<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article  PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd"><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article"><front><journal-meta><journal-id journal-id-type="publisher-id">JEMAA</journal-id><journal-title-group><journal-title>Journal of Electromagnetic Analysis and Applications</journal-title></journal-title-group><issn pub-type="epub">1942-0730</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/jemaa.2012.46037</article-id><article-id pub-id-type="publisher-id">JEMAA-20341</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Engineering</subject><subject> Physics&amp;Mathematics</subject></subj-group></article-categories><title-group><article-title>
 
 
  Revisiting Magnetic Net and a Bouncing Magnetic Ball
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>aiduke</surname><given-names>Sarafian</given-names></name><xref ref-type="aff" rid="aff1"><sub>1</sub></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib></contrib-group><aff id="aff1"><label>1</label><addr-line>Department of Physics, Pennsylvania State University, University College, York, PA 17403, USA.</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>has2@psu.edu</email></corresp></author-notes><pub-date pub-type="epub"><day>27</day><month>06</month><year>2012</year></pub-date><volume>04</volume><issue>06</issue><fpage>271</fpage><lpage>272</lpage><history><date date-type="received"><day>April</day>	<month>24th,</month>	<year>2012</year></date><date date-type="rev-recd"><day>May</day>	<month>20th,</month>	<year>2012</year>	</date><date date-type="accepted"><day>May</day>	<month>28th,</month>	<year>2012</year></date></history><permissions><copyright-statement>&#169; Copyright  2014 by authors and Scientific Research Publishing Inc. </copyright-statement><copyright-year>2014</copyright-year><license><license-p>This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/</license-p></license></permissions><abstract><p>
 
 
  Recently the author reported the feasibility of envisioning a scenario where a massive permanent magnetic dipole bounces off and oscillates about an invisible horizontal magnetic net in the presence of gravity. The scenario has been revisited, modifying its physical contents. The modification embodies analysis of the impact of the induced current due to the falling magnetic dipole. The induced current counteracts the conduction current and alters the dynamics and kinematics of the motion. This rapid communication reports the recent advances.
 
</p></abstract><kwd-group><kwd>Magnetic net</kwd><kwd> Induced current</kwd><kwd> Mathematica</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Motivations and Goals</title><p>In [<xref ref-type="bibr" rid="scirp.20341-ref1">1</xref>] we utilize the well-known recipe for a magnetic field of a looping conduction DC along the symmetry axis perpendicular to the plane of the loop. The inhomogeneity of the field along this axis causes the field to exert an attractive force on a permanent magnetic dipole with its magnetic moment aligned with the field. In a scenario where the symmetry axis is vertical and so gravity is present we justified the feasibility of oscillations of a loose permanent magnet. Interested readers may review [<xref ref-type="bibr" rid="scirp.20341-ref1">1</xref>] for details.</p><p>We revisit the given scenario outlined above modifying its physical content by including the induced current due to the rate of change of magnetic flux of the falling magnet through the loop. For the sake of simplicity we assume this change comes about from the variation of the axial component of the magnetic field of the magnetic dipole. This puts the characteristics of these two fields, the field of the conduction current and the field of the magnetic dipole in the same footing. The character of the azimuthal field is addressed in [<xref ref-type="bibr" rid="scirp.20341-ref2">2</xref>].</p><p>Magnetic field of the DC looping current along the symmetry axis of the loop is,</p><disp-formula id="scirp.20341-formula140001"><label>(1)</label><graphic position="anchor" xlink:href="7-9801322\a9f703b7-4f6f-4fc4-ba5e-630a7a823db1.jpg"  xlink:type="simple"/></disp-formula><p>where<img src="7-9801322\968109e8-71d9-4a2c-bc94-f2bde9826dad.jpg" />, R, n and i<sub>c</sub> are the radius of the loop, number of the turns and the conduction current, respectively.</p><p>This yields the magnitude of the magnetic force,</p><disp-formula id="scirp.20341-formula140002"><label>(2)</label><graphic position="anchor" xlink:href="7-9801322\7cd7317c-dc26-4b74-803c-70c56c38d8fc.jpg"  xlink:type="simple"/></disp-formula><p>where &#181; is the magnetic moment of the permanent magnet. Equation (1) with a few modifications is written as,</p><disp-formula id="scirp.20341-formula140003"><label>(3)</label><graphic position="anchor" xlink:href="7-9801322\307bf77a-95a3-45f5-97f6-81aa4ad33ebf.jpg"  xlink:type="simple"/></disp-formula><p>This equation is to apply to a cylindrical permanent magnetic dipole of a circular base radius r and a magnetic dipole moment &#181;. The flux of this field through the area of the circular looping DC is<img src="7-9801322\e4f37963-c140-47f1-9a81-5d422da7b9f5.jpg" />. Its rate of change is the induced emf conducive the induced current, i<sub>ind</sub>. Combining these pieces yields,</p><disp-formula id="scirp.20341-formula140004"><label>(4)</label><graphic position="anchor" xlink:href="7-9801322\1553289a-d973-4857-85e4-eddb11061287.jpg"  xlink:type="simple"/></disp-formula><p>where R<sub>resistance</sub> is the ohmic resistance of the conduction loops.</p><p>The induction current given by Equation (4) counteracts the conduction current, i<sub>c</sub> modifying the force F given by Equation (2) to its effective value,</p><disp-formula id="scirp.20341-formula140005"><label>(5)</label><graphic position="anchor" xlink:href="7-9801322\d61c778f-393d-4e7d-accf-24946c0a9fc7.jpg"  xlink:type="simple"/></disp-formula><p>Utilizing F<sub>eff</sub> the equation of motion for the permanent magnet of mass m becomes,</p><disp-formula id="scirp.20341-formula140006"><label>(6)</label><graphic position="anchor" xlink:href="7-9801322\5c7e7875-607c-49b6-acb5-62d39de5a277.jpg"  xlink:type="simple"/></disp-formula><p>At first glance one realizes the order of magnitude of the second term in the brace is O(k'<sup>2</sup>). Knowing the k' is small, one concludes the impact of the i<sub>ind</sub> when compared to i<sub>c</sub> is negligible. Therefore, the dynamics of the falling magnet is being controlled solely by the conduction current. In fact implicitly we have utilized F<sub>eff</sub> = F in [<xref ref-type="bibr" rid="scirp.20341-ref1">1</xref>]. However, if one considers resistances as small as mΩ range this changes the scenario considerably. For instance with the parameters stored in values in MKS units utilizing Mathematica [<xref ref-type="bibr" rid="scirp.20341-ref3">3</xref>] we solve Equation (6) numerically. What follows are the graphic display of the results.</p><p><img src="7-9801322\3b872aea-f1fc-440d-80e8-b744c303a922.jpg" /></p><p>As shown in the first row of <xref ref-type="fig" rid="fig1">Figure 1</xref>, for chosen parameters in [<xref ref-type="bibr" rid="scirp.20341-ref1">1</xref>] a freely dropped magnetic dipole oscillates about the magnetic net. The dashed line is added and serves as a reference; it is the position of the free falling magnet from the loop. The phase diagram, the third graph, is the signature character of an oscillator. In our current analysis with the parameters stored in values the impact of the induced current is shown in the plots of the second row. Accordingly, the induced current softens the attractive magnetic DC force. The profile of the active force vs. time is depicted in the last graph of the second row. The magnet after a few irregular oscillations comes to a halt and settles underneath the loop. In other words, the induced current dampens the motion, preventing the magnet to oscillate steady. At the final resting position the induced current is inactive, and the DC driven attractive magnetic force equalizes the gravity. Interested readers may consider a different set of range parameters for the resistance and the mass conducive to various scenarios.</p></sec><sec id="s2"><title>2. Conclusion</title><p>The author analyzes the impact of the induced current on the equation of motion of a mobile permanent magnetic dipole in the presence of an inhomogeneous magnetic field of a DC. It is shown that by selecting a set of thoughtful parameters the value of the induced current effectively may interfere with the conduction current resulting in curious outcomes.</p></sec><sec id="s3"><title>REFERENCES</title></sec></body><back><ref-list><title>References</title><ref id="scirp.20341-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">H. Sarafian, “Magnetic Net and a Bouncing Magnetic Ball,” Springer-Verlag, Berlin, 2012.</mixed-citation></ref><ref id="scirp.20341-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">H. Sarafian, “Symbolic Computation and Graphic Presentation of Magneto-Static Field and its Associated Vector Potential,” Journal of Electromagnetic Analysis and Applications, Vol. 3, No. 5, 2011, pp. 172-177.  
doi:10.4236/jemaa.2011.35028</mixed-citation></ref><ref id="scirp.20341-ref3"><label>3</label><mixed-citation publication-type="other" xlink:type="simple">Mathematica V 8.01, Wolfram Research Inc., Champaign.</mixed-citation></ref></ref-list></back></article>