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Magnetic self‐field effects on current collection by an ionospheric bare tether
Author(s) -
Sanmartín J. R.,
Estes R. D.
Publication year - 2002
Publication title -
journal of geophysical research: space physics
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.67
H-Index - 298
eISSN - 2156-2202
pISSN - 0148-0227
DOI - 10.1029/2002ja009344
Subject(s) - current (fluid) , dimensionless quantity , physics , radius , magnetic field , electrical conductor , plasma , ohmic contact , ionosphere , field (mathematics) , electric field , atomic physics , condensed matter physics , mechanics , geophysics , thermodynamics , mathematics , electrode , quantum mechanics , computer science , pure mathematics , computer security
It was recently suggested that the magnetic field created by the current of a bare tether strongly reduces its own electron‐collection capability when a magnetic separatrix disconnecting ambient magnetized plasma from tether extends beyond its electric sheath. It is here shown that current reduction by the self‐field depends on the ratio L * / L t parameterizing bias and current profiles along the tether ( L t ≡ tether length, L * ≡ characteristic length gauging ohmic effects) and on a new dimensionless number K s involving ambient and tether parameters. Current reduction is weaker the lower K s and L * / L t , which depend critically on the type of cross section: K s varies as R 5/3 , h 2/3 R , and h 2/3 × 1/4 width for wires, round tethers conductive only in a thin layer, and thin tapes, respectively; L * varies as R 2/3 for wires and as h 2/3 for tapes and round tethers conductive in a layer ( R ≡ radius, h ≡ thickness). Self‐field effects are fully negligible for the last two types of cross sections whatever the mode of operation. In practical efficient tether systems having L * / L t low, maximum current reduction in case of wires is again negligible for power generation; for deorbiting, reduction is <1% for a 10 km tether and ∼15% for a 20 km tether. In the reboost mode there are no effects for K s below some threshold; moderate effects may occur in practical but heavy reboost‐wire systems that need no dedicated solar power.

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