3 edition of Self-modulational formation of pulsar microstructures found in the catalog.
Self-modulational formation of pulsar microstructures
1983 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
|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. Self-modulational formation of pulsar microstructures book and C.
Kennel. Principles of Pulse Code Modulation Hardcover – January 1, by Kenneth W. Cattermole (Author) › Visit Amazon's Kenneth W. Cattermole Page.
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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 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.
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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,  .
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.
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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. 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: 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.
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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. The universe contains many strange and wonderful astronomical phenomena, and pulsars are extraordinary in many ways.
This essay will examine pulsars, including their formation, general characteristics, modern theories about pulsars, and the discovery of the unique characteristics of a millisecond pulsar.
Pulsar Properties For additional information about pulsars, see the books Pulsar Astronomy by Andrew Lyne and Francis Graham-Smith and Handbook 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. the pulsar age contraryto reports in the past. The absence of a correlation with age in this large sample of pulsars with drifting subpulses (90) suggests that if such a cor-relation would exist, it must be a very weak correlation.
Also, the evidence for a pulsar sub-population located close to the P3 =2P0 Nyquist limit (Wright , Rankin [9. pulsar novation We are a team of graduates in mathematics, computer science, electronic and electrical engineering. We develop applications for the iOS and Mac OSX.
Pulsar Headquarters Superior Ave. Cleveland, OH USA [email protected] Pulsar Asia, LTD 广州市天河区天源路长 工业区13栋室. Pulsars are rapidly rotating neutron stars A neutron star is all that remains of the core of large stars within a certain mass range, when those stars end their lives in a supernova explosion. If the remnant of a dead star is left with less than about solar masses then it becomes a white dwarf, and if it is left with more than about 5 solar masses it becomes a black hole.
Pulsar is a network fuzzer with automatic protocol learning and simulation capabilites. The tool allows to model a protocol through machine learning techniques, such as clustering and hidden Markov models. Abraham C.-L Chian has written: 'Self-modulational formation of pulsar microstructures' -- subject(s): Radio emission, Pulsars, Space plasmas, Pulse modulation Asked in Travel & Places.Astronomers can measure the spin period (P) of a pulsar to such high accuracy that the rate of change of the period can usually be determined with a year or so of observations.
Knowing the period and its rate of change (dP/dt) allows us to infer the magnetic field strength (B) of the pulsar since the only significant source of energy loss is the magnetic dipole radiation.the speci cities of pulsar candidate classi cation.
We attach particular importance on how to properly represent pulsar candidates as vectors of real-valued inputs (or features) to the algorithm.
A detailed understanding of the entire pulsar searching process is helpful, if Cited by: 1.