H.O. Rucker - W.S. Kurth - P. Louarn - G. Fischer (Eds.)


Planetary Radio Emissions VII

Proceedings of the 7th International Workshop on Planetary, Solar and Heliospheric Radio Emissions held at Graz, Austria, September 15–17, 2010


Helmut Rucker
Space Research Institute, Austrian Academy of Sciences, Graz, Austria

William Kurth
Department of Physics and Astronomy, University of Iowa, Iowa City, USA

Philippe Louarn
Centre d'Etude Spatiale de Rayonnements, CNRS/Universitè Paul-Sabatier Toulouse III, Toulouse, France

Georg Fischer
Space Research Institute, Austrian Academy of Sciences, Graz, Austria




ISBN 978-3-7001-7125-6 Print Edition
ISBN 978-3-7001-7246-8 Online Edition

doi:10.1553/PRE7

2011  578 Seiten, 23x15cm, broschiert
€  79,–   

The 7th International Workshop on "Planetary, Solar and Heliospheric Radio Emissions" is the continuation of an established tradition: This PRE VII conference followed previous successful international workshops held at Graz, Austria, in 1984, 1987, 1991, 1996, 2001, and 2005. This 7th workshop in September 2010 offered again the unique opportunity to discuss the observations from Cassini at Saturn and to investigate the measurements by other spacecraft and from the ground of the Jovian, terrestrial and solar radio emissions, also including studies on radiation from exoplanetary sources.

Verlag der Österreichischen Akademie der Wissenschaften
Austrian Academy of Sciences Press
A-1011 Wien, Dr. Ignaz Seipel-Platz 2
Tel. +43-1-515 81/DW 3420, Fax +43-1-515 81/DW 3400
https://verlag.oeaw.ac.at, e-mail: verlag@oeaw.ac.at

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Planetary Radio Emissions VII


ISBN 978-3-7001-7125-6
Print Edition
ISBN 978-3-7001-7246-8
Online Edition



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doi:10.1553/PRE7s285



Thema: mathphy
H.O. Rucker - W.S. Kurth - P. Louarn - G. Fischer (Eds.)


Planetary Radio Emissions VII

Proceedings of the 7th International Workshop on Planetary, Solar and Heliospheric Radio Emissions held at Graz, Austria, September 15–17, 2010



ISBN 978-3-7001-7125-6
Print Edition
ISBN 978-3-7001-7246-8
Online Edition
doi:10.1553/PRE7

2011  578 Seiten, 23x15cm, broschiert
€  79,–   
Open access


Helmut Rucker
Space Research Institute, Austrian Academy of Sciences, Graz, Austria

William Kurth
Department of Physics and Astronomy, University of Iowa, Iowa City, USA

Philippe Louarn
Centre d'Etude Spatiale de Rayonnements, CNRS/Universitè Paul-Sabatier Toulouse III, Toulouse, France

Georg Fischer
Space Research Institute, Austrian Academy of Sciences, Graz, Austria

J. Labelle, R. R. Anderson
PDF Icon  Ground-Level Detection of Auroral Kilometric Radiation (abstract) ()
S.  285 - 286
doi:10.1553/PRE7s285

Open access

Verlag der Österreichischen Akademie der Wissenschaften

Abstract:
The Earth’s aurorae radiate away up to 1% of their energy in the form of radio waves, called Auroral Kilometric Radiation (AKR). The mechanism responsible for the emission, the electron cyclotron maser (ECM), produces similar emissions at other planets, in the solar atmosphere, and in astrophysical systems. AKR was not unambiguously identified until the 1970’s because its detection requires a suitably instrumented satellite. The ECM theory predicts radiation beamed outward that cannot penetrate the increasing magnetic field and electron density near the Earth. Nevertheless, there have been observations over the years of AKR-like radio signals detected by ground-based, rocket-borne, and low-earth orbiting satellite-borne instruments, raising the question of whether a mechanism exists by which AKR can penetrate to low altitudes. Here we show the first unambiguous evidence that AKR indeed penetrates to low altitudes on occasions. We identified three examples of AKR-like emissions detected with a ground-based radio receiver at South Pole Station, Antarctica, during a 9-day interval in July, 2004, when the Geotail satellite, monitoring AKR, had a field of view including the auroral field lines above the station. The AKR-like emissions detected at ground-level have the same frequenc–time structure as simultaneous AKR emissions detected on Geotail 115,000-190,000 km away from the Earth. Slight differences in the frequency extent of the emissions at the two locations can be explained by, for example, plasmaspheric screening of the emissions detected by Geotail. These observations represent the first coincident detections of AKR in space and on the ground. They require the existence of an as-yet unidentified mechanism to produce the ground-level emissions which are not predicted by ECM theory, they suggest that previous AKR-like emissions observed at low altitudes may indeed be AKR, and they require revision of the widely-held view that AKR is only detectable from space.

  2011/12/28 14:50:24
Object Identifier:  0xc1aa5576 0x002a1d1a
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The 7th International Workshop on "Planetary, Solar and Heliospheric Radio Emissions" is the continuation of an established tradition: This PRE VII conference followed previous successful international workshops held at Graz, Austria, in 1984, 1987, 1991, 1996, 2001, and 2005. This 7th workshop in September 2010 offered again the unique opportunity to discuss the observations from Cassini at Saturn and to investigate the measurements by other spacecraft and from the ground of the Jovian, terrestrial and solar radio emissions, also including studies on radiation from exoplanetary sources.



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Verlag der Österreichischen Akademie der Wissenschaften
Austrian Academy of Sciences Press
A-1011 Wien, Dr. Ignaz Seipel-Platz 2
Tel. +43-1-515 81/DW 3420, Fax +43-1-515 81/DW 3400
https://verlag.oeaw.ac.at, e-mail: verlag@oeaw.ac.at