitudes with decreasing areas for data selection based on empirical relations in seismotectonics.</p>
<fig id="F1" position="float">
<label>FIGURE 1</label>
<caption>
<p>Map of the completeness magnitude <italic>M</italic>
<sub>
<italic>c</italic>
</sub> for the land part of Japan. The yellow line outlines the area of <italic>M</italic>
<sub>
<italic>c</italic>
</sub> &#x2264; 1. Epicenters of the earthquakes (parent events) we used in the analysis of the productivity are shown by circles (5 &#x2264; <italic>M</italic> &#x3c; 6) and stars (<italic>M</italic> &#x2265; 6). Red star shows the epicenter of the Tohoku earthquake of 11 March 2011, <italic>M</italic>
<sub>
<italic>w</italic>
</sub> &#x3d; 9.1. Tab at the top shows the frequency-magnitude distribution of earthquakes within the area of <italic>M</italic>
<sub>
<italic>c</italic>
</sub> &#x2264; 1.</p>
</caption>
<graphic xlink:href="feart-10-881425-g001.tif"/>
</fig>
<p>The map of the completeness magnitude <italic>M</italic>
<sub>
<italic>c</italic>
</sub> is constructed as follows: at each point, events are selected from the magnitude intervals [<italic>M</italic>, <italic>M</italic> &#x2b; <italic>W</italic>
<sub>
<italic>M</italic>
</sub>] in a circle with radius <italic>R</italic>(<italic>M</italic>) &#x3d; 15 &#xd7; 10<sup>
<italic>pM</italic>
</sup> km, left end of the magnitude interval varies from 0.5 to 3. The <italic>W</italic>
<sub>
<italic>M</italic>
</sub> is the length of the segment of the frequency-magnitude distribution where we check a linear shape of the distribution. The exponent <italic>p</italic> has an order of <italic>b</italic>/2, that provides at a given location near-constant sample size with change of magnitude <italic>M</italic>. The radius for data selection is constant at a given magnitude segment [<italic>M</italic>, <italic>M</italic> &#x2b; <italic>W</italic>
<sub>
<italic>M</italic>
</sub>] over the entire territory. The completeness magnitude <italic>M</italic>
<sub>
<italic>c</italic>
</sub> is defined as the minimum value of <italic>M</italic> for which the corresponding sample follows the Gutenberg-Richter law. This estimation is done simultaneously with the <italic>b</italic>-value estimation performed using the <xref ref-type="bibr" rid="B2">Bender (1983)</xref> method. The method assumes the grouping of magnitude values with a step of &#x394;<italic>m</italic>. To decide whether the sample conforms to the Gutenberg-Richter law we check the fulfillment of the relation <italic>N</italic>
<sub>0</sub> &#x2265; <italic>N</italic>
<sub>1</sub>10<sup>(<italic>b</italic>&#x2212;<italic>&#x3b4;</italic>)&#x394;<italic>m</italic>
</sup>, where <italic>b</italic> is the estimate of <italic>b</italic>-value in the interval [<italic>M</italic>, <italic>M</italic> &#x2b; <italic>W</italic>
<sub>
<italic>M</italic>
</sub>], <italic>&#x3b4;</italic> is the estimated error according to <xref ref-type="bibr" rid="B10">Shi and Bolt (1982)</xref>, <italic>N</italic>
<sub>0</sub> number of events with magnitude <italic>m</italic> &#x2265; <italic>M</italic>, and <italic>N</italic>
<sub>1</sub> number of events with magnitude <italic>m</italic> &#x2265; <italic>M</italic> &#x2b; &#x394;<italic>m</italic>.</p>
<p>High resolution of the <italic>M</italic>
<sub>
<italic>c</italic>
</sub>-value is achieved through the determination of the smallest space-magnitude scale in which the Gutenberg-Richter law is verified. The multiscale procedure isolates the magnitude range that meets the best local seismicity and local record capacity. Here we use the values of the parameters <italic>W</italic>
<sub>
<italic>M</italic>
</sub> &#x3d; 1, <italic>p</italic> &#x3d; 0.4, the minimum number of events in the sample is 100. The resulting value <italic>M</italic>
<sub>
<italic>c</italic>
</sub> is assigned to the centers of the circles located on a grid of 0.1 &#xd7; 0.1&#xb0;.</p>
<p>For further analysis, we chose the <italic>M</italic>
<sub>
<italic>c</italic>
</sub> &#x3d; 1 completeness level (yellow outline in <xref ref-type="fig" rid="F1">Figure 1</xref>). The coordinates of the nodes of this contour are given in <xref ref-type="sec" rid="s11">Supplementary Table S1</xref>. The <italic>M</italic>
<sub>
<italic>c</italic>
</sub> &#x2265; 1 region closely matches the <italic>M</italic>
<sub>
<italic>c</italic>
</sub> &#x2265; 1.7 completeness magnitude region found by the JMA for the whole period in the earthquake catalog. The <italic>M</italic>
<sub>
<italic>c</italic>
</sub> &#x2265; 1 region closely matches the <italic>M</italic>
<sub>
<italic>c</italic>
</sub> &#x2265; 1.7 completeness magnitude region declared by the JMA for the earthquakes with focal depth <italic>h</italic> &#x2264; 150 km<xref ref-type="fn" rid="fn2">
<sup>2</sup>
</xref>. The difference in <italic>M</italic>
<sub>
<italic>c</italic>
</sub> estimates is explained by the difference in focal depth of earthquakes. The level of registration is better for the most shallow seismicity <italic>h</italic> &#x2264; 40&#xa0;km, which we use in our study.</p>
</sec>
</sec>
<sec id="s4">
<title>4 Study of Earthquake Productivity in Land Part of Japan</title>
<p>For the territory under consideration, estimates were made of the values of the proximity function parameters (1): <italic>b</italic> &#x3d; 0.86, <italic>d</italic>
<sub>
<italic>f</italic>
</sub> &#x3d; 1.68 and log<sub>10</sub>
<italic>&#x3b7;</italic>
<sub>0</sub> &#x3d; &#x2212;1.46. <italic>b</italic>-value is determined by <xref ref-type="bibr" rid="B2">Bender (1983)</xref> method in magnitude interval <italic>m</italic> &#x2265; 3; <italic>d</italic>
<sub>
<italic>f</italic>
</sub> is determined by <xref ref-type="bibr" rid="B3">Grassberger (1983)</xref> method also for events of magnitude <italic>m</italic> &#x2265; 3. The <italic>&#x3b7;</italic>
<sub>0</sub> threshold was determined using the method from (<xref ref-type="bibr" rid="B9">Shebalin et al., 2020b</xref>). To avoid the possible influence of the Tohoku earthquake on 11 March 2011 with <italic>M</italic> &#x3d; 9.1, all three parameters were estimated using data for 2000&#x2013;2010.</p>
<p>For each earthquake with <italic>M</italic>
<sub>
<italic>m</italic>
</sub> &#x2265; 6.0, we calculated the productivity: the number of offsprings with magnitude <italic>M</italic>
<sub>
<italic>a</italic>
</sub> &#x2265; <italic>M</italic>
<sub>
<italic>m</italic>
</sub> &#x2212; &#x394;<italic>M</italic>, &#x394;<italic>M</italic> &#x3d; 5. It turned out that 39,464 triggered events were associated with 56 parent events. The frequency-productivity graph is shown in <xref ref-type="fig" rid="F2">Figure 2</xref>. This plot is similar to the commonly used frequency-magnitude cumulative graph, in which frequencies are summed starting at higher values. The rectilinear form of the graph, as in the case of the Gutenberg-Richter law, indicates the exponential form of the distribution. The difference is that the productivity of each earthquake is an integer, so the resulting distribution is more correctly interpreted as a geometric distribution, for which the cumulative frequency plot, starting from large values of the argument, also has a linear form on a logarithmic scale. The slope of the graph is uniquely related to a single distribution parameter.</p>
<fig id="F2" position="float">
<label>FIGURE 2</label>
<caption>
<p>Cumulative frequency-productivity graphs for parent earthquakes with <italic>M</italic>
<sub>
<italic>m</italic>
</sub> &#x2265; 6 and offspring events with <italic>M</italic>
<sub>
<italic>a</italic>
</sub> &#x2265; <italic>M</italic>
<sub>
<italic>m</italic>
</sub> &#x2212; 5.</p>
</caption>
<graphic xlink:href="feart-10-881425-g002.tif"/>
</fig>
<p>Thus, we may conclude that the exponential form of the distribution of &#x394;<italic>M</italic>-earthquake productivity established by <xref ref-type="bibr" rid="B9">Shebalin et al. (2020b)</xref> for &#x394;<italic>M</italic> &#x2264; 2.5 is also confirmed for a very large range of magnitudes for &#x394;<italic>M</italic> &#x3d; 5.</p>
<p>In the presented analysis, the earthquake productivity was not separated according to different levels of the hierarchy due to small number of <italic>M</italic>
<sub>
<italic>m</italic>
</sub> &#x2265; 6.0 events. Using worlwide stastistics of productivity, it was shown by <xref ref-type="bibr" rid="B9">Shebalin et al. (2020b)</xref> that the exponential form of the distribution and the value of its parameter change little for different levels of the hierarchy. It is this observation that gave grounds to simultaneously analyze the productivity of all earthquakes, regardless of whether they are main shocks or aftershocks in the traditional terminology. We repeated this check for earthquakes of the land part of Japan with <italic>M</italic>
<sub>
<italic>m</italic>
</sub> &#x2265; 5.0 and &#x394;<italic>M</italic> &#x3d; 4. This property is maintained: for at least eight levels of the hierarchy, starting with background events (hierarchy level 0), the frequency-productivity plots remain linear on a logarithmic scale and have approximately the same slope (<xref ref-type="fig" rid="F3">Figure 3</xref>).</p>
<fig id="F3" position="float">
<label>FIGURE 3</label>
<caption>
<p>Cumulative frequency-productivity graphs for parent earthquakes with <italic>M</italic>
<sub>
<italic>m</italic>
</sub> &#x2265; 5 and offspring events with <italic>M</italic>
<sub>
<italic>a</italic>
</sub> &#x2265; <italic>M</italic>
<sub>
<italic>m</italic>
</sub> &#x2212; 4: all earthquakes and separately for 8 highest hierarchy levels. Tab at the top shows the estimates of &#x39b;<sub>4</sub> and its standard errors calculated by bootstrap method.</p>
</caption>
<graphic xlink:href="feart-10-881425-g003.tif"/>
</fig>
<p>We verified whether the observed exponential distribution of productivity is a property of the data, or, alternatively, the result of the choice of the proximity function. We selected only background earthquakes (events of the hierarchy level 0) from the catalog and, assuming <italic>&#x3b7;</italic>
<sub>0</sub> &#x3d; <italic>&#x221e;</italic>, repeated the procedure for finding for each event its parent (the closest neighbor) and calculated the productivity. The resulting distribution of the productivity of background earthquakes has a pronounced non-zero maximum (<xref ref-type="fig" rid="F4">Figure 4</xref>) and, thus, is not geometric. Comparison of the distributions for background and clustered seismicity demonstrates completely different spatiotemporal structure. Thus, it is confirmed that the exponential form of the productivity distribution is a property of clustered seismicity.</p>
<fig id="F4" position="float">
<label>FIGURE 4</label>
<caption>
<p>Productivity distribution for background events (blue histogram) compared to productivity distribution for clustered events (red histogram).</p>
</caption>
<graphic xlink:href="feart-10-881425-g004.tif"/>
</fig>
</sec>
<sec id="s5">
<title>5 Discussion</title>
<p>The main result obtained here&#x2014;the exponential form of the distribution of the &#x394;<italic>M</italic>-productivity of earthquakes [the productivity law (<xref ref-type="bibr" rid="B9">Shebalin et al., 2020b</xref>)] is preserved even at a very large value of &#x394;<italic>M</italic>. The density of the geometric distribution&#x2014;an integer version of the exponential one&#x2014;has a maximum value at 0. This makes this form of distribution counterintuitive. It is difficult to imagine that the most probable number of direct aftershocks is 0. It is even more difficult to believe this when direct aftershocks are considered, the magnitude of which is 5 units less than the magnitude of the earthquakes that caused them. Our analysis, however, shows that this is possible, and it becomes clear why the productivity law can remain valid even for large &#x394;<italic>M</italic>. The point is that for large magnitude ranges under consideration, the total number of offsprings is orders of magnitude greater than the number of parent earthquakes. In the considered example (<xref ref-type="fig" rid="F2">Figure 2</xref>), with <italic>M</italic>
<sub>
<italic>m</italic>
</sub> &#x2265; 6 and &#x394;<sub>
<italic>M</italic>
</sub> &#x3d; 5, the productivity reaches 3,000, but the total number of parent events is only 56. Under these conditions, the probability of realizing the productivity value exactly 0 is small: <italic>p</italic> &#x3d; 0.0014, and expected number of such earthquakes is 0.08, e.g., zero, because number of earthquakes is integer. Nevertheless, the smallest productivity values still predominate. If the number of analyzed events is much greater than the average productivity, then the number of events without direct aftershocks (productivity 0) is indeed large compared to the number of events of any other productivity (see <xref ref-type="sec" rid="s11">Supplementary Material</xref>).</p>
<p>It is usually assumed that the productivity of earthquakes depends mainly on their magnitude. This, in particular, is used in the ETAS (<xref ref-type="bibr" rid="B13">Zhuang et al., 2002</xref>) and MISD (<xref ref-type="bibr" rid="B6">Marsan and Lengline, 2008</xref>) stochastic declustering methods. The expected &#x394;<italic>M</italic>-productivity distribution for such models is a Poisson distribution having a pronounced non-zero mode, this is actually predefined in these models. However, <xref ref-type="bibr" rid="B9">Shebalin et al. (2020b)</xref> showed, and here it is confirmed for large values of &#x394;<italic>M</italic>, that in reality this distribution is rather a monotone geometric one with a mode at 0. This gives additional advantages to the <xref ref-type="bibr" rid="B12">Zaliapin and Ben-Zion (2013)</xref> declustering method, which does not use any specified assumption. The spatiotemporal version of the ETAS model (<xref ref-type="bibr" rid="B7">Ogata, 1998</xref>; <xref ref-type="bibr" rid="B13">Zhuang et al., 2002</xref>) is also often used for seismicity modeling. The Poisson productivity distribution embedded in the model contradicts the observations. The earthquake productivity law confirmed here makes it possible to correct the ETAS model.</p>
<p>In a nearest neighbor schema, each parent can have multiple offsprings, but each offspring can only have one parent. This makes the productivity averaging procedure meaningful, since in such a procedure each offspring is taken into account only once. We have also shown that productivity depends little on the level of the hierarchy. This means that there is no need to distinguish between main shocks and aftershocks during averaging. &#x394;<italic>M</italic>-productivity averaged over some space-time region, we call after <xref ref-type="bibr" rid="B9">Shebalin et al. (2020b)</xref> the clustering factor. Note that in ETAS model the clustering factor is called a branching ratio. It should be less than 1 to avoid diverging aftershocks occurrence rate (<xref ref-type="bibr" rid="B5">Helmstetter and Sornette, 2002</xref>). For large &#x394;<italic>M</italic> we obtain clustering factor much larger than 1. But there is no apparent contradiction here, because the ETAS model assumes a strong relationship between the number of direct aftershocks and the main shock magnitude (<xref ref-type="bibr" rid="B4">Helmstetter, 2003</xref>), which was refuted by <xref ref-type="bibr" rid="B9">Shebalin et al. (2020b)</xref> and here again. In &#x394;<italic>M</italic>-analysis, the number of offsprings turns out to be weakly dependent on the magnitude of the parent, and its statistical distribution has exponential form with clear maximum at 0. This explains why large values of the clustering factor do not cause a diverging aftershock sequence. Of course, if we consider all offsprings with magnitudes above a certain threshold, their number increases with the magnitude of the parent. But this is controlled by Gutenberg-Richter law.</p>
<p>&#x394;<italic>M</italic>-productivity, similar manner to magnitude, can be seen as a property inherent in every earthquake. In this case, this value does not have to be an integer. Let&#x2019;s denote this value <italic>&#x3bb;</italic>. The observed value in this case is the concrete realization of the &#x201c;potential&#x201d; productivity of <italic>&#x3bb;</italic>. It can be assumed that a particular sample is a Poisson random variable with rate <italic>&#x3bb;</italic>. One more assumption can be made: the parameter <italic>&#x3bb;</italic> of earthquakes, similarly to the magnitude, has an exponential distribution of the form:<disp-formula id="e2">
<mml:math id="m2">
<mml:msub>
<mml:mrow>
<mml:mi>p</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>e</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mfenced open="(" close=")">
<mml:mrow>
<mml:mi>&#x3bb;</mml:mi>
</mml:mrow>
</mml:mfenced>
<mml:mo>&#x3d;</mml:mo>
<mml:mfrac>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi mathvariant="normal">&#x39b;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi mathvariant="normal">&#x394;</mml:mi>
<mml:mi>M</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:mfrac>
<mml:mi>exp</mml:mi>
<mml:mfenced open="(" close=")">
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:mfrac>
<mml:mrow>
<mml:mi>&#x3bb;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi mathvariant="normal">&#x39b;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi mathvariant="normal">&#x394;</mml:mi>
<mml:mi>M</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:mfrac>
</mml:mrow>
</mml:mfenced>
<mml:mo>,</mml:mo>
</mml:math>
<label>(2)</label>
</disp-formula>where &#x39b;<sub>&#x394;<italic>M</italic>
</sub> is a parameter.</p>
<p>It is easy to show (<xref ref-type="bibr" rid="B9">Shebalin et al., 2020b</xref>) that the distribution of a sample of the productivity of an arbitrary earthquake in this case has the form of a geometric distribution. The estimate of the parameter &#x39b;<sub>&#x394;<italic>M</italic>
</sub> is the average value of <italic>&#x3bb;</italic> over the ensemble. Thus, the clustering factor has the meaning of the &#x39b;<sub>&#x394;<italic>M</italic>
</sub> parameter and its estimate. The clustering factor is a convenient and a simple parameter to characterize the productivity in a set of earthquakes, for example, earthquakes in a certain space-time volume.</p>
</sec>
</body>
<back>
<sec id="s6">
<title>Data Availability Statement</title>
<p>Publicly available datasets were analyzed in this study. This data can be found here: <ext-link ext-link-type="uri" xlink:href="https://www.data.jma.go.jp/svd/eqev/data/bulletin/index_e.html">https://www.data.jma.go.jp/svd/eqev/data/bulletin/index_e.html</ext-link>.</p>
</sec>
<sec id="s7">
<title>Author Contributions</title>
<p>All authors listed have made a substantial, direct, and intellectual contribution to the work and approved it for publication.</p>
</sec>
<sec id="s8">
<title>Funding</title>
<p>The study was supported by a grant from the Russian Science Foundation (project No. 20-17-00180).</p>
</sec>
<sec sec-type="COI-statement" id="s9">
<title>Conflict of Interest</title>
<p>The authors declare that the research was conducted in the absence of any commercial or financial relationships that could be construed as a potential conflict of interest.</p>
</sec>
<sec sec-type="disclaimer" id="s10">
<title>Publisher&#x2019;s Note</title>
<p>All claims expressed in this article are solely those of the authors and do not necessarily represent those of their affiliated organizations, or those of the publisher, the editors, and the reviewers. Any product that may be evaluated in this article, or claim that may be made by its manufacturer, is not guaranteed or endorsed by the publisher.</p>
</sec>
<ack>
<p>The authors thank the Japan Meteorological Agency for providing the Seismological Bulletin of Japan.</p>
</ack>
<sec id="s11">
<title>Supplementary Material</title>
<p>The Supplementary Material for this article can be found online at: <ext-link ext-link-type="uri" xlink:href="https://www.frontiersin.org/articles/10.3389/feart.2022.881425/full#supplementary-material">https://www.frontiersin.org/articles/10.3389/feart.2022.881425/full&#x23;supplementary-material</ext-link>
</p>
<supplementary-material xlink:href="DataSheet1.PDF" id="SM1" mimetype="application/PDF" xmlns:xlink="http://www.w3.org/1999/xlink"/>
<supplementary-material xlink:href="DataSheet2.CSV" id="SM2" mimetype="application/CSV" xmlns:xlink="http://www.w3.org/1999/xlink"/>
</sec>
<fn-group>
<fn id="fn1">
<label>1</label>
<p>Japan Meteorological Agency, The Seismological Bulletin of Japan. (2022). <ext-link ext-link-type="uri" xlink:href="https://www.data.jma.go.jp/svd/eqev/data/bulletin/index_e.html">https://www.data.jma.go.jp/svd/eqev/data/bulletin/index_e.html</ext-link> (Accessed 10 January 2022).</p>
</fn>
<fn id="fn2">
<label>2</label>
<p>Japan Meteorological Agency, User&#x2019;s guide for The Seismological Bulletin of Japan. (2022) <ext-link ext-link-type="uri" xlink:href="https://www.data.jma.go.jp/svd/eqev/data/bulletin/catalog/notes_e.html">https://www.data.jma.go.jp/svd/eqev/data/bulletin/catalog/notes_e.html</ext-link> (Accessed 10 January 2022).</p>
</fn>
</fn-group>
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