13,136 research outputs found

    The Global Baroclinic Instability in Accretion Disks. II: Local Linear Analysis

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    This paper contains a local linear stability analysis for accretion disks under the influence of a global radial entropy gradient beta = - d log T / d log r for constant surface density. Numerical simulations suggested the existence of an instability in two- and three-dimensional models of the solar nebula. The present paper tries to clarify, quantify, and explain such a global baroclinic instability for two-dimensional flat accretion disk models. As a result linear theory predicts a transient linear instability that will amplify perturbations only for a limited time or up to a certain finite amplification. This can be understood as a result of the growth time of the instability being longer than the shear time which destroys the modes which are able to grow. So only non-linear effects can lead to a relevant amplification. Nevertheless, a lower limit on the entropy gradient ~beta = 0.22 for the transient linear instability is derived, which can be tested in future non-linear simulations. This would help to explain the observed instability in numerical simulations as an ultimate result of the transient linear instability, i.e. the Global Baroclinic Instability.Comment: 35 pages, 11 figures; ApJ in pres

    Surface properties of ocean fronts

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    Background information on oceanic fronts is presented and the results of several models which were developed to study the dynamics of oceanic fronts and their effects on various surface properties are described. The details of the four numerical models used in these studies are given in separate appendices which contain all of the physical equations, program documentation and running instructions for the models

    Issues for further study

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    The topics covered include the following: a lunar outpost map, lunar resource utilization, asteroid resource utilization, space energy utilization, and space 'real estate' utilization

    Low-field microwave absorption in epitaxial La-Sr-Mn-O films resulting from the angle-tuned ferromagnetic resonance in the multidomain state

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    We studied magnetic-field induced microwave absorption in 100-200 nm thick La0.7_{0.7}Sr0.3_{0.3}MnO3_{3} films on SrTiO3_{3} substrate and found a low-field absorption with a very peculiar angular dependence: it appears only in the oblique field and is absent both in the parallel and in the perpendicular orientations. We demonstrate that this low-field absorption results from the ferromagnetic resonance in the multidomain state (domain-mode resonance). Its unusual angular dependence arises from the interplay between the parallel component of the magnetic field that drives the film into multidomain state and the perpendicular field component that controls the domain width through its effect on domain wall energy. The low-field microwave absorption in the multidomain state can be a tool to probe domain structure in magnetic films with in-plane magnetization.Comment: 9 pages, 9 Figure

    Rational invariants of even ternary forms under the orthogonal group

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    In this article we determine a generating set of rational invariants of minimal cardinality for the action of the orthogonal group O3\mathrm{O}_3 on the space R[x,y,z]2d\mathbb{R}[x,y,z]_{2d} of ternary forms of even degree 2d2d. The construction relies on two key ingredients: On one hand, the Slice Lemma allows us to reduce the problem to dermining the invariants for the action on a subspace of the finite subgroup B3\mathrm{B}_3 of signed permutations. On the other hand, our construction relies in a fundamental way on specific bases of harmonic polynomials. These bases provide maps with prescribed B3\mathrm{B}_3-equivariance properties. Our explicit construction of these bases should be relevant well beyond the scope of this paper. The expression of the B3\mathrm{B}_3-invariants can then be given in a compact form as the composition of two equivariant maps. Instead of providing (cumbersome) explicit expressions for the O3\mathrm{O}_3-invariants, we provide efficient algorithms for their evaluation and rewriting. We also use the constructed B3\mathrm{B}_3-invariants to determine the O3\mathrm{O}_3-orbit locus and provide an algorithm for the inverse problem of finding an element in R[x,y,z]2d\mathbb{R}[x,y,z]_{2d} with prescribed values for its invariants. These are the computational issues relevant in brain imaging.Comment: v3 Changes: Reworked presentation of Neuroimaging application, refinement of Definition 3.1. To appear in "Foundations of Computational Mathematics
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