Spacelab-2 plasma depletion experiments for ionospheric and radio astronomical studies

Details Spacelab-2 plasma depletion experiments for ionospheric and radio astronomical studies Spacelab-2 plasma depletion experiments for ionospheric and radio astronomical studies

Nov 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987sci...238.1260m&link_type=abstract

Science (ISSN 0036-8075), vol. 238, Nov. 27, 1987, p. 1260-1264.

Astronomy and Astrophysics

Astronomy

19

Ionospheric Ion Density, Plasma Diffusion, Radio Astronomy, Spacelab, Infrared Spectroscopy, Magnetohydrodynamic Stability

Scientific paper

The Spacelab-2 Plasma Depletion Experiments were a series of studies to examine Shuttle-induced perturbations in the ionosphere and their application to ground-based radio astronomy. The Space Shuttle Challenger fired its orbital maneuvering subsystem engines, releasing large amounts of exhaust molecules that caused the electrons and ions in earth's upper atmosphere to chemically recombine, thereby creating so-called 'ionospheric holes'. Two burns conducted over New England produced ionospheric peak depletions ranging from 25 to 50 percent, affected the ionosphere over a 200-kilometer altitude range, and covered 1 to 2 deg of latitude. Optical emissions associated with the hole spanned an area of several hundred thousand square kilometers. A third burn was conducted over a low-frequency radio observatory in Hobart, Australia, to create an 'artificial window' for ground-based observations at frequencies normally below the natural ionospheric cutoff (penetration) frequency. The Hobart experiment succeeded in making high-resolution observations at 1.7 megahertz through the induced ionospheric hole.

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