Self-modulational formation of pulsar microstructures
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Ministerio da Ciència e Tecnologia, Instituto de Pesquisas Espaciais, National Aeronautics and Space Administration, National Technical Information Service, distributor , São José dos Campos, Brazil, [Washington, D.C, Springfield, Va
Pulsars., Pulse modulation., Radio emission., Space pla
|Statement||by A.C.-L. Chian and C.F. Kennel.|
|Series||NASA contractor report -- NASA CR-182420|
|Contributions||Kennel, Charles F., 1939-., United States. National Aeronautics and Space Administration.|
|The Physical Object|
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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 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 microstructures. SELF-MODULATIONAL FORMATION OF PULSAR MICROSTRUCTURES by A.C.-L.
Chian* and C.F. Kennel institute Self-modulational formation of pulsar microstructures book 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,  .
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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.
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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.
Details Self-modulational formation of pulsar microstructures PDF
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.
Description Self-modulational formation of pulsar microstructures PDF
Exact (nonlinear, relativistic) results for known special cases, and some others Cited by: Mounting Options. This page illustrates the differences between wall mount, fascia mount, panel mount and rack mount. It also shows the standard size Blackbox and the larger Blackbox units.
Wall Mount - IP A complete built-in enclosure (wall mounted). The IP65 rating makes it ideal for use in outdoor harsh weather conditions. Pulsar Properties For additional information about pulsars, see the books P ulsar Astronomy by Andrew Lyne and Francis Graham-Smith and H andbook of Pulsar Astronomy by Duncan Lorimer and Michael Kramer.
Known radio pulsars appear to emit short pulses of radio radiation with pulse periods between ms and seconds. Formation: The formation of a pulsar is very similar to the creation of a neutron star.
When a massive star with 4 to 8 times the mass of our Sun dies, it detonates as a supernova. PULSAR® Universal Test System The PULSAR test set includes a ROM-resident computer program.
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PULSAR Manual 3 The PULSAR project is an Australian training and research project funded by the Victorian State Government’s Mental Illness Research Fund (MIRF).
PULSAR is based on the Refocus program from the UK. This project is testing a practical approach to address the vital issue of how different types of services.A plasma antenna is provided having an ionizer, which when energized, generates a bounded or unbounded plasma column extending along a vertical axis.
When ionization is initiated, the difference in the diffusion characteristics of ions and electrons and the resulting gas plasma produce a current pulse in a first direction. As the plasma extinguishes, the difference in relaxation times for the Cited by: Abraham C.-L Chian has written: 'Self-modulational formation of pulsar microstructures' -- subject(s): Radio emission, Pulsars, Space plasmas, Pulse modulation Asked in .
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