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<front>
<journal-meta>
<journal-id journal-id-type="publisher">NPG</journal-id>
<journal-title-group>
<journal-title>Nonlinear Processes in Geophysics</journal-title>
<abbrev-journal-title abbrev-type="publisher">NPG</abbrev-journal-title>
<abbrev-journal-title abbrev-type="nlm-ta">Nonlin. Processes Geophys.</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">1607-7946</issn>
<publisher><publisher-name>Copernicus Publications</publisher-name>
<publisher-loc>Göttingen, Germany</publisher-loc>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="doi">10.5194/npg-12-733-2005</article-id>
<title-group>
<article-title>Avalanches in bi-directional sandpile and burning models: a comparative study</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Gedalin</surname>
<given-names>M.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Bregman</surname>
<given-names>M.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Balikhin</surname>
<given-names>M.</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>Coca</surname>
<given-names>D.</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>Consolini</surname>
<given-names>G.</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>Treumann</surname>
<given-names>R. A.</given-names>
</name>
<xref ref-type="aff" rid="aff4">
<sup>4</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Ben-Gurion University, Beer-Sheva, Israel</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>ACSE, University of Sheffield, Sheffield, UK</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>Ist. Fisica Spazio Interplanetario, Istituto Nazionale di Astrofisica, Rome, Italy</addr-line>
</aff>
<aff id="aff4">
<label>4</label>
<addr-line>Max-Planck-Institute for Extraterrestrial Physics, Garching, Germany</addr-line>
</aff>
<pub-date pub-type="epub">
<day>29</day>
<month>07</month>
<year>2005</year>
</pub-date>
<volume>12</volume>
<issue>5</issue>
<fpage>733</fpage>
<lpage>739</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2005 M. Gedalin et al.</copyright-statement>
<copyright-year>2005</copyright-year>
<license license-type="open-access">
<license-p>This work is licensed under the Creative Commons Attribution-NonCommercial-ShareAlike 2.5 Generic License. To view a copy of this licence, visit <ext-link ext-link-type="uri"  xlink:href="https://creativecommons.org/licenses/by-nc-sa/2.5/">https://creativecommons.org/licenses/by-nc-sa/2.5/</ext-link></license-p>
</license>
</permissions>
<self-uri xlink:href="https://npg.copernicus.org/articles/12/733/2005/npg-12-733-2005.html">This article is available from https://npg.copernicus.org/articles/12/733/2005/npg-12-733-2005.html</self-uri>
<self-uri xlink:href="https://npg.copernicus.org/articles/12/733/2005/npg-12-733-2005.pdf">The full text article is available as a PDF file from https://npg.copernicus.org/articles/12/733/2005/npg-12-733-2005.pdf</self-uri>
<abstract>
<p>We perform a statistical analysis of two one-dimensional avalanching models:
the bi-directional sandpile and the burning model (described in detail in the
companion paper by Gedalin et al.&amp;nbsp;(2005) &quot;Dynamics of the burning model&quot;). Such a
comparison helps understand whether very limited measurements done by a
remote observer may provide sufficient information to distinguish between the
two physically different avalanching systems. We show that the passive phase
duration reflects the avalanching nature of the system. The cluster size
analysis may provide some clues. The distribution of the active phase
durations shows a clear difference between the two models, reflecting the
dependence on the internal dynamics. Deeper insight into the active phase
duration distribution even provides information about the system parameters.</p>
</abstract>
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