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3 edition of Self-modulational formation of pulsar microstructures found in the catalog.

Self-modulational formation of pulsar microstructures

Self-modulational formation of pulsar microstructures

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Published by Ministerio da Ciència e Tecnologia, Instituto de Pesquisas Espaciais, National Aeronautics and Space Administration, National Technical Information Service, distributor in São José dos Campos, Brazil, [Washington, D.C, Springfield, Va .
Written in English

    Subjects:
  • Pulsars.,
  • Pulse modulation.,
  • Radio emission.,
  • Space plasmas.

  • Edition Notes

    Statementby A.C.-L. Chian and C.F. Kennel.
    SeriesNASA contractor report -- NASA CR-182420
    ContributionsKennel, Charles F., 1939-., United States. National Aeronautics and Space Administration.
    The Physical Object
    FormatMicroform
    Pagination1 v.
    ID Numbers
    Open LibraryOL17118421M

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Self-modulational formation of pulsar microstructures Download PDF EPUB FB2

The nonlinearities arising from wave intensity induced particle mass variation may excite the modulational instability of circularly and linearly polarized pulsar radiation.

The resulting wave envelopes can take the form of periodic wave trains or solitons. These nonlinear stationary waveforms may account for the formation of pulsar by: These nonlinear stationary waveforms may account for the formation of pulsar microstructures.

The authors discuss a nonlinear plasma theory for self-modulation of pulsar radio pulses. A nonlinear Schödinger equation is derived for strong electromagnetic waves propagating in Cited by: Get this from a library. Self-modulational formation of pulsar microstructures.

[Abraham C -L Chian; Charles F Kennel; United States. National Aeronautics and Space Administration.]. A nonlinear plasma theory for self-modulation of pulsar radio pulses is discussed.

A nonlinear Schroedinger equation is derived for strong electromagnetic waves propagating in an electron-positron : A. C.-L. Chian and C. Kennel. Principles of Pulse Code Modulation Hardcover – January 1, by Kenneth W. Cattermole (Author) › Visit Amazon's Kenneth W. Cattermole Page.

Find all the books, read about the author, and more. See search results for this author. Are you an author. Cited by: The nonlinearities arising from wave-intensity-induced particle-mass variation may excite the modulational Self-modulational formation of pulsar microstructures book of circularly and linearly polarized pulsar radiation.

The resulting wave envelopes can take the form of periodic wave trains or solitons. These nonlinear stationary waveforms may account for the formation of pulsar microstructures. SELF-MODULATIONAL FORMATION OF PULSAR MICROSTRUCTURES by A.C.-L.

Chian* and C.F. Kennel institute of Geophysics and Planetary Physic' University of California, Los Angeles Los Angeles, CAUSA PPG May, * Permanent address: Institute for Space Research (INPE/CNPq), C.P.So Jose dos Campos, SP, Brazil. Books A - Z; Journals A - Z; Videos; Librarians; Browse Volumes & Issues.

Astrophysics and Space Science. All Volumes & Issues. Self-modulational formation of pulsar microstructures. Chian, C. Kennel Pages OriginalPaper. Singposts of shock waves in the metagalactic medium. Temporal Variation of Pulsar Dispersion Measure These nonlinear stationary waveforms may account for the formation of pulsar microstructures.

Self-modulational formation of pulsar. PULSAR PROJECT. Alien Technical Research - 25A. Westchester Camp. Office of Central Research #3. CODE: ARAMIS V - ADRAT. The following document is a continuation of the Blue Planet Project, and again, is believed to be the personal notes and scientific dairy of a scientist who was.

A nonlinear theory is discussed for self-modulation of pulsar radio pulses. A nonlinear Schroedinger equation is derived for strong electromagnetic waves propagating in an electron-positron plasma. The nonlinearities arising from wave intensity induced relativistic particle mass variation may excite the modulational instability of circularly and linearly polarized pulsar radiation.

Pulsar multifunction spectroscopy service pairs multiple detectors with a high-output pulsed neutron generator to provide stand-alone cased hole formation evaluation and reservoir saturation monitoring—all with a single tool. The result is comprehensive reservoir rock and fluid content data that is comparable to data acquired during openhole.

Our results may contribute to improve the understanding of physical processes in pair plasmas such as the formation and evolution of pulsar microstructures [1,[32] [33] [34][35][36].

Your personal data will be used to support your experience throughout this website, to manage access to your account, and for other purposes described in our privacy policy.

Operator’s Manual Model # PS Arch Chemicals, Inc. Lower River Road P.O. Box Box Charleston, TN PULSAR 11/30/00File Size: KB. Self-modulational formation of pulsar microstructures: Solar system plasma physics: Unstable growth of unducted whistlers propagating at an angle to the geomagnetic field.

Explore RCC Remote Control Wireless Remote Control The Pulsar RCC Wireless Remote Control is designed to control remotely device's selected functions and to navigate its menu. Explore C-Clamp Mount Pulsar Accessories The Pulsar C-Clamp is designed for fixing Pulsar units equipped with a 1/4" tripod mount on various elements (crossbeam, handrail.

A nonlinear model of modulational processes in the subsonic regime involving a linearly unstable wave and two linearly damped waves with different damping rates in a plasma is studied numerically. We compute the maximum Lyapunov exponent as a function of the damping rates in a two-parameter space, and identify shrimp-shaped self-similar structures in the parameter by: 2.

An artistic impression showing the formation of the double pulsar system. After the supernova explosion of the more massive star and the formation of a pulsar, the companion evolves and becomes a. Electromagnetic pulses in a strongly magnetized electron-positron plasma.

Electromagnetic pulses in a strongly magnetized electron-positron plasma. Yu MY, Rao NN. Physical review. A Self-modulational formation of pulsar microstructures. Chian. Astrophysics and Cited by: 2. Chian and Kennel () showed that the nonlinearities arising in a model for strong electromagnetic waves propagating in an electron–positron plasma may excite the modulational instability of pulsar radiation, resulting in periodic wave trains or solitons which may account for the formation of pulsar by: In particular the supersonic Langmuir turbulence can operate in two regimes: (1) the electrostatic supersonic modulational instability is excited when W > y.

and feoAo W > y^^k^o and feo-^o > I1' These two supersonic regimes are char- acterized by the excitation of non-resonant ion-acous- tic waves such Cited by: 8.Wave propagation in a cold, collisionless, two-component plasma is analyzed by considering, first, the frame of reference in which the field has no space dependence, and then applying a Lorentz transformation to obtain a wave whose space-time dependence is a function of t — nz / c only, where n is a constant.

Exact (nonlinear, relativistic) results for known special cases, and some others Cited by: