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Livres sur le sujet « Pulsar: generale »

Auteur : Grafiati

Publié le 9 mars 2023

Mis à jour le 10 mars 2023

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1

Lyne, A. G. Pulsar astronomy. 2^e éd. Cambridge : Cambridge University Press, 1998.

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2

1923-, Graham-Smith Francis Sir, dir. Pulsar astronomy. 3^e éd. Cambridge : Cambridge University Press, 2006.

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3

Lyne, A. G. Pulsar astronomy. Cambridge [England] : Cambridge University Press, 1989.

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4

Venancio Pulgar : Autonomía e identidad del Zulia. Zulia : Universidad del Zulia, Ediciones del Vice Rectorado Académico, 2008.

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5

Marquand, John P. H.M. Pulham, Esquire. Chicago : Academy Chicago Publishers, 1986.

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6

Francisco Martínez de la Rosa. Hernán Pérez del Pulgar, el de las hazañas. Granada [Spain] : Caja General de Ahorros de Granada, 1991.

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7

Śekhāvata, Sumana. Pulisa praśāsana : Rājasthāna Pulisa Mahānideśaka Kāryālaya ke sandarbha meṃ. Jodhapura : Mahārājā Mānasiṃha Pustaka Prakāśa Śodha Kendra, 2009.

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8

Śekhāvata, Sumana. Pulisa praśāsana : Rājasthāna Pulisa Mahānideśaka Kāryālaya ke sandarbha meṃ. Jodhapura : Mahārājā Mānasiṃha Pustaka Prakāśa Śodha Kendra, 2009.

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9

Śekhāvata, Sumana. Pulisa praśāsana : Rājasthāna Pulisa Mahānideśaka Kāryālaya ke sandarbha meṃ. Jodhapura : Mahārājā Mānasiṃha Pustaka Prakāśa Śodha Kendra, 2009.

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10

Śekhāvata, Sumana. Pulisa praśāsana : Rājasthāna Pulisa Mahānideśaka Kāryālaya ke sandarbha meṃ. Jodhapura : Mahārājā Mānasiṃha Pustaka Prakāśa Śodha Kendra, 2009.

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11

1967-, Arzoumanian Zaven, Hooft F. van der et Heuvel, Edward Peter Jacobus van den, 1940-, dir. Pulsar timing, general relativity, and the internal structure of neutron stars : Proceedings of the colloquium, Amsterdam, 24-27 September 1996. Amsterdam : Royal Netherlands Academy of Arts and Sciences, 1999.

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12

A, Freeman Kerry, et Chilton Book Company, dir. Chilton Book Company repair manual. : All U.S. and Canadian models of F10, 310, Stanza, Pulsar. Radnor, Pa : Chilton Book Co., 1989.

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13

Vorhees, Duance. The woodcutter and the heavenly maiden = : Sŏnnyŏ wa namukkun ; The firedogs = Pulgae. Elizabeth, NJ, U.S.A : Hollym, 1990.

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14

1966-, Camilo Fernando, et Gaensler Bryan M, dir. Young neutron stars and their environments : Proceedings of the 218th Symposium of the International Astronomical Union held during the IAU General Assembly XXV, Sydney, Australia, 14-17 July 2003. San Francisco, Calif : Published on behalf of the International Astronomical Union by Astronomical Society of the Pacific, 2004.

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15

Ultrafast Phenomena Topical Meeting (1996 San Diego, Calif.). Ultrafast phenomena : Summaries of the papers presented at the Topical Meeting, May 28-June 1, 1996, San Diego, California. Washington, D.C : The Society, 1996.

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16

I, Owen David, et Lacheman Ernest René 1906-, dir. General studies. Winona Lake, Ind : Eisenbrauns, 1995.

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17

La giustizia secondo Maria : Pola 1947 : la donna che sparò al generale brigadiere Robert W. De Winton. Udine : Del Bianco, 2008.

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18

Ultrashort laser pulses in biology and medicine. Berlin : Springer, 2008.

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19

International, Conference on Megagauss Magnetic Field Generation and Related Topics (4th 1986 Santa Fe N. M. ). Megagauss technology and pulsed power applications. New York : Plenum Press, 1987.

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20

V, Borovskiĭ A., dir. Laser physics at relativistic intensities. New York : Springer, 2003.

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21

Se mo she zhen. Shanghai : Shanghai ke xue ji shu chu ban she, 1987.

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22

Office, General Accounting. Terrorism and drug trafficking : Testing status and views on operational viability of pulsed fast neutron analysis technology : report to the Subcommittee on Treasury and General Government, Committee on Appropriations, U.S. Senate. Washington, D.C. (P.O. Box 37050, Washington, D.C. 20013) : The Office, 1999.

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23

Engineers, Institute Of Electrical and Electronics. IEEE standard methods and equipment for measuring the transmission characteristics of pulse-code modulation (PCM) telecommunications circuits and systems. New York, NY, USA : Institute of Electrical and Electronics Engineers, 1991.

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24

Antonio, Cantoni, et Teo K. L, dir. Filter design with time domain mask constraints : Theory and applications. Dordrecht : Kluwer Academic Publishers, 2001.

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25

IEEE, International Pulsed Power Conference (11th 1997 Baltimore Md ). 11th IEEE International Pulsed Power Conference : Digest of technical papers, Hyatt Regency Baltimore on the Inner Harbor, Baltimore, Maryland, USA, June 29-July 2, 1997. [New York] : Institute of Electrical and Electronics Engineers, 1997.

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26

I͡A, Ushakov V., dir. Impulse breakdown of liquids. Berlin : Springer, 2007.

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27

Kratz, Robert. Principles of pulsed magnet design. Berlin : Springer, 2002.

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28

Graham-Smith, Francis, et Andrew Lyne. Pulsar Astronomy. Cambridge University Press, 2012.

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29

Graham-Smith, Francis, et Andrew Lyne. Pulsar Astronomy. Cambridge University Press, 2012.

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30

Graham-Smith, Francis, et Andrew Lyne. Pulsar Astronomy. Cambridge University Press, 2012.

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31

Graham-Smith, Francis, et Andrew Lyne. Pulsar Astronomy. Cambridge University Press, 2012.

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32

Stappers, Benjamin, Francis Graham-Smith et Andrew Lyne. Pulsar Astronomy. Cambridge University Press, 2022.

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33

Stappers, Benjamin, Francis Graham-Smith et Andrew Lyne. Pulsar Astronomy. Cambridge University Press, 2022.

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34

Graham-Smith, Francis, et Andrew G. Lyne. Pulsar Astronomy, 3rd Edition (Cambridge Astrophysics). 3^e éd. Cambridge University Press, 2006.

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35

Lorimer, D. R., et M. Kramer. Handbook of Pulsar Astronomy (Cambridge Observing Handbooks for Research Astronomers). Cambridge University Press, 2004.

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36

Marquand, John P. H. M. Pulham, Esquire : A Novel. Open Road Integrated Media, Inc., 2015.

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37

Marquand, John P. H. M. Pulham, Esquire : A Novel. Open Road Integrated Media, Inc., 2018.

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38

Wright, A. G. Electronics for PMTs. Oxford University Press, 2017. http://dx.doi.org/10.1093/oso/9780199565092.003.0014.

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Photomultipliers (PMTs) are current generators characterized by high gain, wide bandwidth, and high-output impedance. The role of preamplifiers and amplifiers is generally one of conditioning the PMT output. Either the time signature is preserved using a fast voltage preamplifier, or a voltage proportional to the charge in each event is generated with a charge-sensitive preamplifier. Both preamplifier types are generally of low-output impedance, suitable for driving matched coaxial cable. Preamplifiers and amplifiers are available as modular units (e.g. nuclear instrument module), stand alone, or are incorporated in a module including the PMT. Shaping amplifiers are used to further condition preamplifier signals, using integrating and differentiating circuits—particularly relevant to scintillation spectrometers. Discrete-component amplifiers and current-feedback operational amplifiers serve fast applications. Digital signal processing has overtaken many of the classical electronic techniques involving resolution and in pulse shape discrimination. Electronic circuitry for generating fast LED pulses is discussed.

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39

Wright, A. G. Signal-induced background. Oxford University Press, 2017. http://dx.doi.org/10.1093/oso/9780199565092.003.0011.

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Signal-induced background has a time dependence that distinguishes it from the sources discussed in Chapter 6. These events refer to a progression in which a signal generates a subsequent one, correlated in time to the initial detection. The timescale for correlated background ranges from nanoseconds to days. The earliest signal is a prepulse generated by a photon incident on d1. Late pulses relate to the k-to-d1, and k-to-anode transit time. The next category, the afterpulses, spans ~100 ns to 10 μ‎s, with a peaked time distribution. There is a long-lived source of photons, extending to days and caused by exposure of a photomultiplier to bright light or to nuclear radiation. Afterpulses contribute to the slope of a photon-counting plateau characteristic, distort fluorescent decay, and pulse shape discrimination measurements. They also affect resolution, and processes of a statistical nature.

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40

Wright, A. G. Linear performance. Oxford University Press, 2017. http://dx.doi.org/10.1093/oso/9780199565092.003.0009.

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This chapter is concerned with a single consideration: the degree of proportionality between a light signal and its resulting electrical output. This is formally referred to as linearity, which depends on the suitability of the chosen PMT and the mode of operation (pulsed or analogue). Applications fall into two groups: analogue operation (DC) and transient applications. Linearity in a pulsed mode of operation concerns both pulse height (charge) and the rate of events. Generally, in the DC mode, only the mean anode current is relevant. Methods for determining both forms of non-linearity are presented, based on actual measurements. Test methods using multiple light sources, bootstrapping, single step (piggyback), and shot noise are investigated. A method for uncovering non-linearity in high-Z scintillators by using coincident gamma emissions (60Co) is demonstrated. An analytical means for correcting results at the 1 % level is provided.

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41

Sr, Aguayo Erick. Canito y la Pandilla de Pulgas Llamada Cáncer. Ochoa, Miguel, 2022.

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42

Editors, The Nichols/Chilton. Chilton's Repair Manual Datsun/Nissan F10, 310, Stanza, Pulsar 1976-88 (Chilton's Repair Manual (Model Specific)). Chilton Book Company, 1989.

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43

TENS-like devices. Oxford University Press, 2014. http://dx.doi.org/10.1093/med/9780199673278.003.0011.

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TENS-like devices deliver electrical currents across the intact surface of the skin using pulse generators with technical output specifications that differ from a standard TENS device. Technological advances have resulted in reductions in the size and cost of electrotherapeutic devices with increasing varieties of self-administered hand-held TENS-like devices available to practitioners and the general public. The diversity of TENS-like devices available on the market makes synthesizing evidence difficult. The purpose of this chapter is to categorize TENS-like devices and briefly overview the characteristics, mechanism of action, and effectiveness of various TENS-like devices. The chapter covers high-voltage pulsed (Galvanic) current, microcurrent electrical therapy, low-intensity transcutaneous cranial electrical stimulation, transcutaneous spinal electroanalgesia, transcutaneous piezoelectric current, non-invasive interactive neurostimulation, action potential simulation and H-wave therapy, and transcutaneous electrical acupoint stimulation.

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44

Fleming, Graham R., et Anthony E. Siegman. Ultrafast Phenomena V : Proceedings of the Fifth OSA Topical Meeting Snowmass, Colorado, June 16-19 1986. Springer Berlin / Heidelberg, 2014.

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45

(Editor), A. E. Siegman, dir. Ultrafast Phenomena V. Springer, 1987.

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46

Maggiore, Michele. Gravitational Waves. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198570899.001.0001.

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A comprehensive and detailed account of the physics of gravitational waves and their role in astrophysics and cosmology. The part on astrophysical sources of gravitational waves includes chapters on GWs from supernovae, neutron stars (neutron star normal modes, CFS instability, r-modes), black-hole perturbation theory (Regge-Wheeler and Zerilli equations, Teukoslky equation for rotating BHs, quasi-normal modes) coalescing compact binaries (effective one-body formalism, numerical relativity), discovery of gravitational waves at the advanced LIGO interferometers (discoveries of GW150914, GW151226, tests of general relativity, astrophysical implications), supermassive black holes (supermassive black-hole binaries, EMRI, relevance for LISA and pulsar timing arrays). The part on gravitational waves and cosmology include discussions of FRW cosmology, cosmological perturbation theory (helicity decomposition, scalar and tensor perturbations, Bardeen variables, power spectra, transfer functions for scalar and tensor modes), the effects of GWs on the Cosmic Microwave Background (ISW effect, CMB polarization, E and B modes), inflation (amplification of vacuum fluctuations, quantum fields in curved space, generation of scalar and tensor perturbations, Mukhanov-Sasaki equation,reheating, preheating), stochastic backgrounds of cosmological origin (phase transitions, cosmic strings, alternatives to inflation, bounds on primordial GWs) and search of stochastic backgrounds with Pulsar Timing Arrays (PTA).

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47

Wright, A. G. Secondary emission and gain. Oxford University Press, 2017. http://dx.doi.org/10.1093/oso/9780199565092.003.0005.

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Secondary-electron emission generates gain in conventional vacuum photomultipliers with discrete dynodes. This is a cascade process involving between 6 and 20 elements. Generally, the higher the number of stages, the higher is the gain and similarly for applied voltage. Gain is dependent on the composition of the dynodes, with SbCs and activated BeO being the most common materials. There are ten different dynode types, each of which serves a particular purpose: for example, operation in high magnetic fields and high temperature. The continuous channel dynode is available as a single unit and as a multichannel structure, the microchannel plate. The quality of a dynode system is described by its single-electron response. Discrete dynodes produce a spread in output size whereas the channel devices are generally operated in saturation. Gain may be quoted as DC, G, and pulsed ‹g› and methods for measuring these parameters are given.

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48

Cabrera Perramón, Jorge, et Ignacio Cerda V. Precios de productos forestales chilenos (actualizados al primer semestre de 1991). INFOR : CORFO, 1991. http://dx.doi.org/10.52904/20.500.12220/6342.

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Durante el primer semestre de 1991 los precios de los productos forestales tradicionales que se transan en el mercado interno presentaron una tendencia al alza, derivado de un conjunto de factores en que predominan la cierta escasez relativa de trozas de diámetros mayores, una mayor demanda por parte de nueva capacidad instalada y por una mayor actividad que se genera en el sector de la construcción. En tanto, los precios de exportación de los principales productos forestales chilenos mostraron una tendencia en general estable, con excepción de la pulpa blanqueada y semiblanqueada, lo que se debe a una mayor competitividad en los mercados, originados por mayores cantidades ofrecidas.

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49

America, Optical Society Of. Ultrafast Phenomena (Technical Digest Series). Optical Society of America, 1996.

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50

Wright, A. G. Voltage dividers. Oxford University Press, 2017. http://dx.doi.org/10.1093/oso/9780199565092.003.0013.

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Voltage dividers provide accelerating voltages to generate multiplier gain. Dynode voltages must remain constant and independent of the light input to maintain stable gain. The standard resistive divider never quite satisfies this requirement, although acceptable performance can be achieved by careful design. The inclusion of zener diodes improves performance but field-effect transistor (FET) circuits can provide gain stability at high mean anode currents, regardless of whether the application is pulsed or analogue. Design procedures for active and semi-active voltage dividers are presented. Dividers based on the Cockcroft–Walton (CW) principle are particularly suited to portable instrumentation because of their low standing current. Consideration is given to pulsed operation, decoupling, switch-on transients, ripple, dynode signals, single cable dividers, and equivalent circuits at high frequencies. Gating is used to protect a photomultiplier, in the presence of high light levels, by reducing the gain electronically. Various methods for gating a voltage divider are presented.

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