<?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">WJM</journal-id><journal-title-group><journal-title>World Journal of Mechanics</journal-title></journal-title-group><issn pub-type="epub">2160-049X</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/wjm.2012.21001</article-id><article-id pub-id-type="publisher-id">WJM-17679</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>
 
 
  Modulation Equations for Roll Waves on Vertically Falling Films of a Power-Law Fluid
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>bdelaziz</surname><given-names>Boudlal</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Valery</surname><given-names>Liapidevskii</given-names></name><xref ref-type="aff" rid="aff2"><sup>2</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib></contrib-group><aff id="aff2"><addr-line>Lavrentyev Institute of Hydrodynamics, Novosibirsk State University, Novosibirsk, Russia</addr-line></aff><aff id="aff1"><addr-line>Laboratoire de Mecanique de Lille, UMR CNRS 8107, Villeneuve d’Ascq, France</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>abdelaziz.boudlal@univ-lille1.fr(BB)</email>;<email>liapid@hydro.nsc.ru(VL)</email>;</corresp></author-notes><pub-date pub-type="epub"><day>29</day><month>02</month><year>2012</year></pub-date><volume>02</volume><issue>01</issue><fpage>1</fpage><lpage>8</lpage><history><date date-type="received"><day>November</day>	<month>20,</month>	<year>2011</year></date><date date-type="rev-recd"><day>December</day>	<month>20,</month>	<year>2011</year>	</date><date date-type="accepted"><day>December</day>	<month>30,</month>	<year>2011</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>
 
 
  Waves of finite amplitude on a thin layer of non-Newtonian fluid modelled as a power-law fluid are considered. In the long wave approximation, the system of equations taking into account the viscous and nonlinear effects has the hyper- bolic type. For the two-parameter family of periodic waves in the film flow on a vertical wall the modulation equations for nonlinear wave trains are derived and investigated. The stability criterium for roll waves based on the hyperbolicity of the modulation equations is suggested. It is shown that the evolution of stable roll waves can be described by self-similar solutions of the modulation equations.
 
</p></abstract><kwd-group><kwd>Power-Law Fluid; Thin Film Flow; Vertical Wall; Modulation Equations; Nonlinear Stability; Roll Wave</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Mud flows are frequently encountered in mountainous regions, especially after torrential rains, and often exhibit a series of breaking waves (roll waves). These type of waves can also be observed as an event following volcano eruptions. A report on roll waves can be found in extensive references quoted by Ng &amp; Mei [<xref ref-type="bibr" rid="scirp.17679-ref1">1</xref>]. The roll waves which occur in inclined open channels are important in drainage problems and have received an extensive treatement in turbulent regime by Jefffreys [<xref ref-type="bibr" rid="scirp.17679-ref2">2</xref>], Dressler [<xref ref-type="bibr" rid="scirp.17679-ref3">3</xref>], Boudlal &amp; Liapidevskii [<xref ref-type="bibr" rid="scirp.17679-ref4">4</xref>], among others, and for a laminar sheet flow by considering the flow with quadratic distribution of velocity profile (Alekseenko &amp; Nakoryakov [<xref ref-type="bibr" rid="scirp.17679-ref5">5</xref>]; Buchin &amp; Shaposhnikova [<xref ref-type="bibr" rid="scirp.17679-ref6">6</xref>]; Julien &amp; Hartley [<xref ref-type="bibr" rid="scirp.17679-ref7">7</xref>]; Boudlal &amp; Liapidevski [<xref ref-type="bibr" rid="scirp.17679-ref8">8</xref>]).</p><p>The discontinuous waves play an important role in engineering and geophysical processes. Roll waves consist of a periodic pattern of bores separated by continuous profiles of free boundary. The transition from uniform flow to intermittent flow regime is usually tackled by resorting to stability theory. When it is perturbed, a steady flow becomes unstable, if certain criteria are satisfied, and evolves towards wave breaking. Dressler has been the first, who gave the analytical solution for such waves in open channel flows. Based on long wave approximation, Dressler’s theory of roll waves was extended in [<xref ref-type="bibr" rid="scirp.17679-ref1">1</xref>] to a shallow layer of fluid mud, which has been modelled as a power law fluid. It has been shown, particularly, that if the fluid is highly non-Newtonian, very long waves may still exist even if the corresponding uniform flow is stable to infinitesimal perturbations.</p><p>The aim of the paper is to give a nonlinear study on stability of permanent roll waves on a shear thinning fluid in the frame of one-dimensional, unsteady, gradually varied, laminar mud flow with the shear stress being evaluated in a conventional manner. Starting from long waves equations averaged over the normal to the bed [<xref ref-type="bibr" rid="scirp.17679-ref1">1</xref>], the standard procedure of roll wave construction is used by matching continuous solutions of shallow water equations through stable hydraulic jumps. As the amplitude and the phase velocity of waves are slowly varying during their propagation and as these variations give rise to instability, the problem of stability is solved by deriving modulation equations for wave series. The stability criterion is formulated in terms of hyperbolicity of modulation equations that need the calculation of averaged quantities.</p><p>All results presented herein can be regarded as a generalization to a power law mud fluid in laminar flow regime of non linear stability method alredy applied to Newtonian turbulent flows in open channels (Boudlal &amp; Liapidevskii [<xref ref-type="bibr" rid="scirp.17679-ref9">9</xref>]).</p></sec><sec id="s2"><title>2. Governing Equations</title><p>Consider two-dimensional film flows of a non-Newtonian liquid on a vertical wall. The coordinate system <img src="1-4900089\fa6d614c-fca6-4fb6-9143-0a72d2e9b574.jpg" /> is defined as follows: the <img src="1-4900089\94b25728-42cd-4498-811c-ee5b3b9cb8cf.jpg" /> axis is directed vertically down and <img src="1-4900089\a6e4b6d8-fea5-4418-8f0a-2f208af6fafa.jpg" /> axis is horizontal and directed outward of the liquid layer. The longitudinal velocity component is denoted by <img src="1-4900089\62a0c28a-762a-4141-be73-458fc703db69.jpg" /> The boundary layer approximation is assumed to be valid, with a power-law shear stress relation for laminar flows taken in the form</p><disp-formula id="scirp.17679-formula7152"><label>(2.1)</label><graphic position="anchor" xlink:href="1-4900089\514ebaf8-4e13-4c30-ae15-bc6c18752edd.jpg"  xlink:type="simple"/></disp-formula><p>Here <img src="1-4900089\7ebff5df-7b3b-479c-8e09-6baefd0ed02f.jpg" /> is the viscosity coefficient of dimension</p><p><img src="1-4900089\12601049-ff54-4ef8-9a36-ea12c916aa78.jpg" />and <img src="1-4900089\075d7ea5-8677-4101-8547-90424683036e.jpg" /> is the flow index<img src="1-4900089\abc04953-7a96-49ff-9dc7-6126eec68c77.jpg" />. The case n = 1 corresponds to the Newtonian fluid and <img src="1-4900089\8aae92cc-ec37-4aa3-804b-346010205d2f.jpg" /> is the ordinary dynamic viscosity [<xref ref-type="bibr" rid="scirp.17679-ref1">1</xref>]. By assuming the following form of the velocity profile in the film flow</p><disp-formula id="scirp.17679-formula7153"><label>, (2.2)</label><graphic position="anchor" xlink:href="1-4900089\78e19764-22e0-4937-8ce9-5497e036a1b2.jpg"  xlink:type="simple"/></disp-formula><p>the governing equations, which consist of the mass and momentum conservation equations averaged in the ordinate direction, are reduced to the system [<xref ref-type="bibr" rid="scirp.17679-ref1">1</xref>].</p><disp-formula id="scirp.17679-formula7154"><label>(2.3)</label><graphic position="anchor" xlink:href="1-4900089\b6a94cc5-b5fb-4715-9646-4b845d8de9fa.jpg"  xlink:type="simple"/></disp-formula><p>Here h is the layer thickness, <img src="1-4900089\ef639bcf-da61-49ac-973d-2e50b4bb3c56.jpg" />is the depth-averaged velocity, <img src="1-4900089\7a90376b-9470-4502-a262-27e4379f201b.jpg" />is the bottom stress, g is the gravity acceleration, <img src="1-4900089\5b427dbc-e225-47ba-8cf5-ad1be2a005c8.jpg" />is the momentum flux factor. For a shear-thinning fluid, which will be considered bellow, we have <img src="1-4900089\fd869a5e-7d82-4aba-8909-ffb8aa16011c.jpg" /> and, consequently,<img src="1-4900089\926fab22-f704-45d1-945c-27cf05394502.jpg" />.</p><p>In dimensionless variables introduced in [<xref ref-type="bibr" rid="scirp.17679-ref1">1</xref>]; namely,</p><disp-formula id="scirp.17679-formula7155"><label>(2.4)</label><graphic position="anchor" xlink:href="1-4900089\d87b2dcf-b77d-485f-82d4-611518bf9c25.jpg"  xlink:type="simple"/></disp-formula><p>Equation (2.3) take the form (asterisks are omitted)</p><disp-formula id="scirp.17679-formula7156"><label>(2.5)</label><graphic position="anchor" xlink:href="1-4900089\345d4205-36ff-4314-82e4-af55ff727e5e.jpg"  xlink:type="simple"/></disp-formula><p>Here the reference depth <img src="1-4900089\9add4289-a235-4c37-b261-4fbd930829a7.jpg" /> and the reference velocity <img src="1-4900089\46f93749-bbc7-406e-8df2-44d1fa7add9e.jpg" /> are expressed through the given flow rate <img src="1-4900089\e1b1a909-9cd8-44e6-a761-2186c5fe8d4e.jpg" /> and the viscosity <img src="1-4900089\b5dcad8b-2233-4355-8ac9-bc76a2594e69.jpg" /> as follows:</p><disp-formula id="scirp.17679-formula7157"><label>(2.6)</label><graphic position="anchor" xlink:href="1-4900089\3545e55f-81dc-4ada-b457-e68a9a0a9d79.jpg"  xlink:type="simple"/></disp-formula><p>Note that Equation (2.5) are hyperbolic with the characteristics</p><disp-formula id="scirp.17679-formula7158"><label>. (2.7)</label><graphic position="anchor" xlink:href="1-4900089\1972bd7c-1b6b-4fba-a87e-f549bbf2a0e9.jpg"  xlink:type="simple"/></disp-formula><p>It is shown by linear analysis in [<xref ref-type="bibr" rid="scirp.17679-ref1">1</xref>] that any steady-state solution of (2.5)</p><p><img src="1-4900089\c6d629e7-6af5-4ed2-886e-e842ce5bd357.jpg" /></p><p>is unstable. The instability of the uniform steady-state flow also can be easily checked by the Whitham method [<xref ref-type="bibr" rid="scirp.17679-ref9">9</xref>]. The flow is unstable if the velocity of the kinematic wave <img src="1-4900089\7f5d029b-503b-4808-81ad-8e22d87598c7.jpg" /> exceeds the velocity of long waves in (2.5), i.e.</p><disp-formula id="scirp.17679-formula7159"><label>. (2.8)</label><graphic position="anchor" xlink:href="1-4900089\99504502-efc3-4018-bfc8-0b9cdd5b0d51.jpg"  xlink:type="simple"/></disp-formula><p>It is clear that (2.8) is satisfied for<img src="1-4900089\5eb7c03a-457f-4931-a00d-6cb5cc529809.jpg" />, since</p><p><img src="1-4900089\abed5eef-8bee-46db-a34d-927b6ff0d5ad.jpg" />and<img src="1-4900089\79adc6d1-5c60-4d6a-bb80-f292ba32911f.jpg" />.</p></sec><sec id="s3"><title>3. Roll Waves</title><p>Analogously to unstable flow regimes in open channel flows, the roll waves or periodic discontinuous solutions, have been constructed for (2.5) [<xref ref-type="bibr" rid="scirp.17679-ref1">1</xref>]. In this section we give the short description of roll waves in the form suitable for the purposes of the paper.</p><p>Consider the travelling waves propagating with a constant velocity<img src="1-4900089\694de846-d18e-41b1-809f-85cb77be5db3.jpg" />. Introducing the variable <img src="1-4900089\71aa3fee-1128-4a4b-9002-8898cc62efd8.jpg" /> and assuming the flow being steady in the coordinate system moving with the velocity<img src="1-4900089\da34edb3-6659-4277-b6c2-79158006f907.jpg" />, Equation (2.5) are reduced to the ODE</p><disp-formula id="scirp.17679-formula7160"><label>, (3.1)</label><graphic position="anchor" xlink:href="1-4900089\e1a080e9-71fa-40d5-9464-82df98e61f1e.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="1-4900089\ed2cbcfd-fa0c-4c3e-bf4b-4376a16c35aa.jpg" /> and</p><disp-formula id="scirp.17679-formula7161"><label>(3.2)</label><graphic position="anchor" xlink:href="1-4900089\e51c6232-f42f-44c1-8093-b7c1c61a8a26.jpg"  xlink:type="simple"/></disp-formula><p>Let y and <img src="1-4900089\53886802-2bb0-4ed4-861e-148e3a5ffea4.jpg" /> be the critical depth and the critical velocity with <img src="1-4900089\27ba7991-81cf-44f7-9e50-cfc91ad599b7.jpg" /> It follows from (3.1) that the necessary condition of roll wave existence is</p><disp-formula id="scirp.17679-formula7162"><label>(3.3)</label><graphic position="anchor" xlink:href="1-4900089\1323889a-2120-4361-974b-7ded1b2fe4ec.jpg"  xlink:type="simple"/></disp-formula><p>In view of (3.2) we have</p><disp-formula id="scirp.17679-formula7163"><label>. (3.4)</label><graphic position="anchor" xlink:href="1-4900089\2c5776c2-778b-44f4-9bff-60b2365a03fe.jpg"  xlink:type="simple"/></disp-formula><p>Note that</p><disp-formula id="scirp.17679-formula7164"><label>(3.5)</label><graphic position="anchor" xlink:href="1-4900089\13302f52-7287-41ca-b7e9-4f48a6c0c534.jpg"  xlink:type="simple"/></disp-formula><p>and, consequently, <img src="1-4900089\d79714f7-11c5-47af-9d2c-7530e65c9915.jpg" />at the critical depth.</p><p>Let <img src="1-4900089\91fa4b03-07fc-4967-9b45-78c04ebb1414.jpg" /> be fixed and<img src="1-4900089\96dbf4cd-935e-4863-bc17-26cfcab24332.jpg" />. Equations (3.1)-(3.2) take the form</p><disp-formula id="scirp.17679-formula7165"><label>. (3.6)</label><graphic position="anchor" xlink:href="1-4900089\fb36cc73-79d2-41c1-bc04-208f3d5bd4e0.jpg"  xlink:type="simple"/></disp-formula><p>To find the function <img src="1-4900089\726072e1-abca-4cf8-8087-37f286281b46.jpg" />in (3.6), the following identity is used:</p><p><img src="1-4900089\771a213d-2848-4c70-963f-908307720f84.jpg" />.</p><p>Furthermore, the function <img src="1-4900089\4a43216d-2fab-4600-99ba-4cce81023376.jpg" /> can be represented as follows</p><disp-formula id="scirp.17679-formula7166"><label>(3.7)</label><graphic position="anchor" xlink:href="1-4900089\d91679ab-cdd7-47da-821f-07af79b7bfe5.jpg"  xlink:type="simple"/></disp-formula><p>where<img src="1-4900089\d5a51194-b561-4f6d-9eea-ae781047574e.jpg" />, and <img src="1-4900089\7c31501f-3583-4e3a-9376-00ac9d991992.jpg" /> is a root of the equation <img src="1-4900089\9f5fb32d-c281-44d0-a223-f64f3b641de9.jpg" /> at the interval<img src="1-4900089\fb2ff09d-bf95-4481-b292-9085b7ffc9a0.jpg" />. The continuous function</p><p><img src="1-4900089\bc896dcd-be7e-497b-bd4e-9e8bd828f2ab.jpg" /></p><p>is positive for<img src="1-4900089\4ac54157-067b-48a8-ae9c-bce918d7ad3b.jpg" />. It means that the function <img src="1-4900089\2b971497-c3d6-409c-80b5-94c1935e03d2.jpg" /> vanishes only at two points <img src="1-4900089\5a6e825c-bfc2-4449-ac49-9b132b5e16c8.jpg" /> and <img src="1-4900089\4c96cf25-cd5f-4e1c-bac4-246a37f5e97d.jpg" /> for <img src="1-4900089\318d3d23-ca46-45ac-916c-be598a3abdd8.jpg" /> [<xref ref-type="bibr" rid="scirp.17679-ref1">1</xref>]. Therefore, <img src="1-4900089\69ffacd8-e16c-4cf9-82bc-2941e51cba5c.jpg" />for <img src="1-4900089\a5e48337-1053-439b-97b8-52e9d7bbba9f.jpg" /> and</p><p><img src="1-4900089\bea2f4f1-3b71-4d29-a690-7ad42642c8f7.jpg" />.</p><p>Now we can construct the two-parameter family of roll waves as follows: for given <img src="1-4900089\f16adbcc-d29a-4a35-bdbb-caad020deca4.jpg" /> and <img src="1-4900089\adc2caa6-7871-4a2c-af6d-128a94d1fb7d.jpg" /> we put<img src="1-4900089\8f394a47-35d1-4d95-a706-1b03f23f4e97.jpg" />, <img src="1-4900089\439c7e53-ef2e-4096-a71b-06f44e9868d0.jpg" />,<img src="1-4900089\2ee22261-927a-4447-88aa-48f57403b2a6.jpg" />. Note that <img src="1-4900089\51fc26a1-ac78-4608-990f-9a42a613ec9b.jpg" /> and <img src="1-4900089\2481a429-c344-45e6-b76d-5ca2a716dc53.jpg" /> are the conjugate depths, since the Rankine-Hugoniot conditions for discontinuous solutions of (2.5), which are reduced to the relation</p><p><img src="1-4900089\bb75c099-56b8-4f14-9249-8e9c399419f9.jpg" />or</p><p><img src="1-4900089\f31a6cd8-6d5d-4ed7-8a3e-8a7088fcbd28.jpg" />,(3.8)</p><p>are fulfilled. The stability condition for shocks satisfying (3.8) takes the form (Rozhdestvenskii and Janenko [<xref ref-type="bibr" rid="scirp.17679-ref10">10</xref>])</p><p><img src="1-4900089\b70333dd-1720-446b-a11d-9406bb527142.jpg" />or</p><disp-formula id="scirp.17679-formula7167"><label>(3.9)</label><graphic position="anchor" xlink:href="1-4900089\1ea769a3-0dc5-4237-bfb4-17d32cf593b1.jpg"  xlink:type="simple"/></disp-formula><p>Thus the admissible values of the governing parameters<img src="1-4900089\0269bb31-6d66-4ba0-95a3-da9c16a76a00.jpg" />, for which a roll wave exists, belong to the domain</p><p><img src="1-4900089\809f4360-1668-4b6a-ba8a-302e6b1f5316.jpg" /></p><p>For<img src="1-4900089\b6fed92f-f5cb-40a1-a55b-534d42c3d0a7.jpg" />, a roll wave consists of the smooth part defined by the monotonous solution <img src="1-4900089\bd58ea33-4abc-47e6-9828-4cc66d465d6b.jpg" /> of (3.6) at the interval <img src="1-4900089\d8cc18e8-4ca0-49e9-b1b4-aa4b17973528.jpg" /> and of the jump with the conjugate depths <img src="1-4900089\1b50d75b-bab7-4e65-b7ba-b0a0d0daff68.jpg" /> and <img src="1-4900089\e8109fdd-2938-499f-9cf9-394f26addce2.jpg" /></p></sec><sec id="s4"><title>4. Modulation Equations</title><p>It is shown in the previous section that analogously to the roll waves in open channel flows governed by the classic shallow water theory (Whitham [<xref ref-type="bibr" rid="scirp.17679-ref10">10</xref>]), the periodic travelling waves (roll waves) in film flow of a non-Newtonian fluid can be represented by the two-parameter family of discontinuous solutions of (2.5). We chose <img src="1-4900089\f3562935-79bc-4ab4-b26a-c749fbc66ebc.jpg" /> and <img src="1-4900089\0c2a0aba-b813-41b1-8c0a-b53d1e5454ad.jpg" /> as such parameters. The problem on nonlinear stability of periodic wave trains with slowly varying values <img src="1-4900089\c189eee0-45d5-46ad-a209-891f147819a7.jpg" /> and <img src="1-4900089\26a150c6-97f6-4e42-b518-09e6fd74e078.jpg" /> can be solved by analysis of hyperbolicity of the modulation equations for roll waves (Boudlal and Liapidevskii, [<xref ref-type="bibr" rid="scirp.17679-ref11">11</xref>]). After averaging (2.5) over the fixed length scale, which is large enough compared with the length of roll waves, we have the following modulation equations:</p><disp-formula id="scirp.17679-formula7168"><label>(4.1)</label><graphic position="anchor" xlink:href="1-4900089\967743a7-1833-4e7b-ba76-b810942db4e8.jpg"  xlink:type="simple"/></disp-formula><p>All averaged quantities can be expressed as functions of <img src="1-4900089\c61745ad-856c-42b4-80a3-e3ab8e78acc3.jpg" /> and <img src="1-4900089\ca61e372-0ea2-41ae-937b-4f986b9a4eb8.jpg" /> as follows :</p><disp-formula id="scirp.17679-formula7169"><label>(4.2)</label><graphic position="anchor" xlink:href="1-4900089\ea9464bd-8031-4674-a3b6-15bcaa929431.jpg"  xlink:type="simple"/></disp-formula><p>Here we have used (3.1)-(3.2), (3.8) for periodic roll waves defined by parameters <img src="1-4900089\b7ed8f29-f5f1-43eb-aced-ee12009615a2.jpg" /> and<img src="1-4900089\b26fc3c2-df08-4dce-900d-7f54b32f20bf.jpg" />.</p><p>In view of (4.2) and (3.4) the modulation equations take the form</p><disp-formula id="scirp.17679-formula7170"><label>(4.3)</label><graphic position="anchor" xlink:href="1-4900089\9857af37-9aa4-449c-9575-9d4b99605aa9.jpg"  xlink:type="simple"/></disp-formula><p>where</p><disp-formula id="scirp.17679-formula7171"><label>(4.4)</label><graphic position="anchor" xlink:href="1-4900089\bc784976-5cc0-4374-a213-22b19deb3ea3.jpg"  xlink:type="simple"/></disp-formula><p>The nonstationary evolution of the governing parameters <img src="1-4900089\2500b862-64ae-4136-b0ea-16c05bf08a55.jpg" /> for a periodic wave train is described by Equation (4.3). We say the roll waves are stable if the modulation Equation (4.3) for corresponding values <img src="1-4900089\81555b90-8710-43b3-ad8d-c3f023482b61.jpg" /> are hyperbolic. Considering <img src="1-4900089\537e55f2-9835-4c33-89a6-e1bdb8e08739.jpg" /> and <img src="1-4900089\485d3c9f-7337-4211-a746-a66c0d99ced0.jpg" /> as new dependent variables instead of <img src="1-4900089\e90e38d5-2b91-4a8a-bd9c-2c57c8186dae.jpg" /> and<img src="1-4900089\df49b3c7-e08f-43b9-a4e4-af81f83df6a8.jpg" />, we can find the characteristics of (4.3) from the quadratic equation</p><disp-formula id="scirp.17679-formula7172"><label>(4.5)</label><graphic position="anchor" xlink:href="1-4900089\c4be1b33-9da7-4709-aa0d-dda541fab2bd.jpg"  xlink:type="simple"/></disp-formula><p>where</p><disp-formula id="scirp.17679-formula7173"><label>(4.6)</label><graphic position="anchor" xlink:href="1-4900089\59843e3e-8f2b-485b-ba7b-ec3ef074cdac.jpg"  xlink:type="simple"/></disp-formula><p>Here “&#183;” denotes the differentiation on <img src="1-4900089\3dcd832d-bc71-48f9-a668-6d6c3fc40fcc.jpg" /> and<img src="1-4900089\ca21d844-881f-466d-82da-a5e66f3c47f2.jpg" />.</p><p>Equation (4.3) are hyperbolic for<img src="1-4900089\c058cca7-9532-4aae-b520-a5340e18d433.jpg" />. It means that the hyperbolicity domain depends only on the variable <img src="1-4900089\5a864d3a-5b6d-440a-b061-c3d4d7423065.jpg" /> or <img src="1-4900089\bcddca35-4394-40cc-8350-82b34552bf23.jpg" /> Note that <img src="1-4900089\7f74ff56-9db7-45d2-b6ff-fffeb461be8c.jpg" /> for<img src="1-4900089\08cfb94a-9813-430a-b34e-ece148e1eb76.jpg" />. It can be shown by numerical calculations that the hyperbolicity interval is rather narrow and it lies in vicinity of<img src="1-4900089\3fd5a714-8469-49d5-bb4a-4b264a6c942e.jpg" />. For n = 1 <img src="1-4900089\e7f22738-43c7-4419-baf9-39d6da76746b.jpg" /> the values of <img src="1-4900089\dc04d992-4546-4c30-9ef9-e8803dceaa19.jpg" /> corresponding to the hyperbolicity domain belong to the interval <img src="1-4900089\d1c1cc08-de6f-415c-bbfc-83c18e67079f.jpg" /> with <img src="1-4900089\1583ebdc-fe8a-408e-8f53-dfef62520514.jpg" /> Therefore, the boundary of the hyperbolicity domain can be found effectively by the following approximation of the function <img src="1-4900089\d1e63516-5a86-4eef-b5d2-0e6900761ee1.jpg" /> for long waves <img src="1-4900089\86358fd1-75a1-4854-8d5b-441abdfbc447.jpg" /></p><disp-formula id="scirp.17679-formula7174"><label>(4.7)</label><graphic position="anchor" xlink:href="1-4900089\2b040ea0-16db-4fe2-9d14-3cdddcfe6764.jpg"  xlink:type="simple"/></disp-formula><p>Approximate values of characteristics are given by (4.5)-(4.6) with <img src="1-4900089\aa220d24-e98d-4cb6-b5b1-278d7d76e5e3.jpg" /> instead of <img src="1-4900089\61812342-d679-467b-9f91-f2234eea14a7.jpg" /> and <img src="1-4900089\b5867394-46c1-4a6b-be1d-2f564a809c62.jpg" /> instead of<img src="1-4900089\a8256445-2e07-484e-aea1-2cb22ee99ce0.jpg" />. In this case the modulation equations simplify considerably since the functions <img src="1-4900089\27b185e2-a89f-4dbb-9b57-eec73f9accf8.jpg" /> and <img src="1-4900089\84e71f13-8248-4aab-a13c-1fb83f68efc8.jpg" /> are linear on<img src="1-4900089\6f2cfc87-6406-4989-809d-43fcb11c5634.jpg" />:</p><disp-formula id="scirp.17679-formula7175"><label>(4.8)</label><graphic position="anchor" xlink:href="1-4900089\9eb29bc6-5a0e-4e7b-83fb-31a0f7224919.jpg"  xlink:type="simple"/></disp-formula><p>The dependence <img src="1-4900089\94eb43ed-18d2-4eae-b4f1-1fe50ae60717.jpg" /> for Equations (4.3), (4.8) with n = 1 is shown in <xref ref-type="fig" rid="fig1">Figure 1</xref> for real roots of (4.5) (<img src="1-4900089\e7882cd3-3f1b-44fd-8cd8-58e296d184c8.jpg" />). Note that the corresponding graphs for (4.3), (4.4) and the approximate system (4.3), (4.8) practically concide, so we can use the latter system for the analysis of nonlinear stability of roll waves in the flows governed by (2.5). It follows from <xref ref-type="fig" rid="fig1">Figure 1</xref> that the hyperbolicity interval <img src="1-4900089\adbe2b78-4c49-469c-8864-75a0bb00060e.jpg" /> for (4.3), (4.8) lies inside of the admissible interval of roll wave existence<img src="1-4900089\7044a389-6049-4028-b939-ef3c98a5174d.jpg" />. It means that short roll waves <img src="1-4900089\c0c0e585-5638-4cdf-8501-e8105e90a6c6.jpg" /> and very long roll waves <img src="1-4900089\5d423380-7c69-4d24-9779-2dd338605ab3.jpg" /> are unstable.</p><p>The simple centered waves, i.e. the self-similar solutions of (4.3) depending on the variable<img src="1-4900089\b31e0513-bf95-4d9e-ae78-d32ec2de0f38.jpg" />, can be found analytically. Equations (4.3), (4.8) for simple</p><p>waves take the form</p><disp-formula id="scirp.17679-formula7176"><label>(4.9)</label><graphic position="anchor" xlink:href="1-4900089\3765134c-e8e1-4c51-a93a-aff0eac0c1e7.jpg"  xlink:type="simple"/></disp-formula><p>A solution of (4.9) can be represented in the form</p><disp-formula id="scirp.17679-formula7177"><label>(4.10)</label><graphic position="anchor" xlink:href="1-4900089\5080cbec-1718-44df-bfb8-daac60b21a6b.jpg"  xlink:type="simple"/></disp-formula><p>Here <img src="1-4900089\fbd8fb2c-82ee-4291-acf2-a4369d1adc10.jpg" /> is a solution of (4.3) for the corresponding family of characteristics. The solution (4.10) can be applied to explain some specific features of roll wave dynamics considered below.</p></sec><sec id="s5"><title>5. Roll Wave Dynamics</title><p>In this section we compare the numerical calculations performed for the model derived by Meza and Balakotaiah (2008) for vertically falling films of Newtonian fluid with numerical solutions of (2.3) for n = 1. Both models are derived for moderate Reynolds numbers of flow, but in contrast to the former model, the surface tension in Equation (2.3) is ignored. Let us rescale (2.3) slightly according to (Meza and Balakotaiah, 2008). For that we introduce the Reynolds number <img src="1-4900089\6284d121-7660-4c57-b7df-224d7533d6bb.jpg" /> and the Weber number <img src="1-4900089\bf2e28d3-2b66-454b-8d43-eb50ed31476a.jpg" /> as follows</p><p><img src="1-4900089\798029cb-ee51-4f52-b921-d76700f5cb80.jpg" /></p><p>Here <img src="1-4900089\aa0c144e-6ab7-458e-ab6f-4921fcb3b99a.jpg" /> is the surface tension. Consider two models of film flows on a vertical wall depending on <img src="1-4900089\269a011f-7e5c-440d-8795-fae962155745.jpg" /> and <img src="1-4900089\14a5878f-a8a6-4e62-9d09-f0038a25c192.jpg" /> explicitly. The first one is the Shkadov model [<xref ref-type="bibr" rid="scirp.17679-ref12">12</xref>], which with the dependent variables <img src="1-4900089\a294b950-3aac-483e-815b-958991ecdcbd.jpg" /> and <img src="1-4900089\fd57f0c7-d3fd-4c6b-a745-578387b1a208.jpg" /> takes the form</p><disp-formula id="scirp.17679-formula7178"><label>(5.1)</label><graphic position="anchor" xlink:href="1-4900089\c208fa44-d9d5-466d-9d1f-7ed04b8512f5.jpg"  xlink:type="simple"/></disp-formula><p>It is clear that for <img src="1-4900089\05a5492a-a25d-407b-a46f-c88064683a84.jpg" /> and<img src="1-4900089\998aa4b7-5f9d-4371-9e5d-e3c6db8f2ae6.jpg" />. Equations (2.5) are equivalent to (5.1) and the systems can be transformed to each other by dilatation of independent variables. The momentum equation derived by Meza and Balakotaiah [<xref ref-type="bibr" rid="scirp.17679-ref13">13</xref>] gives the more accurate dispersion relations comparing with the Shkadov model as it has reported in their paper:</p><disp-formula id="scirp.17679-formula7179"><label>(5.2)</label><graphic position="anchor" xlink:href="1-4900089\82ac6a42-0f56-4c69-ae28-0d96ac66d2fa.jpg"  xlink:type="simple"/></disp-formula><p>We will compare below numerical solutions of the model (5.2) presented in [<xref ref-type="bibr" rid="scirp.17679-ref13">13</xref>] with the corresponding numerical solutions of the hyperbolic model (5.1) with<img src="1-4900089\f5ffb356-1973-48a2-a21f-8079cc04d7dc.jpg" />. It will be shown that despite of the difference in the shape of individual roll waves for the models with and without surface tension, the evolution of nonlinear periodic wave trains generated by monochromatic initial perturbations is very alike for both models. Note that Equations (5.1) and (5.2) are written in dimensionless variables. The characteristics of (5.1) with <img src="1-4900089\849111b4-78dc-4425-9144-2e71b68bd99b.jpg" /> coincide with (2.7) and are positive. Therefore, to find a solution of (5.1) in the domain <img src="1-4900089\f2997090-cb86-4cb0-a69b-193bdb4f5012.jpg" />, we must put the values of <img src="1-4900089\51a914a8-3dc4-411a-b213-7a5a1b715eef.jpg" /> at the boundaries <img src="1-4900089\90913fce-7597-4242-a252-b915894b59c5.jpg" />and<img src="1-4900089\2cb6811a-d53e-461e-aca8-83714896c15c.jpg" />. The corresponding data are taken from (Meza and Balakotaiah, 2008) for the cases considered in their paper, namely:</p><disp-formula id="scirp.17679-formula7180"><label>(5.3)</label><graphic position="anchor" xlink:href="1-4900089\63e2dcf2-a2b0-4ae8-a87b-77fa2230c25b.jpg"  xlink:type="simple"/></disp-formula><p>We restrict our attention to the case 1 in [<xref ref-type="bibr" rid="scirp.17679-ref13">13</xref>] with<img src="1-4900089\f30c5aa1-1ba7-4ece-8afc-d83849c9dec7.jpg" />. The Weber number for (5.2) is finite (<img src="1-4900089\af815cc1-4f95-48bc-9edb-c5065dfa4feb.jpg" />) and it vanishes for (5.1). The values of the dimensionless frequency <img src="1-4900089\fc322339-321f-4a96-954a-de9c47cf08e8.jpg" /> are varied to demonstrate its influence on roll wave dynamics.</p><p>Numerical calculations using a variant of the Godunov standard scheme illustrate the development of roll waves on the free surface of a thin film flowing on a vertical wall in the frame of the hyperbolic model (5.1). In Figures 2-4 the perturbations of free surface of the liquid layer calculated by (5.1) are comparing with correspond-</p><p>ing calculations from [<xref ref-type="bibr" rid="scirp.17679-ref13">13</xref>], at given time. In both cases small perturbations, which amplitudes do not exceed a small fraction of the depth of the initial steady-state flow, are developing into roll waves of finite amplitude. Note that the waves stop to grow after they reach some critical value of amplitude. The interesting feature of roll wave evolution is the transition from “saturated” waves to very long waves (“tsunami” waves according [<xref ref-type="bibr" rid="scirp.17679-ref11">11</xref>]). Such transition is most pronounced in <xref ref-type="fig" rid="fig4">Figure 4</xref>. It is seen from Figures 4(a)-(c) that the length of the transition zone is increasing with time linearly. The analysis of the nonstationary evolution of roll wave packets is the subject of future investigations. Here we just give an idea how the self-similar solutions (4.10) can be applied to describe the transition “0” - “1” shown in Figures 4(a)-(c). First of all, for given frequency <img src="1-4900089\af815bda-d9e9-42cb-bb8d-d7ede3bd0768.jpg" /> of the monochromatic wave packet “0”, the governing parameters <img src="1-4900089\7a993fee-3aef-4075-bc7d-850fb31c374e.jpg" /> are uniquelly determined by (3.4), (4.2), (4.7). Furthermore, in virtue of (4.10) the left boundary <img src="1-4900089\4bd2f1b3-309b-496a-8ef3-6c3b810cd152.jpg" /> of the centered simple wave is known. The right boundary of the simple wave is calculated using (4.10) and the additional condition for “tsunami” waves:<img src="1-4900089\49e3296c-26e0-44c2-87a8-05cd9e763484.jpg" />.</p><p>This algorithm gives the reasonable values for the boundaries of the states “0” and “1” in numerical calculations of the nonstationary problem of roll wave evolution. Therefore, the transition “0” - “1” in Figures 4(a)- (c) can be described by the centered simple wave of (4.9) moving on the left <img src="1-4900089\1b45cc72-d707-4b5d-bf78-324e543b8868.jpg" /> and the roll waves shown in <xref ref-type="fig" rid="fig4">Figure 4</xref> are stable, since the governed parameters <img src="1-4900089\2b6772f9-4655-445c-ab1e-febe04d62578.jpg" /> in a simple wave always belong to the hyperbolicity domain of the modulation equations</p></sec><sec id="s6"><title>6. Conclusion</title><p>We have investigated the roll wave generation on vertically falling films by the nonlinear hyperbolic model (2.3), in which the viscous effects are taken into account by assuming that the velocity profile of an exact steady-state solution of the two-dimensional problem can be used also in the one-dimensional wavy flows. The model is based on the first order long-wave approximation of non-Newtonian fluid flows, which shear rate is modeled by a power law [<xref ref-type="bibr" rid="scirp.17679-ref1">1</xref>]. The capillarity effects are ignored to reveal the interplay between nonlinear and viscous terms in the governing equations. It is shown that</p><p>the periodic discontinuous solutions of (2.3) (roll waves) can be described by two parameters analogously to the roll waves in open channel flows. Moreover, the nonlinear stability of finite amplitude roll waves can be expressed in the terms of the hyperbolicity of modulation Equations (4.3) for the governing parameters of roll waves. Comparison of numerical calculations of roll wave evolution for the models with and without surface tension effects reveal that in spite of the difference in the individual wave shapes the behavior of roll wave packets is very alike for the models. In particular, the transition from “saturated” to “tsunami” waves described in [<xref ref-type="bibr" rid="scirp.17679-ref13">13</xref>] can be described by a simple wave of the modulation Equations (4.3).</p></sec><sec id="s7"><title>7. Acknowledgements</title><p>The work was supported by the Russian Foundation for Basic Research (Grant No. 10-01-00338) and by the Program for support of leading scientific schools of the Russian Federation (Grant No. NSh-6706.2012.1).</p></sec><sec id="s8"><title>REFERENCES</title></sec></body><back><ref-list><title>References</title><ref id="scirp.17679-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">C. O. Ng and C. C. Mei, “Roll Waves on Shallow Layer of Mud Modelled as a Power-Law Fluid,” Journal of Fluid Mechanics, Vol. 263, 1994, pp. 151-1834.</mixed-citation></ref><ref id="scirp.17679-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">T. 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