WorldCat Identities

Manchester, Richard N.

Overview
Works: 18 works in 41 publications in 2 languages and 816 library holdings
Genres: Conference papers and proceedings  Music  Songs and music  Electronica (Music)  Folk-rock music  Periodicals  Academic theses 
Roles: Author, Honoree
Classifications: QB843.P8, 523
Publication Timeline
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Most widely held works about Richard N Manchester
 
Most widely held works by Richard N Manchester
Pulsars by Richard N Manchester( Book )

12 editions published between 1971 and 1977 in English and Undetermined and held by 677 WorldCat member libraries worldwide

Accurate flux densities at 5009 MHz of 753 radio sources by A. J Shimmins( Book )

1 edition published in 1969 in English and held by 9 WorldCat member libraries worldwide

Sound image : a magazine of aural and visual art. Number 1( Recording )

2 editions published in 1975 and held by 4 WorldCat member libraries worldwide

Observations of pulsar polarization at 410 and 1665 MHz by Richard N Manchester( Book )

2 editions published in 1971 in English and held by 3 WorldCat member libraries worldwide

Publications of the Astronomical Society of Australia : [Volume 20, 2003]( )

1 edition published in 2003 in English and held by 2 WorldCat member libraries worldwide

Gamma-Ray and Radio Observations of PSR B1509-58( Book )

2 editions published in 1993 in English and held by 2 WorldCat member libraries worldwide

We report concurrent radio and gamma-ray observations of PSR B1509-58 carried out by the Parkes Radio Telescope and by the Burst and Transient Source Experiment (BATSE) and the Oriented Scintillation Spectrometer Experiment (OSSE) on the Compton Gamma Ray Observatory (CGRO-Gamma-ray light curves fitted at several energies between ~ 20-500 keV yield a phase offset with respect to the radio pulse that is independent of energy, with an average value 0.32 plus or minus 0.02. Although this value is larger by 0.07 than that reported by Kawai et al., the difference is not statistically significant (only~2 sigma) when account is taken of the uncertainty associated with their result. We briefly discuss the possibility that the energy-independence of the gamma-ray pulse phase is a signature of non-thermal radiation in the X-ray/gamma-ray range and the suggestion of a dependence of pulsar radio-gamma-ray phase offset on pulse period
Accurate flux densities at 5009 MHz of 753 radio sources by A. J Shimmins( Book )

1 edition published in 1969 in English and held by 2 WorldCat member libraries worldwide

Propagation of pcl micropulsations in an ionospheric duct( Book )

1 edition published in 1966 in English and held by 1 WorldCat member library worldwide

The propagation mechanism of Pc1 micropulsations from their relatively high generation latitude to middle and low latitudes is considered. The study is confined to the type of micropulsations commonly known as pearls or hm emissions. It is shown that propagation probably takes place in a duct centred on the F region of the ionosphere. The diurnal variations of the duct properties are calculated, using typical profiles for the ionospheric parameters at the time of sunspot minimum. It is shown that the duct has a low frequency cutoff at about 0.5 c/s, implying that the lack of low frequency events at middle latitudes may be largely a propagation effect. Duct attenuation is very small during the night hours when the majority of Pc1 events are observed at middle latitudes, but is very large during the day. The calculated average horizontal component of the phase velocity for propagation in the duct is of the same order as that given in initial reports of experimental observations. (Author)
Propagation of pc1 geomagnetic micropulsations in the magnetosphere and the ionosphere( Book )

1 edition published in 1968 in English and held by 1 WorldCat member library worldwide

The report details original equipment for continuously recording Pc1 geomagnetic micropulsations on magnetic tape with timing accuracy of less than 0.1 second. Analysis of the records is carried out by using both frequency-time and amplitude-time techniques. An extensive study of temporal variations in Pc1 in relation to propagation in the magnetosphere is detailed. Signals are generated in the lambda = 4.5 - 9.5 region of the magnetosphere and show diurnal and geomagnetic disturbance variations. The theoretical problem of north-south propagation of Pc1 signals in an ionospheric duct is treated. Comparison with experimental results show that wave group velocities in the duct vary from 400 to 800 km/sec, depending on the electron concentration in the duct and hence local time. (Author)
Accurate flux densities at 5009 MHz of 753 radio sources by A. J Shimmins( Book )

1 edition published in 1969 in English and held by 1 WorldCat member library worldwide

Accurate flux densities at 5009 MHZ of 753 radio sources [by] A.J. Shimmins, R.N. Manchester and Beverley J. Harris by A. J Shimmins( Book )

1 edition published in 1969 in English and held by 1 WorldCat member library worldwide

An investigation of the propagation of hydromagnetic emissions away from their generation latitude to both high and low latitudes by Richard N Manchester( )

1 edition published in 1968 in English and held by 1 WorldCat member library worldwide

Dating supernova remnants by Richard N Manchester( Book )

1 edition published in 1992 in Undetermined and held by 1 WorldCat member library worldwide

Pulʹsary by Richard N Manchester( Book )

1 edition published in 1980 in Russian and held by 1 WorldCat member library worldwide

Wide-band profile domain pulsar timing analysis( )

1 edition published in 2016 in English and held by 1 WorldCat member library worldwide

Abstract We extend profile domain pulsar timing to incorporate wide-band effects such as frequency-dependent profile evolution and broad-band shape variation in the pulse profile. We also incorporate models for temporal variations in both pulse width and in the separation in phase of the main pulse and interpulse. We perform the analysis with both nested sampling and Hamiltonian Monte Carlo methods. In the latter case, we introduce a new parametrization of the posterior that is extremely efficient in the low signal-to-noise regime and can be readily applied to a wide range of scientific problems. We apply this methodology to a series of simulations, and to between seven and nine years of observations for PSRs J1713+0747, J1744−1134 and J1909−3744 with frequency coverage that spans 700–3600Mhz. We use a smooth model for profile evolution across the full frequency range, and compare smooth and piecewise models for the temporal variations in dispersion measure (DM). We find that the profile domain framework consistently results in improved timing precision compared to the standard analysis paradigm by as much as 40percent for timing parameters. Incorporating smoothness in the DM variations into the model further improves timing precision by as much as 30percent. For PSR J1713+0747, we also detect pulse shape variation uncorrelated between epochs, which we attribute to variation intrinsic to the pulsar at a level consistent with previously published analyses. Not accounting for this shape variation biases the measured arrival times at the level of ∼30ns, the same order of magnitude as the expected shift due to gravitational waves in the pulsar timing band
Observational properties of pulsars by Richard N Manchester( Book )

1 edition published in 2004 in English and held by 1 WorldCat member library worldwide

 
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Alternative Names
Mančester, R.

Manchester, Dick

Manchester, R. N.

Manchester, R. N. (Richard N.)

Manchester, Richard N.

Манчестер, Р

Манчестер, Р. (Ричард)

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