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	<id>http://wiki.fusenet.eu/fusionwiki/index.php?action=history&amp;feed=atom&amp;title=Intermittence</id>
	<title>Intermittence - Revision history</title>
	<link rel="self" type="application/atom+xml" href="http://wiki.fusenet.eu/fusionwiki/index.php?action=history&amp;feed=atom&amp;title=Intermittence"/>
	<link rel="alternate" type="text/html" href="http://wiki.fusenet.eu/fusionwiki/index.php?title=Intermittence&amp;action=history"/>
	<updated>2026-05-09T07:41:09Z</updated>
	<subtitle>Revision history for this page on the wiki</subtitle>
	<generator>MediaWiki 1.43.3</generator>
	<entry>
		<id>http://wiki.fusenet.eu/fusionwiki/index.php?title=Intermittence&amp;diff=7798&amp;oldid=prev</id>
		<title>Admin at 11:07, 21 April 2024</title>
		<link rel="alternate" type="text/html" href="http://wiki.fusenet.eu/fusionwiki/index.php?title=Intermittence&amp;diff=7798&amp;oldid=prev"/>
		<updated>2024-04-21T11:07:32Z</updated>

		<summary type="html">&lt;p&gt;&lt;/p&gt;
&lt;table style=&quot;background-color: #fff; color: #202122;&quot; data-mw=&quot;interface&quot;&gt;
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				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;Revision as of 13:07, 21 April 2024&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l3&quot;&gt;Line 3:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 3:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;The degree of intermittence can be quantified using various methods.&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;The degree of intermittence can be quantified using various methods.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;One traditional approach is through the Kurtosis of the signal &amp;lt;ref&amp;gt;Batchelor G K 1953 The Theory of Homogeneous Turbulence (Cambridge: Cambridge&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;One traditional approach is through the &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;[[:wikipedia:&lt;/ins&gt;Kurtosis&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;|Kurtosis]] &lt;/ins&gt;of the signal &amp;lt;ref&amp;gt;Batchelor G K 1953 The Theory of Homogeneous Turbulence (Cambridge: Cambridge&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;University Press), p. 183&amp;lt;/ref&amp;gt;.&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;University Press), p. 183&amp;lt;/ref&amp;gt;.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;However, the Kurtosis is a quantifier of the shape of the distribution function, and does not really take the time-varying nature of intermittence into account.&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;However, the Kurtosis is a quantifier of the shape of the distribution function, and does not really take the time-varying nature of intermittence into account.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Admin</name></author>
	</entry>
	<entry>
		<id>http://wiki.fusenet.eu/fusionwiki/index.php?title=Intermittence&amp;diff=7797&amp;oldid=prev</id>
		<title>Admin at 10:55, 21 April 2024</title>
		<link rel="alternate" type="text/html" href="http://wiki.fusenet.eu/fusionwiki/index.php?title=Intermittence&amp;diff=7797&amp;oldid=prev"/>
		<updated>2024-04-21T10:55:55Z</updated>

		<summary type="html">&lt;p&gt;&lt;/p&gt;
&lt;table style=&quot;background-color: #fff; color: #202122;&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
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				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;Revision as of 12:55, 21 April 2024&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l9&quot;&gt;Line 9:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 9:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;A better quantifier is provided by a method from the field of Chaos theory, based on a box counting technique &amp;lt;ref&amp;gt;Carreras B A et al 2000 Intermittency of plasma edge fluctuation data: multifractal analysis, [[doi:10.1063/1.874193|Phys. Plasmas &amp;#039;&amp;#039;&amp;#039;7&amp;#039;&amp;#039;&amp;#039; 3278]]&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;B. van Milligen and R. Sánchez. Analysis of Turbulence in Fusion Plasmas. IOP Series in Plasma Physics. IOP Publishing, 2022. {{ISBN|978-0-7503-4854-6}}&amp;lt;/ref&amp;gt;.&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;A better quantifier is provided by a method from the field of Chaos theory, based on a box counting technique &amp;lt;ref&amp;gt;Carreras B A et al 2000 Intermittency of plasma edge fluctuation data: multifractal analysis, [[doi:10.1063/1.874193|Phys. Plasmas &amp;#039;&amp;#039;&amp;#039;7&amp;#039;&amp;#039;&amp;#039; 3278]]&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;B. van Milligen and R. Sánchez. Analysis of Turbulence in Fusion Plasmas. IOP Series in Plasma Physics. IOP Publishing, 2022. {{ISBN|978-0-7503-4854-6}}&amp;lt;/ref&amp;gt;.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;It has been shown that the intermittence can be fruitfully exploited in the framework of fusion plasma physics: namely, it is found to decrease at locations where a single (helical, MHD) mode dominates, thus allowing to study the relation between turbulence and helical modes, and it was found to be affected by plasma flows (such as zonal flows) &amp;lt;ref&amp;gt;B. Carreras, L. García, J. Nicolau, B. van Milligen, U. Hoefel, M. Hirsch, and the TJ-II and W7-X Teams. Intermittence and turbulence in fusion devices. [[doi:10.1088/1361-6587/ab57f9|Plasma Phys. Control. Fusion, 62:025011, 2020]]&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;B. P. van Milligen, B. Carreras, L. &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;Garc ́ıa&lt;/del&gt;, and C. Hidalgo. The localization of low order rational surfaces based on the intermittence parameter in the TJ-II stellarator. [[doi:10.1088/1741-4326/ab79cc|Nucl. Fusion, 60:056010, 2020]]&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;B. van Milligen, A. Melnikov, B. Carreras, L. Garcia, A. Kozachek, C. Hidalgo, J. de Pablos, P. Khabanov, L. Eliseev, M. Drabinskij, A. Chmyga, L. Krupnik, the HIBP Team, and the TJ-II Team. Topology of 2-d turbulent structures based on intermittence in the TJ-II stellarator. [[doi:10.1088/1741-4326/ac27c9|Nucl. Fusion, 61(11):116063, 2021]]&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;B. van Milligen, B. Carreras, I. Voldiner, U. Losada, C. Hidalgo, and the TJ-II Team. Causality, intermittence and crossphase evolution during confinement transitions in the TJ-II stellarator. [[doi:10.1063/5.0057791|Phys. Plasmas, 28:092302, 2021]]&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;B. van Milligen, I. Voldiner, B. Carreras, L. García, M. Ochando, and the TJ-II Team. Rational surfaces, flows and radial structure in the TJ-II stellarator. [[doi:10.1088/1741-4326/aca688|Nucl. Fusion, 63:016027, 2023]]&amp;lt;/ref&amp;gt;.&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;It has been shown that the intermittence can be fruitfully exploited in the framework of fusion plasma physics: namely, it is found to decrease at locations where a single (helical, MHD) mode dominates, thus allowing to study the relation between turbulence and helical modes, and it was found to be affected by plasma flows (such as zonal flows) &amp;lt;ref&amp;gt;B. Carreras, L. García, J. Nicolau, B. van Milligen, U. Hoefel, M. Hirsch, and the TJ-II and W7-X Teams. Intermittence and turbulence in fusion devices. [[doi:10.1088/1361-6587/ab57f9|Plasma Phys. Control. Fusion, 62:025011, 2020]]&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;B. P. van Milligen, B. Carreras, L. &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;García&lt;/ins&gt;, and C. Hidalgo. The localization of low order rational surfaces based on the intermittence parameter in the TJ-II stellarator. [[doi:10.1088/1741-4326/ab79cc|Nucl. Fusion, 60:056010, 2020]]&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;B. van Milligen, A. Melnikov, B. Carreras, L. Garcia, A. Kozachek, C. Hidalgo, J. de Pablos, P. Khabanov, L. Eliseev, M. Drabinskij, A. Chmyga, L. Krupnik, the HIBP Team, and the TJ-II Team. Topology of 2-d turbulent structures based on intermittence in the TJ-II stellarator. [[doi:10.1088/1741-4326/ac27c9|Nucl. Fusion, 61(11):116063, 2021]]&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;B. van Milligen, B. Carreras, I. Voldiner, U. Losada, C. Hidalgo, and the TJ-II Team. Causality, intermittence and crossphase evolution during confinement transitions in the TJ-II stellarator. [[doi:10.1063/5.0057791|Phys. Plasmas, 28:092302, 2021]]&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;B. van Milligen, I. Voldiner, B. Carreras, L. García, M. Ochando, and the TJ-II Team. Rational surfaces, flows and radial structure in the TJ-II stellarator. [[doi:10.1088/1741-4326/aca688|Nucl. Fusion, 63:016027, 2023]]&amp;lt;/ref&amp;gt;.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;== References ==&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;== References ==&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&amp;lt;references /&amp;gt;&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&amp;lt;references /&amp;gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Admin</name></author>
	</entry>
	<entry>
		<id>http://wiki.fusenet.eu/fusionwiki/index.php?title=Intermittence&amp;diff=7796&amp;oldid=prev</id>
		<title>Admin at 10:55, 21 April 2024</title>
		<link rel="alternate" type="text/html" href="http://wiki.fusenet.eu/fusionwiki/index.php?title=Intermittence&amp;diff=7796&amp;oldid=prev"/>
		<updated>2024-04-21T10:55:21Z</updated>

		<summary type="html">&lt;p&gt;&lt;/p&gt;
&lt;table style=&quot;background-color: #fff; color: #202122;&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
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				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;Revision as of 12:55, 21 April 2024&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l9&quot;&gt;Line 9:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 9:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;A better quantifier is provided by a method from the field of Chaos theory, based on a box counting technique &amp;lt;ref&amp;gt;Carreras B A et al 2000 Intermittency of plasma edge fluctuation data: multifractal analysis, [[doi:10.1063/1.874193|Phys. Plasmas &amp;#039;&amp;#039;&amp;#039;7&amp;#039;&amp;#039;&amp;#039; 3278]]&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;B. van Milligen and R. Sánchez. Analysis of Turbulence in Fusion Plasmas. IOP Series in Plasma Physics. IOP Publishing, 2022. {{ISBN|978-0-7503-4854-6}}&amp;lt;/ref&amp;gt;.&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;A better quantifier is provided by a method from the field of Chaos theory, based on a box counting technique &amp;lt;ref&amp;gt;Carreras B A et al 2000 Intermittency of plasma edge fluctuation data: multifractal analysis, [[doi:10.1063/1.874193|Phys. Plasmas &amp;#039;&amp;#039;&amp;#039;7&amp;#039;&amp;#039;&amp;#039; 3278]]&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;B. van Milligen and R. Sánchez. Analysis of Turbulence in Fusion Plasmas. IOP Series in Plasma Physics. IOP Publishing, 2022. {{ISBN|978-0-7503-4854-6}}&amp;lt;/ref&amp;gt;.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;It has been shown that the intermittence can be fruitfully exploited in the framework of fusion plasma physics: namely, it is found to decrease at locations where a single (helical, MHD) mode dominates, thus allowing to study the relation between turbulence and helical modes, and it was found to be affected by plasma flows (such as zonal flows) &amp;lt;ref&amp;gt;B. Carreras, L. García, J. Nicolau, B. van Milligen, U. Hoefel, M. Hirsch, and the TJ-II and W7-X Teams. Intermittence and turbulence in fusion devices. [[doi:10.1088/1361-6587/ab57f9|Plasma Phys. Control. Fusion, 62:025011, 2020]]&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;B. P. van Milligen, B. Carreras, L. Garc ́ıa, and C. Hidalgo. The localization of low order rational surfaces based on the intermittence parameter in the TJ-II stellarator. [[doi:10.1088/1741-4326/ab79cc|Nucl. Fusion, 60:056010, 2020]]&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;B. van Milligen, A. Melnikov, B. Carreras, L. Garcia, A. Kozachek, C. Hidalgo, J. de Pablos, P. Khabanov, L. Eliseev, M. Drabinskij, A. Chmyga, L. Krupnik, the HIBP Team, and the TJ-II Team. Topology of 2-d turbulent structures based on intermittence in the TJ-II stellarator. [[doi:10.1088/1741-4326/ac27c9|Nucl. Fusion, 61(11):116063, 2021]]&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;B. van Milligen, B. Carreras, I. Voldiner, U. Losada, C. Hidalgo, and the TJ-II Team. Causality, &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;inter- mittence &lt;/del&gt;and crossphase evolution during confinement transitions in the TJ-II stellarator. [[doi:10.1063/5.0057791|Phys. Plasmas, 28:092302, 2021]]&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;B. van Milligen, I. Voldiner, B. Carreras, L. García, M. Ochando, and the TJ-II Team. Rational surfaces, flows and radial structure in the TJ-II stellarator. [[doi:10.1088/1741-4326/aca688|Nucl. Fusion, 63:016027, 2023]]&amp;lt;/ref&amp;gt;.&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;It has been shown that the intermittence can be fruitfully exploited in the framework of fusion plasma physics: namely, it is found to decrease at locations where a single (helical, MHD) mode dominates, thus allowing to study the relation between turbulence and helical modes, and it was found to be affected by plasma flows (such as zonal flows) &amp;lt;ref&amp;gt;B. Carreras, L. García, J. Nicolau, B. van Milligen, U. Hoefel, M. Hirsch, and the TJ-II and W7-X Teams. Intermittence and turbulence in fusion devices. [[doi:10.1088/1361-6587/ab57f9|Plasma Phys. Control. Fusion, 62:025011, 2020]]&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;B. P. van Milligen, B. Carreras, L. Garc ́ıa, and C. Hidalgo. The localization of low order rational surfaces based on the intermittence parameter in the TJ-II stellarator. [[doi:10.1088/1741-4326/ab79cc|Nucl. Fusion, 60:056010, 2020]]&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;B. van Milligen, A. Melnikov, B. Carreras, L. Garcia, A. Kozachek, C. Hidalgo, J. de Pablos, P. Khabanov, L. Eliseev, M. Drabinskij, A. Chmyga, L. Krupnik, the HIBP Team, and the TJ-II Team. Topology of 2-d turbulent structures based on intermittence in the TJ-II stellarator. [[doi:10.1088/1741-4326/ac27c9|Nucl. Fusion, 61(11):116063, 2021]]&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;B. van Milligen, B. Carreras, I. Voldiner, U. Losada, C. Hidalgo, and the TJ-II Team. Causality, &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;intermittence &lt;/ins&gt;and crossphase evolution during confinement transitions in the TJ-II stellarator. [[doi:10.1063/5.0057791|Phys. Plasmas, 28:092302, 2021]]&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;B. van Milligen, I. Voldiner, B. Carreras, L. García, M. Ochando, and the TJ-II Team. Rational surfaces, flows and radial structure in the TJ-II stellarator. [[doi:10.1088/1741-4326/aca688|Nucl. Fusion, 63:016027, 2023]]&amp;lt;/ref&amp;gt;.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;== References ==&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;== References ==&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&amp;lt;references /&amp;gt;&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&amp;lt;references /&amp;gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Admin</name></author>
	</entry>
	<entry>
		<id>http://wiki.fusenet.eu/fusionwiki/index.php?title=Intermittence&amp;diff=7795&amp;oldid=prev</id>
		<title>Admin at 10:54, 21 April 2024</title>
		<link rel="alternate" type="text/html" href="http://wiki.fusenet.eu/fusionwiki/index.php?title=Intermittence&amp;diff=7795&amp;oldid=prev"/>
		<updated>2024-04-21T10:54:16Z</updated>

		<summary type="html">&lt;p&gt;&lt;/p&gt;
&lt;table style=&quot;background-color: #fff; color: #202122;&quot; data-mw=&quot;interface&quot;&gt;
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				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;Revision as of 12:54, 21 April 2024&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l7&quot;&gt;Line 7:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 7:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;However, the Kurtosis is a quantifier of the shape of the distribution function, and does not really take the time-varying nature of intermittence into account.&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;However, the Kurtosis is a quantifier of the shape of the distribution function, and does not really take the time-varying nature of intermittence into account.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;A better quantifier is provided by a method from the field of Chaos theory, based on a box counting technique &amp;lt;ref&amp;gt;Carreras B A et al 2000 Intermittency of plasma edge fluctuation data: multifractal analysis, [[&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;coi&lt;/del&gt;:10.1063/1.874193|Phys. Plasmas &#039;&#039;&#039;7&#039;&#039;&#039; 3278]]&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;B. van Milligen and R. Sánchez. Analysis of Turbulence in Fusion Plasmas. IOP Series in Plasma Physics. IOP Publishing, 2022. {{ISBN|978-0-7503-4854-6}}&amp;lt;/ref&amp;gt;.&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;A better quantifier is provided by a method from the field of Chaos theory, based on a box counting technique &amp;lt;ref&amp;gt;Carreras B A et al 2000 Intermittency of plasma edge fluctuation data: multifractal analysis, [[&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;doi&lt;/ins&gt;:10.1063/1.874193|Phys. Plasmas &#039;&#039;&#039;7&#039;&#039;&#039; 3278]]&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;B. van Milligen and R. Sánchez. Analysis of Turbulence in Fusion Plasmas. IOP Series in Plasma Physics. IOP Publishing, 2022. {{ISBN|978-0-7503-4854-6}}&amp;lt;/ref&amp;gt;.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;It has been shown that the intermittence can be fruitfully exploited in the framework of fusion plasma physics: namely, it is found to decrease at locations where a single (helical, MHD) mode dominates, thus allowing to study the relation between turbulence and helical modes, and it was found to be affected by plasma flows (such as zonal flows) &amp;lt;ref&amp;gt;B. Carreras, L. García, J. Nicolau, B. van Milligen, U. Hoefel, M. Hirsch, and the TJ-II and W7-X Teams. Intermittence and turbulence in fusion devices. [[doi:10.1088/1361-6587/ab57f9|Plasma Phys. Control. Fusion, 62:025011, 2020]]&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;B. P. van Milligen, B. Carreras, L. Garc ́ıa, and C. Hidalgo. The localization of low order rational surfaces based on the intermittence parameter in the TJ-II stellarator. [[doi:10.1088/1741-4326/ab79cc|Nucl. Fusion, 60:056010, 2020]]&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;B. van Milligen, A. Melnikov, B. Carreras, L. Garcia, A. Kozachek, C. Hidalgo, J. de Pablos, P. Khabanov, L. Eliseev, M. Drabinskij, A. Chmyga, L. Krupnik, the HIBP Team, and the TJ-II Team. Topology of 2-d turbulent structures based on intermittence in the TJ-II stellarator. [[doi:10.1088/1741-4326/ac27c9|Nucl. Fusion, 61(11):116063, 2021]]&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;B. van Milligen, B. Carreras, I. Voldiner, U. Losada, C. Hidalgo, and the TJ-II Team. Causality, inter- mittence and crossphase evolution during confinement transitions in the TJ-II stellarator. [[doi:10.1063/5.0057791|Phys. Plasmas, 28:092302, 2021]]&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;B. van Milligen, I. Voldiner, B. Carreras, L. García, M. Ochando, and the TJ-II Team. Rational surfaces, flows and radial structure in the TJ-II stellarator. [[doi:10.1088/1741-4326/aca688|Nucl. Fusion, 63:016027, 2023]]&amp;lt;/ref&amp;gt;.&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;It has been shown that the intermittence can be fruitfully exploited in the framework of fusion plasma physics: namely, it is found to decrease at locations where a single (helical, MHD) mode dominates, thus allowing to study the relation between turbulence and helical modes, and it was found to be affected by plasma flows (such as zonal flows) &amp;lt;ref&amp;gt;B. Carreras, L. García, J. Nicolau, B. van Milligen, U. Hoefel, M. Hirsch, and the TJ-II and W7-X Teams. Intermittence and turbulence in fusion devices. [[doi:10.1088/1361-6587/ab57f9|Plasma Phys. Control. Fusion, 62:025011, 2020]]&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;B. P. van Milligen, B. Carreras, L. Garc ́ıa, and C. Hidalgo. The localization of low order rational surfaces based on the intermittence parameter in the TJ-II stellarator. [[doi:10.1088/1741-4326/ab79cc|Nucl. Fusion, 60:056010, 2020]]&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;B. van Milligen, A. Melnikov, B. Carreras, L. Garcia, A. Kozachek, C. Hidalgo, J. de Pablos, P. Khabanov, L. Eliseev, M. Drabinskij, A. Chmyga, L. Krupnik, the HIBP Team, and the TJ-II Team. Topology of 2-d turbulent structures based on intermittence in the TJ-II stellarator. [[doi:10.1088/1741-4326/ac27c9|Nucl. Fusion, 61(11):116063, 2021]]&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;B. van Milligen, B. Carreras, I. Voldiner, U. Losada, C. Hidalgo, and the TJ-II Team. Causality, inter- mittence and crossphase evolution during confinement transitions in the TJ-II stellarator. [[doi:10.1063/5.0057791|Phys. Plasmas, 28:092302, 2021]]&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;B. van Milligen, I. Voldiner, B. Carreras, L. García, M. Ochando, and the TJ-II Team. Rational surfaces, flows and radial structure in the TJ-II stellarator. [[doi:10.1088/1741-4326/aca688|Nucl. Fusion, 63:016027, 2023]]&amp;lt;/ref&amp;gt;.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Admin</name></author>
	</entry>
	<entry>
		<id>http://wiki.fusenet.eu/fusionwiki/index.php?title=Intermittence&amp;diff=7794&amp;oldid=prev</id>
		<title>Admin: Created page with &quot;A signal is called intermittent when at irregularly spaced intervals, its standard deviation increases sharply. The time intervals with larger standard deviation are sometimes called &#039;bursts&#039;.  The degree of intermittence can be quantified using various methods. One traditional approach is through the Kurtosis of the signal &lt;ref&gt;Batchelor G K 1953 The Theory of Homogeneous Turbulence (Cambridge: Cambridge University Press), p. 183&lt;/ref&gt;. However, the Kurtosis is a quanti...&quot;</title>
		<link rel="alternate" type="text/html" href="http://wiki.fusenet.eu/fusionwiki/index.php?title=Intermittence&amp;diff=7794&amp;oldid=prev"/>
		<updated>2024-04-21T10:53:08Z</updated>

		<summary type="html">&lt;p&gt;Created page with &amp;quot;A signal is called intermittent when at irregularly spaced intervals, its standard deviation increases sharply. The time intervals with larger standard deviation are sometimes called &amp;#039;bursts&amp;#039;.  The degree of intermittence can be quantified using various methods. One traditional approach is through the Kurtosis of the signal &amp;lt;ref&amp;gt;Batchelor G K 1953 The Theory of Homogeneous Turbulence (Cambridge: Cambridge University Press), p. 183&amp;lt;/ref&amp;gt;. However, the Kurtosis is a quanti...&amp;quot;&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;A signal is called intermittent when at irregularly spaced intervals, its standard deviation increases sharply.&lt;br /&gt;
The time intervals with larger standard deviation are sometimes called &amp;#039;bursts&amp;#039;.&lt;br /&gt;
&lt;br /&gt;
The degree of intermittence can be quantified using various methods.&lt;br /&gt;
One traditional approach is through the Kurtosis of the signal &amp;lt;ref&amp;gt;Batchelor G K 1953 The Theory of Homogeneous Turbulence (Cambridge: Cambridge&lt;br /&gt;
University Press), p. 183&amp;lt;/ref&amp;gt;.&lt;br /&gt;
However, the Kurtosis is a quantifier of the shape of the distribution function, and does not really take the time-varying nature of intermittence into account.&lt;br /&gt;
&lt;br /&gt;
A better quantifier is provided by a method from the field of Chaos theory, based on a box counting technique &amp;lt;ref&amp;gt;Carreras B A et al 2000 Intermittency of plasma edge fluctuation data: multifractal analysis, [[coi:10.1063/1.874193|Phys. Plasmas &amp;#039;&amp;#039;&amp;#039;7&amp;#039;&amp;#039;&amp;#039; 3278]]&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;B. van Milligen and R. Sánchez. Analysis of Turbulence in Fusion Plasmas. IOP Series in Plasma Physics. IOP Publishing, 2022. {{ISBN|978-0-7503-4854-6}}&amp;lt;/ref&amp;gt;.&lt;br /&gt;
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It has been shown that the intermittence can be fruitfully exploited in the framework of fusion plasma physics: namely, it is found to decrease at locations where a single (helical, MHD) mode dominates, thus allowing to study the relation between turbulence and helical modes, and it was found to be affected by plasma flows (such as zonal flows) &amp;lt;ref&amp;gt;B. Carreras, L. García, J. Nicolau, B. van Milligen, U. Hoefel, M. Hirsch, and the TJ-II and W7-X Teams. Intermittence and turbulence in fusion devices. [[doi:10.1088/1361-6587/ab57f9|Plasma Phys. Control. Fusion, 62:025011, 2020]]&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;B. P. van Milligen, B. Carreras, L. Garc ́ıa, and C. Hidalgo. The localization of low order rational surfaces based on the intermittence parameter in the TJ-II stellarator. [[doi:10.1088/1741-4326/ab79cc|Nucl. Fusion, 60:056010, 2020]]&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;B. van Milligen, A. Melnikov, B. Carreras, L. Garcia, A. Kozachek, C. Hidalgo, J. de Pablos, P. Khabanov, L. Eliseev, M. Drabinskij, A. Chmyga, L. Krupnik, the HIBP Team, and the TJ-II Team. Topology of 2-d turbulent structures based on intermittence in the TJ-II stellarator. [[doi:10.1088/1741-4326/ac27c9|Nucl. Fusion, 61(11):116063, 2021]]&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;B. van Milligen, B. Carreras, I. Voldiner, U. Losada, C. Hidalgo, and the TJ-II Team. Causality, inter- mittence and crossphase evolution during confinement transitions in the TJ-II stellarator. [[doi:10.1063/5.0057791|Phys. Plasmas, 28:092302, 2021]]&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;B. van Milligen, I. Voldiner, B. Carreras, L. García, M. Ochando, and the TJ-II Team. Rational surfaces, flows and radial structure in the TJ-II stellarator. [[doi:10.1088/1741-4326/aca688|Nucl. Fusion, 63:016027, 2023]]&amp;lt;/ref&amp;gt;.&lt;br /&gt;
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== References ==&lt;br /&gt;
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&amp;lt;references /&amp;gt;&lt;/div&gt;</summary>
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