Orbital stability

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1FOR RELEASE: 9:20 AM EST, January 7, 2002 ORBITAL STABILITY OF EARTH-LIKE PLANETS IN STELLAR HABITABLE ZONES Long-term orbital stability of Earth-like planets in stellar habitable zones is necessary for the evolution of

FOR RELEASE: 9:20 AM EST, January 7, 2002 ORBITAL STABILITY OF EARTH-LIKE PLANETS IN STELLAR HABITABLE ZONES Long-term orbital stability of Earth-like planets in stellar habitable zones is necessary for the evolution of

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Source URL: www.uta.edu

Language: English - Date: 2015-06-10 15:36:23
    2Transverse stability issues in Hamiltonian partial differential equations Nikolay Tzvetkov (University Cergy-Pontoise) The famous Korteweg- de Vries (KdV) equation ∂t u + u∂x u + ∂x3 u = 0 is a one dimensional asym

    Transverse stability issues in Hamiltonian partial differential equations Nikolay Tzvetkov (University Cergy-Pontoise) The famous Korteweg- de Vries (KdV) equation ∂t u + u∂x u + ∂x3 u = 0 is a one dimensional asym

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    Source URL: www.7ecm.de

    Language: English - Date: 2016-06-10 05:01:15
    3JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 116, E03010, doi:2010JE003652, 2011  Effects of orbital evolution on lunar ice stability Matthew A. Siegler,1 Bruce G. Bills,2 and David A. Paige1 Received 13 May 2010; revis

    JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 116, E03010, doi:2010JE003652, 2011 Effects of orbital evolution on lunar ice stability Matthew A. Siegler,1 Bruce G. Bills,2 and David A. Paige1 Received 13 May 2010; revis

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    Source URL: diviner.ucla.edu

    Language: English - Date: 2014-10-30 17:13:24
      4Stability of Nonlinear Systems By Guanrong Chen Department of Electronic Engineering City University of Hong Kong

      Stability of Nonlinear Systems By Guanrong Chen Department of Electronic Engineering City University of Hong Kong

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      Source URL: www.ee.cityu.edu.hk

      Language: English - Date: 2009-10-04 02:52:38
      5Orbital stability for NLS Jordan Bell  Department of Mathematics, University of Toronto April 3, 2014 Let n = 3, and take p < 43 . Some of the material we will present for general

      Orbital stability for NLS Jordan Bell Department of Mathematics, University of Toronto April 3, 2014 Let n = 3, and take p < 43 . Some of the material we will present for general

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      Source URL: individual.utoronto.ca

      Language: English - Date: 2014-04-03 12:52:33
      6J. Phys. Chem. B 2004, 108, 17337 Why Does Disubstituted Hexamolybdate with Arylimido Prefer to Form an Orthogonal Derivative? Analysis of Stability, Bonding Character, and Electronic Properties on

      J. Phys. Chem. B 2004, 108, 17337 Why Does Disubstituted Hexamolybdate with Arylimido Prefer to Form an Orthogonal Derivative? Analysis of Stability, Bonding Character, and Electronic Properties on

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      Source URL: yangtze.hku.hk

      Language: English - Date: 2010-12-19 08:35:07
      7J. Phys. Chem. B 2004, 108, [removed]17337 Why Does Disubstituted Hexamolybdate with Arylimido Prefer to Form an Orthogonal Derivative? Analysis of Stability, Bonding Character, and Electronic Properties on

      J. Phys. Chem. B 2004, 108, [removed]17337 Why Does Disubstituted Hexamolybdate with Arylimido Prefer to Form an Orthogonal Derivative? Analysis of Stability, Bonding Character, and Electronic Properties on

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      Source URL: yangtze.hku.hk

      Language: English - Date: 2010-12-19 08:35:07
      8NONLINEAR DYNAMICS AND SYSTEMS THEORY An International Journal of Research and Surveys Volume 1 Number 2

      NONLINEAR DYNAMICS AND SYSTEMS THEORY An International Journal of Research and Surveys Volume 1 Number 2

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      Source URL: www.e-ndst.kiev.ua

      Language: English - Date: 2011-02-12 10:22:22
      9DYNAMICS OF KDV SOLITONS IN THE PRESENCE OF A SLOWLY VARYING POTENTIAL JUSTIN HOLMER Abstract. We study the dynamics of solitons as solutions to the perturbed KdV (pKdV) equation ∂t u = −∂x (∂x2 u + 3u2 − bu),

      DYNAMICS OF KDV SOLITONS IN THE PRESENCE OF A SLOWLY VARYING POTENTIAL JUSTIN HOLMER Abstract. We study the dynamics of solitons as solutions to the perturbed KdV (pKdV) equation ∂t u = −∂x (∂x2 u + 3u2 − bu),

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      Source URL: www.math.brown.edu

      Language: English - Date: 2010-12-31 00:02:51
      10RESEARCH ARTICLE  The Origin of Chaos in the Outer Solar System N. Murray1 and M. Holman2 Classical analytic theories of the solar system indicate that it is stable, but

      RESEARCH ARTICLE The Origin of Chaos in the Outer Solar System N. Murray1 and M. Holman2 Classical analytic theories of the solar system indicate that it is stable, but

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      Source URL: www.cita.utoronto.ca

      Language: English - Date: 2000-06-14 12:17:18