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Planetary Radio Emissions III

Planetary Radio Emissions III
Proceedings of the 3rd International Workshop, held at Graz, Austria, September 2-4, 1991
1. Auflage, 1992
The International Workshop on Radio Emissions from Planetary Magnetospheres at Graz by now has become somewhat of a tradition. The present, third workshop was held at a time when, with the Voyager 2 flyby of Neptune the number of radio planets in our solar system has finally risen to five. This workshop, as the past ones, has provided the international community working in this discipline an opportunity to present and discuss the observational and theoretical aspects of nonthermal planetary radio emissions and their contribution as a diagnostic tool for planetary magnetospheres in general. The present volume contains edited versions of the papers presented at the workshop; its publication was again made possible through the generous support of the Austrian Academy of Sciences. The organizers and editors also wish to express their gratitude for financial support to the Austrian Space Agency (ASA), NASA, the City of Graz and the Provincial Government of Styria and especially want to thank the University of Graz for again hosting this workshop. We hope to contribute the now established tradition of the Graz workshop on planetary radio emissions at some appropriate time in the future.
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Planetary magnetic fields: Salient characteristics
Page 1 - 12
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Doing more with Jupiter´s magnetic field
Page 13 - 34
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Jovian broadband kilometric radiation: New observations from Ulysses
Page 35 - 44
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Low-frequency auroral radio emission from Jupiter: The hectometric radiation
Page 45 - 68
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Origin of Jupiter´s decametric modulation lanes
Page 69 - 90
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Lane features in Jovian hectometric radio emissions
Page 91 - 104
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Jovian Decametric Io-related source and interplanetary scintillation
Page 105 - 114
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Spectrometric observations of Jupiter S-bursts at the Observatory Lustbühel, Graz 115
Page 115 - 124
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Jovian S-emission: Decametric high sensitivity observations and model of radiation source
Page 125 - 144
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Subpulse structure of Jovian decametric S-bursts (Abstract)
Page 145 - 146
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The elliptical polarization of the Jovian decametric emission and the magnetosphere of Jupiter
Page 147 - 154
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Faraday rotation of Jupiter´s decametric radiation
Page 155 - 170
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Propagation effects influencing the observations of planetary radio emissions
Page 171 - 182
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The Ukrainian radio interferometer system URAN for studies in decametric wavelengths band (Abstract)
Page 183 - 184
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On the propagation of MeV electrons from Jupiter to the Earth
Page 185 - 198
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The AKR of the Earth: From studies inside the sources to distant observations and remote sensing
Page 199 - 216
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Regions of enhanced electron concentration in the auroral zone of the Earth magnetosphere (Abstract)
Page 217 - 218
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A programmable receiver for monitoring LF/MF/HF signals from remote sites
Page 219 - 230
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Source location of the Saturnian kilometric radiation
Page 231 - 240
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Nonthermal radio emissions from Uranus
Page 241 - 270
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Source location determination of UKR from ray tracing and emission lobe modelling
Page 271 - 280
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Neptune as a radio source
Page 281 - 290
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Methods for the localization of radio sources: Application to the smooth Neptunian kilometric radiation
Page 291 - 308
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Neptune´s smoothly varying radio emission between 600-800 kHz
Page 309 - 316
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Numerical simulations of bursty planetary radio emissions
Page 317 - 328
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Continuum radiation in planetary magnetospheres
Page 329 - 350
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Remote Sensing of auroral plasmas
Page 351 - 370
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Lightning at planets in the outer solar system
Page 371 - 390
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Lower hybrid soliton mediated radio emission
Page 391 - 404
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Conversion of upper hybrid waves into magnetospheric radiation
Page 405 - 418
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Nonlinear generation of radiation in planetary magnetospheres
Page 419 - 424
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Direction finding of electromagnetic waves: Application to planetary radio emission
Page 425 - 432
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Polarization and Riemann surfaces
Page 433 - 442
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An overview of Galileo Plasma wave observations at Venus and earth (Abstract)
Page 443 - 444
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Radio emissions associated with shock waves and a brief model of Type II solar radio bursts
Page 445 - 452
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Fine Structures of solar radio bursts and noise storms
Page 453 - 464
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Radio physics of the Sun at decametric wavelengths
Page 465 - 472
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Petschek-type reconnection at the magnetopause: A comparison of theory with data from ISEE 2 on September 11, 1979
Page 473 - 484
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Prospects for the study of planetary radio emission
Page 485 - 488
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References
Page 489 - 524
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Edition:
978-3-7001-2002-5, Print, softcover, 01.01.1992
Edition:
978-3-7001-3906-5, eBook, Digital, 01.01.1992
Edition:
1. Auflage
Pages:
534 Pages
Format:
23x15cm
Language:
English
DOI (Link to Online Edition):

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