z-logo
open-access-imgOpen Access
Floating bare tether as upper atmosphere probe
Author(s) -
Sanmartin J. R.,
Charro M.,
Pelaez J.,
Tinao I.,
Elaskar S.,
Hilgers A.,
MartinezSanchez M.
Publication year - 2006
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 - 10.1029/2006ja011624
Subject(s) - plasma , physics , daytime , spacecraft , atmosphere (unit) , magnetic field , beam (structure) , ion , atmospheric sciences , environmental science , meteorology , optics , astronomy , nuclear physics , quantum mechanics
Use of a conductive bare tape electrically floating in low Earth orbit as an effective electron beam source to produce artificial auroral effects, free of problems that mar standard beams, is considered. Ambient ions impacting the tape with keV energies over most of its length liberate secondary electrons that race down the magnetic field, excite neutrals in the E layer, and result in auroral emissions. The tether would operate with both a power supply and a plasma contactor off at nighttime; power and contactor would be on at daytime for reboost. Tomographic analysis of auroral emissions from the footprint of the beam, as observed from the spacecraft, can provide density profiles of dominant neutral species in the E layer. A characteristic tether system, at altitude ∼300 km and moderate orbital inclination, would involve an aluminum tape with a length of ∼20 km, a width of ∼15 mm, and a thickness of ∼0.2 mm for a full‐system mass around 1200 kg, with two thirds going into the power subsystem.

The content you want is available to Zendy users.

Already have an account? Click here to sign in.
Having issues? You can contact us here
Accelerating Research

Address

John Eccles House
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom