Space-based ultraviolet optical signatures of simulated equatorial ionospheric bubbles

Details Space-based ultraviolet optical signatures of simulated equatorial ionospheric bubbles Space-based ultraviolet optical signatures of simulated equatorial ionospheric bubbles

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001jgr...10630429k&link_type=abstract

Journal of Geophysical Research, Volume 106, Issue A12, p. 30429-30432

Physics

Ionosphere: Equatorial Ionosphere, Ionosphere: Ionospheric Irregularities, Ionosphere: Modeling And Forecasting, Ionosphere: Instruments And Techniques

Scientific paper

Space-based ultraviolet (UV) optical signatures of equatorial ionospheric bubbles have been computed from a first-principles time-dependent physical mesoscale ionospheric simulation model. We find that for nadir-viewing geometry, extreme UV signatures at 911 Å of equatorial ionospheric bubble structures contain large bite-outs in intensity, are structured over tens of kilometers scales, and are distinctly different from the signatures of the quiet ionosphere.

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