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 10/12      Special Issue     
Ann. Geophys., 19, 1721-1730, 2001
www.ann-geophys.net/19/1721/2001/
© European Geosciences Union 2001


Cluster PEACE observations of electrons of spacecraft origin

S. Szita1, A. N. Fazakerley1, P. J. Carter1, A. M. James1, P. Trávnícek1,2, G. Watson1, M. André3, A. Eriksson3, and K. Torkar4
1Mullard Space Science Laboratory, University College London, Holmbury St Mary, Dorking, Surrey, RH5 6NT, UK
2Institute of Atmospheric Physics, Academy of Sciences of the Czech Republic
3Swedish Institute of Space Physics, Uppsala Division, Box 537, SE-75121 Uppsala, Sweden
4Space Research Institute, Austrian Academy of Sciences, Schmiedlstr. 6, 8042 Graz, Austria

Abstract. The two PEACE (Plasma Electron And Current Experiment) sensors on board each Cluster spacecraft sample the electron velocity distribution across the full 4<pi> solid angle and the energy range 0.7 eV to 26 keV with a time resolution of 4 s. We present high energy and angular resolution 3D observations of electrons of spacecraft origin in the various environments encountered by the Cluster constellation, including a lunar eclipse interval where the spacecraft potential was reduced but remained positive, and periods of ASPOC (Active Spacecraft POtential Control) operation which reduced the spacecraft potential. We demonstrate how the spacecraft potential may be found from a gradient change in the PEACE low energy spectrum, and show how the observed spacecraft electrons are confined by the spacecraft potential. We identify an intense component of the spacecraft electrons with energies equivalent to the spacecraft potential, the arrival direction of which is seen to change when ASPOC is switched on. Another spacecraft electron component, observed in the sunward direction, is reduced in the eclipse but unaffected by ASPOC, and we believe this component is produced in the analyser by solar UV. We find that PEACE anodes with a look direction along the spacecraft surfaces are more susceptible to spacecraft electron contamination than those which look perpendicular to the surface, which justifies the decision to mount PEACE with its field-of-view radially outward rather than tangentially.

Key words. Magnetosheric physics (general or miscellaneous) Space plasma physics (spacecraft sheaths, wakes, charging)


Full Article in PDF (275 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