Titlebook: Sources and Scintillations; Refraction and Scatt R. Strom,P. Bo,N. Rendong Book 2001 Springer Science+Business Media Dordrecht 2001 Planet.

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Giant Radio Pulses from Pulsarshe highest rate of occurrenceof giant pulses seen from any known pulsar. Large fluctuations in the intensity levels of individualgiant pulses and in their occurrence rate per unit interval of time are seen during a single day’sobservations, as well as from one day to the next. We conclude that these

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Studying Pulsar Emission Regions Using Interstellar Scatteringmission regions of pulsars, For thepast 25 years, observers have sought to exploit this fact to learn how pulsars shine. I review thetechniques developed, and summarize measurements of size of emission regions of pulsars to date.

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Pulsar Investigation Using Interstellar Scintillation be obtained from analysis of diffractivescintillations at low frequencies. Based on refractive and diffractive scintillation of pulsars we canalso reconstruct the distribution of turbulent plasma along the line of sight, and using this analysis anew approach to pulsar distance estimation can be mad

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Looking Into Pulsar Magnetospheresnamics of the strongly magnetizedelectron-positron plasma allows separation of the magnetospheric and interstellar scattering. Themost distinctive feature of the magneto spheric scintillations is their independence of frequency.Diffractive scattering due to small scale inhomogeneities produces a sca

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Radio Intra-Day Variability: Answers and Questionsability appears to be intrinsic to thesources themselves. However, at radio wavelengths, brightness temperatures as high as 10. to10. K are encountered if the mv is intrinsic to the source. We discuss here the accumulating evidenceshowing that, at radio wavelengths where the highest brightness tempe

Cursory

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on the one hand, of Beijing Astronomical Observatory radio astronomers to organize a conference which would highlight the need for high sensitivity - as a way ofpromoting their own project to build the world‘s largest telescope (FAST) - and to a suggestion from Ron Ekers on the other. During a discu

LARK

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Scattering Of The Low Frequency Pulsar Radiationmeters. The measured dependence of τ. on dispersion measure τ.(.) =40(./100). is close to theoretically expected relation τ.(.) α ... A frequency dependenceof the scattering pulse broadening is weaker than commonly accepted τ. α v..

LVAD360

Giant Radio Pulses from Pulsarsheir occurrence rate per unit interval of time are seen during a single day’sobservations, as well as from one day to the next. We conclude that these intensity variations arelikely to be intrinsic to the pulsar.