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Annales Geophysicae An interactive open-access journal of the European Geosciences Union
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Volume 25, issue 3
Ann. Geophys., 25, 755-767, 2007
https://doi.org/10.5194/angeo-25-755-2007
© Author(s) 2007. This work is distributed under
the Creative Commons Attribution 3.0 License.
Ann. Geophys., 25, 755-767, 2007
https://doi.org/10.5194/angeo-25-755-2007
© Author(s) 2007. This work is distributed under
the Creative Commons Attribution 3.0 License.

  29 Mar 2007

29 Mar 2007

Simulation study of solar wind push on a charged wire: basis of solar wind electric sail propulsion

P. Janhunen1,2 and A. Sandroos2 P. Janhunen and A. Sandroos
  • 1University of Helsinki, Department of Physical Sciences, Finland
  • 2Finnish Meteorological Institute, Space Research, Finland

Abstract. One possibility for propellantless propulsion in space is to use the momentum flux of the solar wind. A way to set up a solar wind sail is to have a set of thin long wires which are kept at high positive potential by an onboard electron gun so that the wires repel and deflect incident solar wind protons. The efficiency of this so-called electric sail depends on how large force a given solar wind exerts on a wire segment and how large electron current the wire segment draws from the solar wind plasma when kept at a given potential. We use 1-D and 2-D electrostatic plasma simulations to calculate the force and present a semitheoretical formula which captures the simulation results. We find that under average solar wind conditions at 1 AU the force per unit length is (5±1×10−8 N/m for 15 kV potential and that the electron current is accurately given by the well-known orbital motion limited (OML) theory cylindrical Langmuir probe formula. Although the force may appear small, an analysis shows that because of the very low weight of a thin wire per unit length, quite high final speeds (over 50 km/s) could be achieved by an electric sailing spacecraft using today's flight-proved components. It is possible that artificial electron heating of the plasma in the interaction region could increase the propulsive effect even further.

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