In the first step, we make use of several linear estimates to solve a fourth-order parabolic regularization of the mKP II equation by a fixed point argument, for regular initial data (one estimate is similar to the sharp Kato smoothing effect proved for the KdV equation by Kenig, Ponce, and Vega, 1991).
Then, compactness arguments (the energy method performed through the Miura transform) give the existence of a local solution of the mKP II equation for regular data.
Finally, we approximate any data in the energy space by a sequence of smooth initial data. Using Bourgain's result concerning the global well-posedness of the KP II equation in and the Miura transformation, we obtain convergence of the sequence of smooth solutions to a solution of mKP II in the energy space.
Zusammenfassung Die Strömung um einen Körper, der sich langsam in einem grossen, rotierenden Behälter bewegt, wird untersucht mit einer asymptotischen Theorie für eine reibungsfreie, inkompressible Flüssigkeit bei einer kleinen Rossby-Zahl, d.h. u c /L1. Der axiale AbstandH zwischen den Gefässwänden wird als soviel grösser als die Körperabmessung angenommen, dass für die reduzierte Höhe =H/L 0(1) gilt. Diese Strömung erlaubt eine säulenähnliche Struktur (Taylor column) in Körpernähe und eine äussere, nichtlineare Struktur vom Wellentyp für Höhenz=0(L/) über dem Köper. Die innere Randbedingung für das äussere Problem wird erhalten, indem die Bedingung an der Wand durch die Säule verschoben wird. Die äussere Lösung bestimmt ihrerseits die Rotation und damit die Lösung im inneren, säulenartigen Bereich.Wenn Körper oder Bodenform flach sind (1), so wird die Aussenlösung durch eine Gleichung bestimmt, welche vergleichbar ist mit einer linearen Gleichung für Trägheitswellen. Lineare Lösungen werden für gleichförmige Bewegung von der Achse weg in einem unbegrenzten Bereich ) gegeben. Sie zeigen, dass die Oberflächenstromlinien orthogonal zu den Stromlinien sind, die bei rotationsfreier (nichtdrehender) Strömung über der gleichen Bodenform entstehen. Im Fernfeld ( z/L l) sind Störungen hauptsächlich auf ein keilförmiges Gebiet stromabwärts von der Rotationsachse ( ) begrenzt. In diesem Gebiet geht ihre Amplitude mit , in Uebereinstimmung mit Lighthill's Resultat, das mit der Gruppengeschwindigkeit hergeleitet wurde. Im keiförmigen Gebiet bestehen drei Familien von Lee-Wellen, welche sich mit unveränderter Stärke weit stromabwärts erstrecken. Ihre Wellenlängen gehören zur OrdnungLx/z, weshalb die Wellen im keilförmigen Bereich dicht gepackt erscheinen. Die Frage der Neigung der Taylor Säule behandelt und die Struktur des Randes vom keilförmigen Bereich wird analysiert.
This work is dedicated to Professor Nicholas Rott on the occasion of his sixtieth birthday. 相似文献
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12.
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13.
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16.
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17.
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18.
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19.
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20.
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