Abstract
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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