Contact Disclaimer
Annales Geophysicae
Copernicus.org Home EGU Copernicus Publications Copernicus Meetings
  Home  
  General Information  
  Submission  
  Special Issues  
  Evaluation  
  Production  
  Subscription  
  Online Library  
  Recent Papers  
  Volumes and Issues  
  Special Issues  
  Topical Library  
  Library Search  
  Title and Author Search  
  Volumes and Issues      Contents of Issue 3     
Ann. Geophys., 25, 823-831, 2007
www.ann-geophys.net/25/823/2007/
© European Geosciences Union 2007


A quantitative test of Jones NTC beaming theory using CLUSTER constellation

S. Grimald1, P. M. E. Décréau1, P. Canu2, X. Suraud1, X. Vallières1, F. Darrouzet3, and C. C. Harvey4
1Laboratoire de Physique et Chimie de l'Environnement (LPCE), Orléans, France
2Centre d'Etude des Environnements Terrestre et Planétaires (CETP), Vélizy, France
3Belgian Institute for Space Aeronomy (IASB-BIRA), Brussels, Belgium
4Centre d'Etude Spatiale des Rayonnements (CESR), Toulouse, France

Abstract. Non-thermal continuum (NTC) radiation is, with auroral kilometric radiation (AKR), one of the two electromagnetic emissions generated within the Earth's magnetosphere and radiated into space. The location of the source of NTC has been sought for several decades, with only limited success. The constellation formed by the four CLUSTER spacecraft provides the possibility of triangulation in the vicinity of the source, thus allowing progress in source localisation, while simultaneously revealing the beaming properties of NTC radio sources.

We present a case event showing two beams localised on opposite sides of the magnetic equator. At any selected frequency, triangulation points to a single region source of small size. Its position is compatible with the range of possible loci of sources predicted by the radio window theory of Jones (1982) in a frame of constraints relaxed from the simple sketch proposed in early works. The analysis of similar observations from the Dynamics Explorer 1 by Jones et al. (1987) enabled the authors to claim validation of the radio window theory. CLUSTER observations, however, reveal a large beaming cone angle projected onto the ecliptic plane, a feature unobservable by Dynamics Explorer which had a different spin axis orientation. According to the radio window theory, such a large observed cone angle can only be formed by a series of point sources, each beaming in a narrow cone angle. This study demonstrates the difficulty of validating NTC linear generation mechanisms using global beaming properties alone.


Full Article in PDF (2323 KB)
  Library Search ANGEO  
       
  Special Services  
  Printer-friendly Version  
  Bookmark  
  Download Acrobat Reader  
  News  
  ISI Impact Factor: 1.427 (2007)
 
Annales Geophysicae is launching a new section: AnGeo Communicates
 
© Copernicus 2004–2006