2010
DOI: 10.1016/j.asr.2009.12.007
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The radiation impedance of electrodynamic tethers in a polar Jovian orbit

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Cited by 6 publications
(21 citation statements)
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References 15 publications
(18 reference statements)
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“…Tethers might be used as alternative to solve the severe power generation problem. An electrodynamic tether, which is a very long wire capable to generate the suggested power, might radiate waves to satisfy communication requirements itself (Sanchez-Torres et al, 2010). The large electromotive force produced by the tether moving in some plasma ambient near the planet generate induced current and then electric power (Sanmartin et al, 1993).…”
Section: Resultsmentioning
confidence: 99%
“…Tethers might be used as alternative to solve the severe power generation problem. An electrodynamic tether, which is a very long wire capable to generate the suggested power, might radiate waves to satisfy communication requirements itself (Sanchez-Torres et al, 2010). The large electromotive force produced by the tether moving in some plasma ambient near the planet generate induced current and then electric power (Sanmartin et al, 1993).…”
Section: Resultsmentioning
confidence: 99%
“…The Alfvén impedance Z A was determined for the first orbit and both equatorial and polar region cases. High Alfvén velocity V A found in paper 2 gives high Alfvén impedance too, because of Z A ∝ V A . Additionally, there are two contributions to the Alfvén impedance, involving logarithmic terms that depend of both tether length and contactor size.…”
Section: Introductionmentioning
confidence: 96%
“…In the present work we generalize the paper 2 work, considering the radiation impedance for both Alfvén and FM waves, and both Juno and LJO missions. Anticipating that the wave vector k will be nearly perpendicular to the ambient magnetic field in all cases considered, k ≃ k , the Doppler relation reads greatly simplifying the calculation of impedances.…”
Section: Introductionmentioning
confidence: 99%
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“…Also, maximum N 0 is typically 10 2 times smaller than at the F-layer daytime maximum, and the Alfven velocity, V A oc BQNNQ, may be up to 10 3 times greater than in LEO. This makes impedances for Fast Magneotosonic and Alfven radiations greater for Jupiter by 2 and up to 3 orders of magnitude in (14a, b), both affecting the tether-current circuit and making significant signals possible [24]. Insertion in orbit and touring the Jovian moons afterwards, which are transport applications of interest, prove possible, a tens-of-km long tape with mass a sensible fraction of the full spacecraft mass being required.…”
Section: Bare Tethers At Jupitermentioning
confidence: 99%