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    <title>DSpace Collection: 01.03.04. Structure and dynamics</title>
    <link>http://hdl.handle.net/2122/107</link>
    <description />
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      <link>http://www.earth-prints.org/simple-search</link>
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    <item>
      <title>A Revised Forest Fire Model Non-Quasistatically Driven for the Sporadic Activity of the Earth’s Magnetotail</title>
      <link>http://hdl.handle.net/2122/4072</link>
      <description>Title: A Revised Forest Fire Model Non-Quasistatically Driven for the Sporadic Activity of the Earth’s Magnetotail
&lt;br/&gt;
&lt;br/&gt;Authors: De Michelis, P.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia; Consolini, G.; Istituto di Fisica dello Spazio Interplanetario, CNR, Via Fosso del Cavaliere 100, 00133 Roma, Italy
&lt;br/&gt;
&lt;br/&gt;Editors: Sawaya-Lacoste, H.; ESA Publications Division
&lt;br/&gt;
&lt;br/&gt;Abstract: The energy release during magnetospheric substorms in response to solar wind changes consists of two main physical processes: the directly-driven and the unloading processes. Recent analysis on the sporadic activity&#xD;
related to the unloading process seems to indicate that the magnetospheric response to solar wind changes might resemble the behaviour of an out-of-equilibrium system near a marginally stable point (critical point). Here, we present a modified version of the well-known forest-fire cellular automaton (FFM) not quasistatically driven for the sporadic activity of the energy release in the geotail regions as revealed by the auroral electrojet index.</description>
      <pubDate>Tue, 29 Jan 2002 22:58:59 GMT</pubDate>
    </item>
    <item>
      <title>On the Earth’s magnetospheric dynamics: Nonequilibrium evolution and the fluctuation theorem</title>
      <link>http://hdl.handle.net/2122/4026</link>
      <description>Title: On the Earth’s magnetospheric dynamics: Nonequilibrium evolution and the fluctuation theorem
&lt;br/&gt;
&lt;br/&gt;Authors: Consolini, G.; Istituto di Fisica dello Spazio Interplanetario, INAF, Rome, Italy; De Michelis, P.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia; Tozzi, R.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia
&lt;br/&gt;
&lt;br/&gt;Abstract: The Earth’s magnetosphere evolves as an out-of-equilibrium system due to the&#xD;
continuous coupling with the solar wind and the Earth’s ionosphere. We test the validity of the symmetries implied in the Fluctuation Theorem for the magnetospheric dynamics by&#xD;
investigating the long-term evolution of the Earth’s magnetospheric ring current, as&#xD;
monitored by the geomagnetic Dst index. We find that the symmetries implied by the&#xD;
Fluctuation Theorem are all verified, thus providing a proof of the existence of a steady state far from equilibrium for the Earth’s magnetosphere. A possible link between the Dst index and the entropy production rate is also proposed and discussed.</description>
      <pubDate>Wed, 20 Aug 2008 22:58:59 GMT</pubDate>
    </item>
    <item>
      <title>Fractal time statistics of AE-index burst waiting times: evidence of metastability</title>
      <link>http://hdl.handle.net/2122/4023</link>
      <description>Title: Fractal time statistics of AE-index burst waiting times: evidence of metastability
&lt;br/&gt;
&lt;br/&gt;Authors: Consolini, G.; Istituto di Fisica dello Spazio Interplanetario – CNR, Roma, Italy; De Michelis, P.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia
&lt;br/&gt;
&lt;br/&gt;Abstract: Recent observations and analyses evidenced that the magnetotail, as well as the magnetospheric dynamics are characterised by a scale-free behaviour and intermittence.&#xD;
These results, along with numerical simulations on cellular automata, suggest that the observed scale-invariance may&#xD;
be due to forced and/or self-organised criticality (FSOC), meaning that the magnetotail operates near a marginally stable&#xD;
state (Chang, 1999). On the other hand, it was underlined that a complex magnetic field topology in the geotail regions may play a relevant role in the impulsive energy relaxation (Consolini and Chang, 2001).</description>
      <pubDate>Mon, 29 Oct 2001 22:58:59 GMT</pubDate>
    </item>
    <item>
      <title>A revised forest-fire cellular automaton for the nonlinear dynamics of the Earth’s magnetotail</title>
      <link>http://hdl.handle.net/2122/4022</link>
      <description>Title: A revised forest-fire cellular automaton for the nonlinear dynamics of the Earth’s magnetotail
&lt;br/&gt;
&lt;br/&gt;Authors: Consolini, G.; Istituto di Fisica dello Spazio Interplanetario, Consiglio Nazionale delle Ricerche-CNR, Via Fosso del Cavaliere 100, 00133 Roma, Italy; De Michelis, P.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia
&lt;br/&gt;
&lt;br/&gt;Abstract: Recent observations and numerical simulations seem to suggest that the Earth’s magnetotail plasma could exist in a near-criticality configuration, and that many features of the magnetospheric response to solar wind changes could be described by avalanche models displaying self-organized criticality. Further evidences of this near-criticality dynamics have been found analyzing the statistical features of the auroral electrojet (AE) index. Here, we present a cellular automaton, based on a revised version of the well-known forest-fire model, for the nonlinear dynamics of the Earth’s magnetotail. This simple model, chaotically driven using a 1-d coupled map, is able to capture many of the statistical features of the magnetospheric response to solar wind changes. The results, compared with previous analyses of the AE-index features, are discussed in the framework of a near-criticality dynamics of the magnetospheric tail plasma.</description>
      <pubDate>Wed, 29 Aug 2001 22:58:59 GMT</pubDate>
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