Pulsar Radio Emission Geometry

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University of California, San Diego, Department of Applied Mechanics/Engineering Sciences, 1986 - Cone - 524 pages

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Contents

List of Figures vi
9
Abstract xi
9
2
9

17 other sections not shown

Common terms and phrases

angular beams Ap.J Arecibo Observatory Astrophys autocorrelation autocovariance average profile average pulse profile axis curvature CALIFORNIA coefficients component positions component separation conal components conal emission conal midpoint cone geometry core component correlation Cross covariance crosscorrelation curvature radiation dispersion correction DM correction drift band drifting subpulses effects estimated exponent f MHz fiducial point field axis field geometry fluctuation spectrum frequency dependence frequency mapping frequency range function higher frequencies interstellar line of sight linear polarization linearised log f(MHz longitude magnetic axis magnetic field magnetosphere mean profile micropulses microstructure modulation index neutron star Normalised intensity observed off-pulse on-pulse open field lines particle peak Phase:milliperiods plasma frequency polar cap model profile width pulsar pulsar magnetosphere pulse intensity pulse number pulse periods pulse window radiofrequency radius radius-frequency radius-to-frequency mapping Random error Relative arrival Rickett rms errors SAN DIEGO spectra stellar rotation subpulse drift subpulse separation systematic error Table UNIVERSITY

Bibliographic information

TitlePulsar Radio Emission Geometry
AuthorArun Gudalur Venkataraman
Editionreprint
PublisherUniversity of California, San Diego, Department of Applied Mechanics/Engineering Sciences, 1986
Original fromthe University of California
DigitizedFeb 25, 2011
Length524 pages
  
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