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Books on the topic 'Pulsar: generale'

Author: Grafiati

Published: 9 March 2023

Last updated: 31 July 2025

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1

Lyne, A. G. Pulsar astronomy. 2nd ed. Cambridge University Press, 1998.

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2

Lyne, A. G. Pulsar astronomy. Cambridge University Press, 1989.

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3

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

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4

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

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5

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

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6

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

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7

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

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8

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

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9

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

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10

1966-, Camilo Fernando, and Gaensler Bryan M, eds. 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. Published on behalf of the International Astronomical Union by Astronomical Society of the Pacific, 2004.

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11

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. The Society, 1996.

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12

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

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13

I, Owen David, and Lacheman Ernest René 1906-, eds. General studies. Eisenbrauns, 1995.

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14

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

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15

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. The Office, 1999.

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16

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. Institute of Electrical and Electronics Engineers, 1991.

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17

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. Institute of Electrical and Electronics Engineers, 1997.

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18

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

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19

I͡A, Ushakov V., ed. Impulse breakdown of liquids. Springer, 2007.

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20

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

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21

Baldacci, David. The escape. Grand Central Publishing, 2015.

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22

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

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23

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

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24

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

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25

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

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26

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

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27

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

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28

Graham-Smith, Francis, and Andrew G. Lyne. Pulsar Astronomy, 3rd Edition (Cambridge Astrophysics). 3rd ed. Cambridge University Press, 2006.

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29

Nordlund, Mark. Pulsar Pirates of Booty Moon: A Science Fiction Novel. Boohouse Books, 2024.

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30

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

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31

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

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32

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

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33

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,

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34

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

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35

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 pr

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36

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

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37

Fleming, Graham R., and 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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38

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 c

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39

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, GW15122

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40

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 a

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41

Cabrera Perramón, Jorge, and 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 d

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42

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

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43

Zinth, Wolfgang, Peter Gilch, and Markus Braun. Ultrashort Laser Pulses in Biology and Medicine. Springer London, Limited, 2008.

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44

Zinth, Wolfgang, Peter Gilch, and Markus Braun. Ultrashort Laser Pulses in Biology and Medicine. Springer, 2010.

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45

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

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46

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. D

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47

Estadísticas forestales 2004 Región del Maule (VII Región). INFOR, 2005. http://dx.doi.org/10.52904/20.500.12220/7835.

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Contenido: Principales indicadores forestales en la Región del Maule 2003-2004; Flujo total de productos forestales en la Industria Primaria VII RegiónCap.1. Indicadores macroeconómicosCap.2. Recurso forestal Uso del suelo, Superficie de Bosque Nativo por provincia y tipo forestal, Plantaciones, Disponibilidad futura de madera de plantaciones de pino radiata y eucalipto, número de viveros, incendios, producción de plantas por especie y comuna, incendios forestales, bonificaciones, poda- raleo, Áreas Silvestre ProtegidasCap.3. Consumo y Producción Trozas, Madera aserrada, Empresas Forestales, a

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48

Fowler, C. M., R. S. Caird, and D. J. Erickson. Megagauss Technology and Pulsed Power Applications. Springer, 1987.

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49

Wright, A. G. PMT background. Oxford University Press, 2017. http://dx.doi.org/10.1093/oso/9780199565092.003.0006.

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Photomultiplier (PMT) background derives from sources of photons, and from photoelectrons generation within a PMT. These may also act as a source of optical and radioactive background for neighbouring detectors. Dark count and dark current are reconciled by allowing for leakage currents flowing into the anode. The optimal gain setting follows from these considerations. Sources of background generated by the photocathode include thermionic emission; light generated within the PMT; gamma rays; muons and minimum ionizing particles (MIPs); insulator glow in the region of the anode; and residual ga

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50

Borovsky, A. V., A. L. Galkin, O. B. Shiryaev, and T. Auguste. Laser Physics at Relativistic Intensities. Springer, 2003.

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