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		<title>Language Mixing between C and Fortran</title>
		<link>http://eisungy.wordpress.com/2010/10/28/language-mixing-between-c-and-fortran/</link>
		<comments>http://eisungy.wordpress.com/2010/10/28/language-mixing-between-c-and-fortran/#comments</comments>
		<pubDate>Thu, 28 Oct 2010 17:52:08 +0000</pubDate>
		<dc:creator>eisungy</dc:creator>
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		<guid isPermaLink="false">http://eisungy.wordpress.com/2010/10/28/language-mixing-between-c-and-fortran/</guid>
		<description><![CDATA[I&#8217;m familiar with C, but in my field, fortran90 or higher version have been widely used. (I met Fortran77, where most irritating and annoying part is dynamic allocation which is not supported) I get accustomed to Fortran, but sometimes, I need to connect my C module to main code written by Fortran. I might describe [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=eisungy.wordpress.com&amp;blog=3164591&amp;post=84&amp;subd=eisungy&amp;ref=&amp;feed=1" width="1" height="1" />]]></description>
			<content:encoded><![CDATA[<p>I&#8217;m familiar with C, but in my field, fortran90 or higher version have been widely used. (I met Fortran77, where most irritating and annoying part is dynamic allocation which is not supported) I get accustomed to Fortran, but sometimes, I need to connect my C module to main code written by Fortran. I might describe my know-how here, but I&#8217;d better list links which would be helpful for you and my memory.</p>
<p>Following links might be very helpful.</p>
<p>http://www.math.utah.edu/software/c-with-fortran.html</p>
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		<title>Totalview in PPPL Cluster</title>
		<link>http://eisungy.wordpress.com/2010/09/29/totalview-in-pppl-cluster/</link>
		<comments>http://eisungy.wordpress.com/2010/09/29/totalview-in-pppl-cluster/#comments</comments>
		<pubDate>Wed, 29 Sep 2010 17:38:50 +0000</pubDate>
		<dc:creator>eisungy</dc:creator>
				<category><![CDATA[Tips]]></category>

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		<description><![CDATA[If you want to run Totalview for a parallel job using several nodes, you might need following: Currently, Totalview in PPPL cluster sets default accessing shell as &#8220;rsh&#8221;. So if you try to run Totalview, the program will try to use &#8220;rsh&#8221;, which is not supported in PPL cluster, and you&#8217;ll meet error message like [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=eisungy.wordpress.com&amp;blog=3164591&amp;post=80&amp;subd=eisungy&amp;ref=&amp;feed=1" width="1" height="1" />]]></description>
			<content:encoded><![CDATA[<p>If you want to run Totalview for a parallel job using several nodes, you might need following:</p>
<p>Currently, Totalview in PPPL cluster sets default accessing shell as &#8220;rsh&#8221;. So if you try to run Totalview, the program will try to use &#8220;rsh&#8221;, which is not supported in PPL cluster, and you&#8217;ll meet error message like &#8221; connection refused &#8221; with several lines showing trials of access to other nodes using rsh.<br />
To change the default value, you might need to add a following line to your &#8220;.cshrc&#8221; (Cshell) or &#8220;.bashrc&#8221;(bash) as</p>
<p>setenv TVDSVRLAUNCHCMD ssh                        (cshell)<br />
export TVDSVRLAUNCHCMD=ssh                        (bash)</p>
<p>In addition, it&#8217;ll be necessary to use interactive job(&#8220;-I&#8221; option) to run totalview. Note that you need one more option &#8220;-V&#8221; to transfer your environmental variable(esp. for DISPLAY) to allocated nodes. If not, you&#8217;ll meet X11 forwarding problem, and an error message telling environmental variable DISPLAY is not properly set. </p>
<p>After you get interactive nodes, you can run totalview(&#8220;-tv&#8221; option) with MPICH as</p>
<p>mpirun -tv -np  (# of CPUs) (executable file)</p>
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		<title>Vi (or Vim)</title>
		<link>http://eisungy.wordpress.com/2010/02/15/vi-or-vim/</link>
		<comments>http://eisungy.wordpress.com/2010/02/15/vi-or-vim/#comments</comments>
		<pubDate>Tue, 16 Feb 2010 02:56:50 +0000</pubDate>
		<dc:creator>eisungy</dc:creator>
				<category><![CDATA[Tips]]></category>

		<guid isPermaLink="false">http://eisungy.wordpress.com/?p=67</guid>
		<description><![CDATA[For word completion : (insert mode) ctrl-n / ctrl-p next/previous word completion referring to the editing file. (insert mode) ctrl-x, ctrl-l line completion For exploring directories and files : :e . For copy or delete using visual block ctrl-V, (select region using arrowkey), y copy ctrl-V, (select region using arrowkey), d delete If you don&#8217;t [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=eisungy.wordpress.com&amp;blog=3164591&amp;post=67&amp;subd=eisungy&amp;ref=&amp;feed=1" width="1" height="1" />]]></description>
			<content:encoded><![CDATA[<p>For word completion :<br />
(insert mode) <strong>ctrl-n / ctrl-p</strong>      next/previous word completion referring to the editing file.<br />
(insert mode) <strong>ctrl-x, ctrl-l</strong>         line completion</p>
<p>For exploring directories and files :<br />
<strong>:e .</strong></p>
<p>For copy or delete using visual block<br />
<strong>ctrl-V, (select region using arrowkey), y</strong> copy<br />
<strong>ctrl-V, (select region using arrowkey), d</strong> delete</p>
<p>If you don&#8217;t want to change settings every time when you use vi(or vim), the permanent setting can be done by changing( or making if it doesn&#8217;t exist in your $HOME directory) following file :<br />
<strong>.vimrc</strong></p>
<p>For coloring :<br />
<strong>syntax on</strong></p>
<p>For backspace :<br />
<strong>set backspace=2</p>
<p><a href="http://www.rayninfo.co.uk/vimtips.html">http://www.rayninfo.co.uk/vimtips.html</a><br />
<a href="http://www.yolinux.com/TUTORIALS/LinuxTutorialAdvanced_vi.html">http://www.yolinux.com/TUTORIALS/LinuxTutorialAdvanced_vi.html</a></p>
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		<title>Poincare&#8217;-Von Zeipel perturbation method</title>
		<link>http://eisungy.wordpress.com/2010/02/05/poincare-von-zeipel-perturbation-method/</link>
		<comments>http://eisungy.wordpress.com/2010/02/05/poincare-von-zeipel-perturbation-method/#comments</comments>
		<pubDate>Sat, 06 Feb 2010 02:56:09 +0000</pubDate>
		<dc:creator>eisungy</dc:creator>
				<category><![CDATA[Classical Mechanics]]></category>

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		<description><![CDATA[I need to finish this post and other posts in my weblog, but due to my laziness and other works in real life, it&#8217;s hard to update the contents. If you have any question, please contact me below e-mail address. But, I&#8217;ll try to update this subject and differential equations with symmetry in near future. [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=eisungy.wordpress.com&amp;blog=3164591&amp;post=55&amp;subd=eisungy&amp;ref=&amp;feed=1" width="1" height="1" />]]></description>
			<content:encoded><![CDATA[<p>I need to finish this post and other posts in my weblog, but due to my laziness and other works in real life, it&#8217;s hard to update the contents. If you have any question, please contact me below e-mail address. But, I&#8217;ll try to update this subject and differential equations with symmetry in near future. There are lots of funs with this subject.</p>
<p>yoones1@gmail.com</p>
<p>last modified : 28th Oct. 2010</p>
<p>&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;<br />
This article is based on a report entitled &#8220;A Pedestrian&#8217;s Guide to Lie Transforms: A New Approach to Perturbation Theory in Classical Mechanics&#8221; by Robert G. Littlejohn (1978). Before rushing  into Lie transform, understanding the method of average and Poincare&#8217;-Von Zeipel perturbation(PV) method would be helpful to understand advantage of Lie trasnform. I&#8217;m planning to update this article with more details. </p>
<p>&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;KEY</p>
<p><img src='http://s0.wp.com/latex.php?latex=F%28%5Ctheta%2CJ%27%29+%3D+%5Ctheta+%5Ccdot+J%27+%2B+%5Cepsilon+F_1+%5Ctheta%2C+J%27%29+%2B+%5Cepsilon%5E2+F_2%28%5Ctheta%2CJ%27%29%2B...&amp;bg=ffffff&amp;fg=333333&amp;s=0' alt='F(&#92;theta,J&#039;) = &#92;theta &#92;cdot J&#039; + &#92;epsilon F_1 &#92;theta, J&#039;) + &#92;epsilon^2 F_2(&#92;theta,J&#039;)+...' title='F(&#92;theta,J&#039;) = &#92;theta &#92;cdot J&#039; + &#92;epsilon F_1 &#92;theta, J&#039;) + &#92;epsilon^2 F_2(&#92;theta,J&#039;)+...' class='latex' /></p>
<p><img src='http://s0.wp.com/latex.php?latex=%5Ctheta%27+%3D+%5Ctheta+%2B+%5Cepsilon+%5Cfrac%7B%5Cpartial+F_1%7D%7B%5Cpartial+J%27%7D%28%5Ctheta%2CJ%27%29+%2B+%5Cepsilon%5E2+%5Cfrac%7B%5Cpartial+F_2%7D%7B%5Cpartial+J%27%7D%28%5Ctheta%2C+J%27%29+%2B+...&amp;bg=ffffff&amp;fg=333333&amp;s=0' alt='&#92;theta&#039; = &#92;theta + &#92;epsilon &#92;frac{&#92;partial F_1}{&#92;partial J&#039;}(&#92;theta,J&#039;) + &#92;epsilon^2 &#92;frac{&#92;partial F_2}{&#92;partial J&#039;}(&#92;theta, J&#039;) + ...' title='&#92;theta&#039; = &#92;theta + &#92;epsilon &#92;frac{&#92;partial F_1}{&#92;partial J&#039;}(&#92;theta,J&#039;) + &#92;epsilon^2 &#92;frac{&#92;partial F_2}{&#92;partial J&#039;}(&#92;theta, J&#039;) + ...' class='latex' /><br />
<img src='http://s0.wp.com/latex.php?latex=J+%3D+J%27+%2B+%5Cepsilon+%5Cfrac%7B%5Cpartial+F_1%7D%7B%5Cpartial+%5Ctheta%7D%28%5Ctheta%2CJ%27%29+%2B+%5Cepsilon%5E2+%5Cfrac%7B%5Cpartial+F_2%7D%7B%5Cpartial+%5Ctheta%7D%28%5Ctheta%2C+J%27%29+%2B+...&amp;bg=ffffff&amp;fg=333333&amp;s=0' alt='J = J&#039; + &#92;epsilon &#92;frac{&#92;partial F_1}{&#92;partial &#92;theta}(&#92;theta,J&#039;) + &#92;epsilon^2 &#92;frac{&#92;partial F_2}{&#92;partial &#92;theta}(&#92;theta, J&#039;) + ...' title='J = J&#039; + &#92;epsilon &#92;frac{&#92;partial F_1}{&#92;partial &#92;theta}(&#92;theta,J&#039;) + &#92;epsilon^2 &#92;frac{&#92;partial F_2}{&#92;partial &#92;theta}(&#92;theta, J&#039;) + ...' class='latex' /><br />
ES) How can we express old variables purely in terms of new variables?<br />
Up to <img src='http://s0.wp.com/latex.php?latex=O%28%5Cepsilon%29&amp;bg=ffffff&amp;fg=333333&amp;s=0' alt='O(&#92;epsilon)' title='O(&#92;epsilon)' class='latex' />,<br />
<img src='http://s0.wp.com/latex.php?latex=%5Ctheta+%3D+%5Ctheta%27+-+%5Cepsilon+%5Cfrac%7B%5Cpartial+F_1%7D%7B%5Cpartial+J%27%7D+%28%5Ctheta%27%2CJ%27%29+%2B+O%28%5Cepsilon%5E2%29&amp;bg=ffffff&amp;fg=333333&amp;s=0' alt='&#92;theta = &#92;theta&#039; - &#92;epsilon &#92;frac{&#92;partial F_1}{&#92;partial J&#039;} (&#92;theta&#039;,J&#039;) + O(&#92;epsilon^2)' title='&#92;theta = &#92;theta&#039; - &#92;epsilon &#92;frac{&#92;partial F_1}{&#92;partial J&#039;} (&#92;theta&#039;,J&#039;) + O(&#92;epsilon^2)' class='latex' /><br />
<img src='http://s0.wp.com/latex.php?latex=J+%3D+J%27+%2B+%5Cepsilon+%5Cfrac%7B%5Cpartial+F_1%7D%7B%5Cpartial+%5Ctheta%27%7D%28%5Ctheta%27%2CJ%27%29+%2B+O%28%5Cepsilon%5E2%29&amp;bg=ffffff&amp;fg=333333&amp;s=0' alt='J = J&#039; + &#92;epsilon &#92;frac{&#92;partial F_1}{&#92;partial &#92;theta&#039;}(&#92;theta&#039;,J&#039;) + O(&#92;epsilon^2)' title='J = J&#039; + &#92;epsilon &#92;frac{&#92;partial F_1}{&#92;partial &#92;theta&#039;}(&#92;theta&#039;,J&#039;) + O(&#92;epsilon^2)' class='latex' /><br />
ES) Note that <img src='http://s0.wp.com/latex.php?latex=%5Ctheta+%5Cto+%5Ctheta%27&amp;bg=ffffff&amp;fg=333333&amp;s=0' alt='&#92;theta &#92;to &#92;theta&#039;' title='&#92;theta &#92;to &#92;theta&#039;' class='latex' /> on the account of near-identity transformation up to <img src='http://s0.wp.com/latex.php?latex=O%28%5Cepsilon%29&amp;bg=ffffff&amp;fg=333333&amp;s=0' alt='O(&#92;epsilon)' title='O(&#92;epsilon)' class='latex' />. What if we need to get higher order? We would face difficulties with disentangling mixed variables.<br />
page 5.20 &#8220;In the Lie method, canonical transformations are generated without mixing old and new variables, therby completely bypassing the disentangling process.&#8221;<br />
&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;&#8212;</p>
<p>page 5.13</p>
<p>&#8220;it is necessary to &#8220;disentangle&#8221; (5.27) to express old variables purely as a function of new variables.&#8221;</p>
<p>ES) Due to the generating function with mixed variables, the disentangling is inevitable in PV method. To the first order, it can be achieved easily since near-identity canonincal transformation is used.</p>
<p>page 5.15</p>
<p>&#8220;In (5.38) it is necessary to assume that the denominator does not vanish, which is equivalent to assuming that ther are no &#8220;first-order resonances&#8221; among the unperturbed oscillators.&#8221;</p>
<p>ES) What if first-order resononces exist among the unperturbed oscillators? What can we do?</p>
<p>page. 5.19</p>
<p>&#8220;The essence of the perturbation method of Poincare&#8217; and Von Zeipel is the use of <strong>near-identity canoncical transformations</strong>, generated by <strong>mixed variable generating functions</strong>, <em><strong>to eliminate the dependence of a Hamiltonian on one or more variables or classes of terms</strong></em>.  &#8230;&#8230;&#8230;.. in the case of time-dependent systems, it is possible to choose the transformation so that the new Hamiltonian K is independent of time. Or, with systems with some fast variables and some slow variables, it may be desirable to choose the transformatin so that the dependence on the fast generalized coordinates is eliminated.&#8221;</p>
<p>page 6.19<br />
&#8220;A much more elegant derivation has been summarized by Cary, who centers his arguments around a certain differential equation in operator space. Cary&#8217;s formulas, including a Lie generator equivalent of the Hamilton-Jacobi equation, are expressed in closed form, i.e. not as a power seires in <img src='http://s0.wp.com/latex.php?latex=%5Cepsilon&amp;bg=ffffff&amp;fg=333333&amp;s=0' alt='&#92;epsilon' title='&#92;epsilon' class='latex' />.&#8221;</p>
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		<title>Streamline, Streakline, and Pathline</title>
		<link>http://eisungy.wordpress.com/2009/09/29/streamline-streakline-and-pathline/</link>
		<comments>http://eisungy.wordpress.com/2009/09/29/streamline-streakline-and-pathline/#comments</comments>
		<pubDate>Tue, 29 Sep 2009 17:41:28 +0000</pubDate>
		<dc:creator>eisungy</dc:creator>
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		<description><![CDATA[From Wiki =) Funny picture Time dependent field is a key!<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=eisungy.wordpress.com&amp;blog=3164591&amp;post=52&amp;subd=eisungy&amp;ref=&amp;feed=1" width="1" height="1" />]]></description>
			<content:encoded><![CDATA[<p>From Wiki =)</p>
<p>Funny picture</p>
<p>Time dependent field is a key!</p>
<div class="wp-caption alignnone" style="width: 510px"><a href="http://en.wikipedia.org/wiki/Stokes_stream_function"><img title="streamline, streakline, pathline" src="http://upload.wikimedia.org/wikipedia/commons/1/13/Streaklines_and_pathlines_animation.gif" alt="The red particle moves in a flowing fluid; its pathline is traced in red; the tip of the trail of blue ink released from the origin follows the particle, but unlike the static pathline (which records the earlier motion of the dot), previously released ink moves up with the flow. (This is a streakline.) The dashed lines represent contours of the velocity field (streamlines), showing the motion of the whole field at the same time." width="500" height="514" /></a><p class="wp-caption-text">The red particle moves in a flowing fluid; its pathline is traced in red; the tip of the trail of blue ink released from the origin follows the particle, but unlike the static pathline (which records the earlier motion of the dot), previously released ink moves up with the flow. (This is a streakline.) The dashed lines represent contours of the velocity field (streamlines), showing the motion of the whole field at the same time.</p></div>
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			<media:title type="html">streamline, streakline, pathline</media:title>
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		<title>Trace and pressure tensor</title>
		<link>http://eisungy.wordpress.com/2009/09/24/trace-and-pressure-tensor/</link>
		<comments>http://eisungy.wordpress.com/2009/09/24/trace-and-pressure-tensor/#comments</comments>
		<pubDate>Thu, 24 Sep 2009 15:43:01 +0000</pubDate>
		<dc:creator>eisungy</dc:creator>
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		<description><![CDATA[Since the trace of any tensor is independent of any coordinate system, the most complete coordinate-free decomposition of a symmetric tensor is to represent it as the sum of a constant tensor and a traceless symmetric tensor. (Symon (1971) Ch. 10) Thus: where δij is the Kronecker delta. The first term on the right is the constant tensor, also [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=eisungy.wordpress.com&amp;blog=3164591&amp;post=50&amp;subd=eisungy&amp;ref=&amp;feed=1" width="1" height="1" />]]></description>
			<content:encoded><![CDATA[<p style="line-height:1.5em;margin:.4em 0 .5em;">Since the <a style="text-decoration:none;color:#002bb8;background-image:none;background-attachment:initial;background-color:initial;background-position:initial initial;background-repeat:initial initial;" title="Trace (linear algebra)" href="http://en.wikipedia.org/wiki/Trace_(linear_algebra)">trace</a> of any tensor is independent of any coordinate system, the most complete coordinate-free decomposition of a symmetric tensor is to represent it as the sum of a constant tensor and a traceless symmetric tensor. <span id="ref_Symon1971"><a style="text-decoration:none;color:#5a3696;background-image:none;background-attachment:initial;background-color:initial;background-position:initial initial;background-repeat:initial initial;" href="http://en.wikipedia.org/wiki/Hooke%27s_law#endnote_Symon1971">(Symon (1971) Ch. 10)</a></span> Thus:</p>
<dl>
<dd><img style="vertical-align:middle;border:initial none initial;" src="http://upload.wikimedia.org/math/2/9/9/299c79b98c8ece815e09b32cc89d3dcb.png" alt="\varepsilon_{ij}=\left(\frac{1}{3}\varepsilon_{kk}\delta_{ij}\right) +\left(\varepsilon_{ij}-\frac{1}{3}\varepsilon_{kk}\delta_{ij}\right)" /></dd>
</dl>
<p style="line-height:1.5em;margin:.4em 0 .5em;">where <span style="font-size:16px;line-height:1.5em;font-family:serif;white-space:nowrap;">δ<sub><em>i</em><em>j</em></sub></span> is the <a style="text-decoration:none;color:#002bb8;background-image:none;background-attachment:initial;background-color:initial;background-position:initial initial;background-repeat:initial initial;" title="Kronecker delta" href="http://en.wikipedia.org/wiki/Kronecker_delta">Kronecker delta</a>. The first term on the right is the constant tensor, also known as the <a style="text-decoration:none;color:#002bb8;background-image:none;background-attachment:initial;background-color:initial;background-position:initial initial;background-repeat:initial initial;" title="Pressure" href="http://en.wikipedia.org/wiki/Pressure">pressure</a>, and the second term is the traceless symmetric tensor, also known as the <a style="text-decoration:none;color:#cc2200;background-image:none;background-attachment:initial;background-color:initial;background-position:initial initial;background-repeat:initial initial;" title="Shear tensor (page does not exist)" href="http://en.wikipedia.org/w/index.php?title=Shear_tensor&amp;action=edit&amp;redlink=1">shear tensor</a>.</p>
<p style="line-height:1.5em;margin:.4em 0 .5em;">
<p style="line-height:1.5em;margin:.4em 0 .5em;"><span id="CITEREFSymon.2C_Keith1971" style="font-style:normal;">Symon, Keith (1971). <em>Mechanics</em>. Addison-Wesley, Reading, MA. <a style="text-decoration:none;color:#002bb8;background-image:none;background-attachment:initial;background-color:initial;background-position:initial initial;background-repeat:initial initial;" href="http://en.wikipedia.org/wiki/Special:BookSources/0201073927">ISBN 0-201-07392-7</a>.</span></p>
<p style="line-height:1.5em;margin:.4em 0 .5em;">
<p style="line-height:1.5em;margin:.4em 0 .5em;"><span style="font-style:normal;">From wiki</span></p>
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			<media:title type="html">\varepsilon_{ij}=\left(\frac{1}{3}\varepsilon_{kk}\delta_{ij}\right) +\left(\varepsilon_{ij}-\frac{1}{3}\varepsilon_{kk}\delta_{ij}\right)</media:title>
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		<title>Working directory</title>
		<link>http://eisungy.wordpress.com/2009/09/11/working-directory/</link>
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		<pubDate>Fri, 11 Sep 2009 19:32:05 +0000</pubDate>
		<dc:creator>eisungy</dc:creator>
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		<description><![CDATA[import os print os.getcwd()<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=eisungy.wordpress.com&amp;blog=3164591&amp;post=48&amp;subd=eisungy&amp;ref=&amp;feed=1" width="1" height="1" />]]></description>
			<content:encoded><![CDATA[<pre style="width:488px;font-family:monospace;margin:0;padding:0;"><span style="color:#ff7700;font-weight:bold;">import</span> <span style="color:#dc143c;">os</span>
<span style="color:#ff7700;font-weight:bold;">print</span> <span style="color:#dc143c;">os</span>.<span style="color:black;">getcwd</span><span style="color:black;">(</span><span style="color:black;">)</span></pre>
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		<title>Data visualization tool</title>
		<link>http://eisungy.wordpress.com/2009/09/10/data-visualization-tool/</link>
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		<pubDate>Thu, 10 Sep 2009 16:38:22 +0000</pubDate>
		<dc:creator>eisungy</dc:creator>
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		<description><![CDATA[A quick look at six open source graphics utilities M. Tim Jones (mtj@mtjones.com), Senior Principal Software Engineer, Emulex Corp. http://www.ibm.com/developerworks/linux/library/l-datavistools/ =============================== This is a good document in that the author explains, compares, and recommend data visualization tools.<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=eisungy.wordpress.com&amp;blog=3164591&amp;post=45&amp;subd=eisungy&amp;ref=&amp;feed=1" width="1" height="1" />]]></description>
			<content:encoded><![CDATA[<p style="font-family:arial, sans-serif;font-size:.76em;margin:0;padding:0 0 1em 4px;"><em>A quick look at six open source graphics utilities</em></p>
<p style="font-family:arial, sans-serif;font-size:.76em;margin:0;padding:0 0 1em 4px;"><span style="background-color:#ffffff;"><em><a style="color:#4c6e94;" rel="#authortip1" href="http://www.ibm.com/developerworks/linux/library/l-datavistools/#author1">M. Tim Jones</a> (<a style="color:#4c6e94;" href="mailto:mtj@mtjones.com?subject=Data%20visualization%20tools%20for%20Linux">mtj@mtjones.com</a>), Senior Principal Software Engineer, Emulex Corp.</em></span></p>
<p><a href="http://www.ibm.com/developerworks/linux/library/l-datavistools/">http://www.ibm.com/developerworks/linux/library/l-datavistools/</a></p>
<p>===============================</p>
<p>This is a good document in that the author explains, compares, and recommend data visualization tools.</p>
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		<title>Fourier series theorem</title>
		<link>http://eisungy.wordpress.com/2009/07/31/fourier-series-theorem/</link>
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		<pubDate>Fri, 31 Jul 2009 15:23:33 +0000</pubDate>
		<dc:creator>eisungy</dc:creator>
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		<description><![CDATA[Fourier Series theorem is relevant to Ballooning representation. Theorem 21.2 (Fourier Series Theorem) . Let  be a function which is piecewise continuous on  .Its Fourier series is given by at each point  where the one sided derivatives  and  both exist. 2. If  is continuous the result is Excerpt from http://www.math.ohio-state.edu/~gerlach/math/BVtypset/node27.html#Fourier_series_theorem Ref. A. Thyagaraja, J. Plasma [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=eisungy.wordpress.com&amp;blog=3164591&amp;post=43&amp;subd=eisungy&amp;ref=&amp;feed=1" width="1" height="1" />]]></description>
			<content:encoded><![CDATA[<p>Fourier Series theorem is relevant to Ballooning representation.</p>
<p><strong>Theorem 21.2</strong> (Fourier Series Theorem)<br />
.<a name="3093"></a></p>
<ol>
<li>Let <img src="http://www.math.ohio-state.edu/~gerlach/math/BVtypset/img341.png" border="0" alt="$ f(x)$" width="41" height="37" align="MIDDLE" /> be a function which is piecewise continuous on <img src="http://www.math.ohio-state.edu/~gerlach/math/BVtypset/img673.png" border="0" alt="$ [-\pi , \pi ]$" width="61" height="37" align="MIDDLE" /> .Its Fourier series is given by</li>
</ol>
<p><img src="http://www.math.ohio-state.edu/~gerlach/math/BVtypset/img674.png" border="0" alt="$\displaystyle \frac{1}{2\pi}\int^\pi_{-\pi}f(t)\,dt+\frac{1}{\pi}\sum^\infty_{n=1} \int^\pi_{-\pi} f(t)\cos n(t-x)\,dt = \frac{1}{2}[f(x^-)+f(x^+)] $" width="540" height="71" align="MIDDLE" /></p>
<p>at each point <img src="http://www.math.ohio-state.edu/~gerlach/math/BVtypset/img675.png" border="0" alt="$ -\pi&lt;x&lt;\pi$" width="103" height="33" align="MIDDLE" /> where the one sided derivatives <img src="http://www.math.ohio-state.edu/~gerlach/math/BVtypset/img662.png" border="0" alt="$ f'_R(x)$" width="50" height="37" align="MIDDLE" /> and <img src="http://www.math.ohio-state.edu/~gerlach/math/BVtypset/img661.png" border="0" alt="$ f'_L(x)$" width="49" height="37" align="MIDDLE" /> both exist.</p>
<p>2. If <img src="http://www.math.ohio-state.edu/~gerlach/math/BVtypset/img9.png" border="0" alt="$ f$" width="16" height="35" align="MIDDLE" /> is continuous the result is</p>
<p><img src="http://www.math.ohio-state.edu/~gerlach/math/BVtypset/img676.png" border="0" alt="$\displaystyle \frac{1}{2\pi}\sum^\infty_{n=-\infty}\int^\pi_{-\pi} e^{in(x-t)} f(t)\,dt =\frac{1}{2}[f(x^-)+f(x^+)]=f(x)\quad \forall\, f\in C[-\pi ,\pi ]\,. $" width="591" height="71" align="MIDDLE" /></p>
<p>Excerpt from <a href="http://www.math.ohio-state.edu/~gerlach/math/BVtypset/node27.html#Fourier_series_theorem">http://www.math.ohio-state.edu/~gerlach/math/BVtypset/node27.html#Fourier_series_theorem</a></p>
<p>Ref. A. Thyagaraja, J. Plasma Physics <strong>59</strong>, 367 (1998)</p>
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			<media:title type="html">eisungy</media:title>
		</media:content>

		<media:content url="http://www.math.ohio-state.edu/~gerlach/math/BVtypset/img341.png" medium="image">
			<media:title type="html">$ f(x)$</media:title>
		</media:content>

		<media:content url="http://www.math.ohio-state.edu/~gerlach/math/BVtypset/img673.png" medium="image">
			<media:title type="html">$ [-\pi , \pi ]$</media:title>
		</media:content>

		<media:content url="http://www.math.ohio-state.edu/~gerlach/math/BVtypset/img674.png" medium="image">
			<media:title type="html">$\displaystyle \frac{1}{2\pi}\int^\pi_{-\pi}f(t)\,dt+\frac{1}{\pi}\sum^\infty_{n=1} \int^\pi_{-\pi} f(t)\cos n(t-x)\,dt = \frac{1}{2}[f(x^-)+f(x^+)] $</media:title>
		</media:content>

		<media:content url="http://www.math.ohio-state.edu/~gerlach/math/BVtypset/img675.png" medium="image">
			<media:title type="html">$ -\pi&#60;x&#60;\pi$</media:title>
		</media:content>

		<media:content url="http://www.math.ohio-state.edu/~gerlach/math/BVtypset/img662.png" medium="image">
			<media:title type="html">$ f'_R(x)$</media:title>
		</media:content>

		<media:content url="http://www.math.ohio-state.edu/~gerlach/math/BVtypset/img661.png" medium="image">
			<media:title type="html">$ f'_L(x)$</media:title>
		</media:content>

		<media:content url="http://www.math.ohio-state.edu/~gerlach/math/BVtypset/img9.png" medium="image">
			<media:title type="html">$ f$</media:title>
		</media:content>

		<media:content url="http://www.math.ohio-state.edu/~gerlach/math/BVtypset/img676.png" medium="image">
			<media:title type="html">$\displaystyle \frac{1}{2\pi}\sum^\infty_{n=-\infty}\int^\pi_{-\pi} e^{in(x-t)} f(t)\,dt =\frac{1}{2}[f(x^-)+f(x^+)]=f(x)\quad \forall\, f\in C[-\pi ,\pi ]\,. $</media:title>
		</media:content>
	</item>
		<item>
		<title>Cygwin Setting only for X11</title>
		<link>http://eisungy.wordpress.com/2009/06/18/cygwin-setting-only-for-x11/</link>
		<comments>http://eisungy.wordpress.com/2009/06/18/cygwin-setting-only-for-x11/#comments</comments>
		<pubDate>Fri, 19 Jun 2009 03:16:11 +0000</pubDate>
		<dc:creator>eisungy</dc:creator>
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		<description><![CDATA[Following module should be installed : X11&#62;xorg-server (required, the Cygwin/X X Server) X11&#62;xinit (required, scripts for starting the X server: xinit, startx, startwin.sh, startxwin.bat (and a shortcut on the Start Menu to run it), startxdmcp.bat ) NET&#62; openssh After cygwin 1.7, you need to type NOT &#8220;startxwin.bat&#8221; BUT &#8220;startxwin&#8221;. There could be some troubles in [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=eisungy.wordpress.com&amp;blog=3164591&amp;post=40&amp;subd=eisungy&amp;ref=&amp;feed=1" width="1" height="1" />]]></description>
			<content:encoded><![CDATA[<p>Following module should be installed :</p>
<li><tt>X11&gt;xorg-server</tt> (required, the Cygwin/X X Server)</li>
<li><tt>X11&gt;xinit</tt> (required, scripts for starting the X server: <strong>xinit</strong>, <strong>startx</strong>, <strong>startwin.sh</strong>, <strong>startxwin.bat</strong> (and a shortcut on the Start Menu to run it), <strong>startxdmcp.bat</strong> )</li>
<li>NET&gt; openssh</li>
<p>After cygwin 1.7, you need to type NOT &#8220;startxwin.bat&#8221; BUT &#8220;startxwin&#8221;.<br />
There could be some troubles in opening multiple X terminals(xterm), and I found a good reference for it even though it&#8217;s for previous version. I have done it with typing &#8220;startxwin.bat&#8221; again and again, but in v.1.7, repeating &#8220;startxwin&#8221; doesn&#8217;t work.</p>
<p><a href="http://http://en.wikibooks.org/wiki/Cygwin#MultiWindow_Mode">http://en.wikibooks.org/wiki/Cygwin#MultiWindow_Mode</a></p>
<p>X -multiwindow &amp;<br />
export DISPLAY=127.0.0.1:0.0<br />
xterm &amp;<br />
xterm &amp;<br />
&#8230;</p>
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